This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461120.6870,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.1870 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:04:36.09 +71:33:20.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.52 05:24:32.24 +69:38:27.5
142.82559 18.23340 galactic Cam Second-epoch detections are separated by 1.1" and 3.6 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 | 05:24:32.24 +69:38:27.5 (user input) | T | P | (position from user input) J-Ks=0.330+/-0.041 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461120.6870,13.52,0.05,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 20260321.1870 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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:24:32.24 +69:38:27.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.59 04:19:02.82 +69:20:51.4
139.51554 13.47408 galactic Cam Second-epoch detections are separated by 2.8" and 3.5 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 496892261195893120 | 04:18:54.28 +69:20:57.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.559+/-0.045 (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 496892261195893120,2461120.6870,13.59,0.05,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 496892261195893120 20260321.1870 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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:19:02.82 +69:20:51.4 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.61 04:57:16.02 +73:02:51.4
138.57317 18.19050 galactic Cam Second-epoch detections are separated by 0.7" and 3.2 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 | 04:57:16.02 +73:02:51.4 (user input) | T | P | (position from user input) J-Ks=0.490+/-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,2461120.6870,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.1870 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:57:16.02 +73:02:51.4 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.57 04:33:03.45 +69:49:44.5
139.99711 14.70098 galactic Cam Second-epoch detections are separated by 2.2" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:33:03.45 +69:49:44.5 (user input) | T | P | (position from user input) J-Ks=0.473+/-0.038 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461120.6870,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.1870 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:33:03.45 +69:49:44.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_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,2461120.6870,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.1870 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:05:53.75 +69:33:17.2 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_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,2461120.6870,13.35,0.05,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 20260321.1870 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:01:49.86 +70:06:53.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.35 06:20:35.55 +72:57:45.6
141.40995 23.63963 galactic Cam Second-epoch detections are separated by 1.6" and 3.4 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 | 06:20:35.55 +72:57:45.6 (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,2461120.6870,13.35,0.05,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 20260321.1870 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:20:35.55 +72:57:45.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.20 05:21:25.28 +71:32:27.7
140.94708 18.94542 galactic Cam Second-epoch detections are separated by 1.2" and 3.6 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 | 05:21:25.28 +71:32:27.7 (user input) | T | P | (position from user input) J-Ks=0.319+/-0.038 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461120.6870,13.20,0.05,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 20260321.1870 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:21:25.28 +71:32:27.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_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,2461120.6870,13.33,0.05,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 20260321.1870 13.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:32:12.99 +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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_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,2461120.6870,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.1870 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:18:16.06 +66:05:23.4 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_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,2461120.6870,13.05,0.05,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 20260321.1870 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:38:01.11 +66:00:41.1 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.31 04:24:13.63 +70:35:39.2
138.89274 14.65121 galactic Cam Second-epoch detections are separated by 1.8" and 3.2 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 | 04:24:13.63 +70:35:39.2 (user input) | T | P | (position from user input) J-Ks=0.458+/-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,2461120.6870,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.1870 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:13.63 +70:35:39.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 12.88 05:14:20.56 +69:52:36.6
142.14087 17.59423 galactic Cam Second-epoch detections are separated by 5.2" and 3.5 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 | NSVS J0514205+695157 | 05:14:20.26 +69:51:56.2 (Gaia DR3) | L: (local) | 124.000000000000 (local) | Gaia3var=VARIABLE SpType: M6/7 2012MNRAS.419.3346G FBS 0508+698
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0514205+695157,2461120.6870,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0514205+695157 20260321.1870 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:14:20.56 +69:52:36.6 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 12.83 05:13:00.03 +68:41:27.9
143.12823 16.86571 galactic Cam Second-epoch detections are separated by 1.7" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:13:00.03 +68:41:27.9 (user input) | T | P | (position from user input) J-Ks=0.380+/-0.038 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461120.6870,12.83,0.05,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 20260321.1870 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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:13:00.03 +68:41:27.9 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J034340.87+680408.2,2461120.6870,12.96,0.05,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
ASASSN-V J034340.87+680408.2 20260321.1870 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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:43:43.33 +68:04:22.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 12.32 04:38:14.21 +70:27:31.8
139.79197 15.44313 galactic Cam Second-epoch detections are separated by 1.6" and 3.2 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 | 04:38:14.21 +70:27:31.8 (user input) | T | P | (position from user input) J-Ks=0.417+/-0.035 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461120.6870,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.1870 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:38:14.21 +70:27:31.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0418017+711356,2461120.6870,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0418017+711356 20260321.1870 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:18:01.09 +71:13:56.3 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 12.04 03:58:02.50 +65:53:36.8
140.46288 9.59570 galactic Cam Second-epoch detections are separated by 1.6" and 3.6 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 489831747279814400 | 03:58:06.32 +65:53:34.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.555+/-0.034 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 489831747279814400,2461120.6870,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 489831747279814400 20260321.1870 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:58:02.50 +65:53:36.8 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 11.97 03:45:59.28 +68:33:52.8
137.81378 10.89769 galactic Cam Second-epoch detections are separated by 2.2" 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 | Gaia DR3 493644475648586496 | 03:46:03.62 +68:34:10.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.333+/-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
Gaia DR3 493644475648586496,2461120.6870,11.97,0.05,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 493644475648586496 20260321.1870 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:45:59.28 +68:33:52.8 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 11.53 04:05:44.49 +69:16:49.5
138.70539 12.60120 galactic Cam Second-epoch detections are separated by 0.9" and 3.5 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 493935979369184384 | 04:05:40.89 +69:16:44.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.887+/-0.025 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 493935979369184384,2461120.6870,11.53,0.05,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 493935979369184384 20260321.1870 11.53CV 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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:05:44.49 +69:16:49.5 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 10.48 03:59:23.96 +65:26:37.4
140.86970 9.34897 galactic Cam Second-epoch detections are separated by 0.4" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 489055728288597504 | 03:59:24.04 +65:26:37.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.310+/-0.027 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 489055728288597504,2461120.6870,10.48,0.05,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
Gaia DR3 489055728288597504 20260321.1870 10.48CV 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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:59:23.96 +65:26:37.4 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 11.12 04:54:16.93 +73:02:38.9
138.44500 18.01017 galactic Cam Second-epoch detections are separated by 0.2" and 3.3 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 500930110271622528 | 04:54:17.15 +73:02:38.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.875+/-0.029 (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 500930110271622528,2461120.6870,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 500930110271622528 20260321.1870 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:54:16.93 +73:02:38.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 11.29 04:00:27.51 +68:34:40.2
138.83299 11.76247 galactic Cam Second-epoch detections are separated by 2.1" and 3.6 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 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 493787098621550976,2461120.6870,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 493787098621550976 20260321.1870 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:00:27.51 +68:34:40.2 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 12.03 04:26:19.32 +74:06:02.1
136.29227 17.11389 galactic Cam Second-epoch detections are separated by 0.6" 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 | 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+74.0978,2461120.6870,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J066.5612+74.0978 20260321.1870 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:26:19.32 +74:06:02.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 12.10 03:49:46.57 +66:14:45.6
139.58306 9.32461 galactic Cam Second-epoch detections are separated by 1.2" and 3.6 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 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 490079549712449664,2461120.6870,12.10,0.05,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
Gaia DR3 490079549712449664 20260321.1870 12.10CV 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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:49:46.57 +66:14:45.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 12.23 04:10:08.79 +68:21:09.3
139.65523 12.20299 galactic Cam Second-epoch detections are separated by 0.7" and 3.6 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 | 04:10:08.79 +68:21:09.3 (user input) | T | P | (position from user input) J-Ks=0.231+/-0.034 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461120.6870,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.1870 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:10:08.79 +68:21:09.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 12.28 03:56:30.26 +68:51:28.1
138.36902 11.73464 galactic Cam Second-epoch detections are separated by 0.7" and 3.5 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 | 03:56:30.26 +68:51:28.1 (user input) | T | P | (position from user input) J-Ks=0.494+/-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,2461120.6870,12.28,0.05,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 20260321.1870 12.28CV 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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:56:30.26 +68:51:28.1 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 12.29 04:28:40.27 +74:01:13.3
136.46648 17.18272 galactic Cam Second-epoch detections are separated by 0.6" and 3.2 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 501969531014011136 | 04:28:34.83 +74:01:43.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.361+/-0.032 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 501969531014011136,2461120.6870,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 501969531014011136 20260321.1870 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:28:40.27 +74:01:13.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 12.54 03:57:23.86 +71:25:01.7
136.69427 13.70629 galactic Cam Second-epoch detections are separated by 0.6" and 3.2 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 495284156721043456,2461120.6870,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 495284156721043456 20260321.1870 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:57:23.86 +71:25:01.7 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 12.61 04:27:18.61 +71:47:16.4
138.14780 15.63583 galactic Cam Second-epoch detections are separated by 0.3" and 3.3 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 500429214005075328 | 04:27:22.92 +71:47:49.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.431+/-0.037 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 500429214005075328,2461120.6870,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 500429214005075328 20260321.1870 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:27:18.61 +71:47:16.4 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_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,2461120.6870,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.1870 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:50:16.29 +72:56:17.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 12.70 04:50:22.39 +72:53:49.4
138.39472 17.69197 galactic Cam Second-epoch detections are separated by 1.7" and 3.4 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 | 04:50:22.39 +72:53:49.4 (user input) | T | P | (position from user input) J-Ks=0.853+/-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,2461120.6870,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.1870 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:50:22.39 +72:53:49.4 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_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,2461120.6870,12.84,0.05,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 20260321.1870 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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:56:31.08 +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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_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 501569652378642560,2461120.6870,12.87,0.05,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
Gaia DR3 501569652378642560 20260321.1870 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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:23:02.74 +73:36:55.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_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,2461120.6870,12.89,0.05,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 20260321.1870 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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:16:55.60 +69:09:49.6 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_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,2461120.6870,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.1870 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:31:57.95 +73:36:35.2 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_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,2461120.6870,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.1870 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:59:57.60 +74:15:19.6 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_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 490870476528554496,2461120.6870,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 490870476528554496 20260321.1870 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:16:23.60 +68:59:10.4 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_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 495224336415689728,2461120.6870,13.10,0.05,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
Gaia DR3 495224336415689728 20260321.1870 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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:50:02.10 +71:09:27.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 12.98 04:20:01.37 +68:13:25.4
140.40969 12.75813 galactic Cam Second-epoch detections are separated by 3.6" and 3.9 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 | NSVS J0420083+681348 | 04:20:08.76 +68:13:47.2 (Gaia DR3) | L: (local) | 111.000000000000 (local) | Gaia3var=VARIABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0420083+681348,2461120.6870,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0420083+681348 20260321.1870 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:20:01.37 +68:13:25.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.17 04:03:35.35 +73:53:16.2
135.31827 15.83849 galactic Cam Second-epoch detections are separated by 1.7" 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 | Large-amplitude variable Gaia DR2 549771245708847616 | 04:03:35.35 +73:53:16.2 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.430+/-0.036 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 549771245708847616,2461120.6870,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 549771245708847616 20260321.1870 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:03:35.35 +73:53:16.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.04 04:14:47.78 +68:29:36.4
139.86646 12.60302 galactic Cam Second-epoch detections are separated by 2.2" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 490781038127204608 | 04:14:42.98 +68:29:07.2 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=1.073+/-0.031 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 490781038127204608,2461120.6870,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 490781038127204608 20260321.1870 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:14:47.78 +68:29:36.4 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_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,2461120.6870,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.1870 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:45:28.73 +74:16:15.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.31 03:53:26.08 +65:59:37.1
140.03517 9.36665 galactic Cam Second-epoch detections are separated by 0.9" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:53:26.08 +65:59:37.1 (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,2461120.6870,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.1870 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:53:26.08 +65:59:37.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 12.93 05:14:11.77 +67:27:38.8
144.27555 16.30266 galactic Cam Second-epoch detections are separated by 1.8" and 3.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:14:11.77 +67:27:38.8 (user input) | T | P | (position from user input) J-Ks=0.355+/-0.035 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461120.6870,12.93,0.05,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 20260321.1870 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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:14:11.77 +67:27:38.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J051555.95+703407.7,2461120.6870,13.10,0.05,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
ZTF J051555.95+703407.7 20260321.1870 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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:15:56.62 +70:34:25.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.27 04:49:15.17 +71:09:23.8
139.80392 16.58594 galactic Cam Second-epoch detections are separated by 2.2" and 3.7 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 | 04:49:15.17 +71:09:23.8 (user input) | T | P | (position from user input) J-Ks=0.435+/-0.086 (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,2461120.6870,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.1870 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:49:15.17 +71:09:23.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_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 502153974090205056,2461120.6870,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 502153974090205056 20260321.1870 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:01:54.86 +72:32:10.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J041944.96+713510.4,2461120.6870,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J041944.96+713510.4 20260321.1870 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:19:44.63 +71:35:09.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_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 496326425025087744,2461120.6870,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 496326425025087744 20260321.1870 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:47:41.42 +69:27:49.6 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_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,2461120.6870,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.1870 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:01:41.20 +70:12:59.8 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.52 03:57:02.42 +65:33:01.0
140.61183 9.26884 galactic Cam Second-epoch detections are separated by 1.4" and 4.0 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 | 03:57:02.42 +65:33:01.0 (user input) | T | P | (position from user input) J-Ks=0.600+/-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,2461120.6870,13.52,0.05,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 20260321.1870 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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:57:02.42 +65:33:01.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.47 03:55:46.78 +71:26:45.2
136.57533 13.64256 galactic Cam Second-epoch detections are separated by 1.9" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:55:46.78 +71:26:45.2 (user input) | T | P | (position from user input) J-Ks=0.541+/-0.058 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461120.6870,13.47,0.05,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 20260321.1870 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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:55:46.78 +71:26:45.2 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.48 03:53:27.41 +67:28:19.7
139.06949 10.49856 galactic Cam Second-epoch detections are separated by 2.2" and 3.4 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 | 03:53:27.41 +67:28:19.7 (user input) | T | P | (position from user input) J-Ks=0.575+/-0.033 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461120.6870,13.48,0.05,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 20260321.1870 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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:53:27.41 +67:28:19.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.64 04:00:25.53 +72:21:14.7
136.22734 14.55964 galactic Cam Second-epoch detections are separated by 1.6" and 3.4 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 | 04:00:25.53 +72:21:14.7 (user input) | T | P | (position from user input) J-Ks=0.521+/-0.064 (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,2461120.6870,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.1870 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:00:25.53 +72:21:14.7 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.51 03:46:42.55 +68:52:22.3
137.66892 11.17885 galactic Cam Second-epoch detections are separated by 2.9" and 3.2 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 493668286945488384 | 03:46:36.64 +68:51:49.0 (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 493668286945488384,2461120.6870,13.51,0.05,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
Gaia DR3 493668286945488384 20260321.1870 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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:46:42.55 +68:52:22.3 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.38 04:37:06.45 +72:47:26.4
137.85618 16.85315 galactic Cam Second-epoch detections are separated by 1.3" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:37:06.45 +72:47:26.4 (user input) | T | P | (position from user input) J-Ks=0.421+/-0.041 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461120.6870,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.1870 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:37:06.45 +72:47:26.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 489917887142564224,2461120.6870,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 489917887142564224 20260321.1870 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:02:25.42 +66:01:49.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.62 04:01:23.92 +70:57:53.8
137.25233 13.58645 galactic Cam Second-epoch detections are separated by 0.8" and 3.4 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 | 04:01:23.92 +70:57:53.8 (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,2461120.6870,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.1870 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:01:23.92 +70:57:53.8 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.41 04:57:48.03 +69:48:33.5
141.37756 16.36879 galactic Cam Second-epoch detections are separated by 1.2" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:57:48.03 +69:48:33.5 (user input) | T | P | (position from user input) J-Ks=0.430+/-0.049 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461120.6870,13.41,0.05,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 20260321.1870 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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:57:48.03 +69:48:33.5 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.66 04:34:11.51 +71:53:50.0
138.42645 16.11283 galactic Cam Second-epoch detections are separated by 1.2" and 3.4 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 | 04:34:11.51 +71:53:50.0 (user input) | T | P | (position from user input) J-Ks=0.441+/-0.048 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461120.6870,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.1870 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:34:11.51 +71:53:50.0 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.68 03:57:19.80 +70:44:20.3
137.15276 13.19532 galactic Cam Second-epoch detections are separated by 1.4" 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 | 03:57:19.80 +70:44:20.3 (user input) | T | P | (position from user input) J-Ks=0.458+/-0.035 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461120.6870,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.1870 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:57:19.80 +70:44:20.3 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.61 04:03:06.81 +66:46:17.9
140.25698 10.59015 galactic Cam Second-epoch detections are separated by 1.9" and 4.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:03:06.81 +66:46:17.9 (user input) | T | P | (position from user input) J-Ks=0.457+/-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,2461120.6870,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.1870 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:03:06.81 +66:46:17.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.62 05:45:34.69 +71:22:41.0
142.02533 20.58294 galactic Cam Second-epoch detections are separated by 2.3" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:45:34.69 +71:22:41.0 (user input) | T | P | (position from user input) J-Ks=0.608+/-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,2461120.6870,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.1870 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:45:34.69 +71:22:41.0 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.43 05:24:15.26 +73:29:09.8
139.25183 20.07462 galactic Cam Second-epoch detections are separated by 2.7" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:24:15.26 +73:29:09.8 (user input) | T | P | (position from user input) J-Ks=0.416+/-0.042 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461120.6870,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.1870 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:24:15.26 +73:29:09.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_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,2461120.6870,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.1870 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:13.93 +73:13:57.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.64 03:51:13.06 +68:31:52.7
138.21235 11.17463 galactic Cam Second-epoch detections are separated by 2.0" and 3.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:51:13.06 +68:31:52.7 (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,2461120.6870,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.1870 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:13.06 +68:31:52.7 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_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 490036806196542208,2461120.6870,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 490036806196542208 20260321.1870 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:00:49.42 +66:52:15.9 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_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,2461120.6870,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.1870 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:36:54.55 +73:15:54.2 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_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 501205885829264640,2461120.6870,13.53,0.05,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 501205885829264640 20260321.1870 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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:03.30 +72:08:32.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.52 05:46:20.36 +71:28:21.1
141.95973 20.67691 galactic Cam Second-epoch detections are separated by 1.4" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:46:20.36 +71:28:21.1 (user input) | T | P | (position from user input) J-Ks=0.405+/-0.042 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461120.6870,13.52,0.05,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 20260321.1870 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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:46:20.36 +71:28:21.1 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.60 04:31:42.81 +67:24:28.7
141.79218 13.01594 galactic Cam Second-epoch detections are separated by 1.9" and 3.5 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 | 04:31:42.81 +67:24:28.7 (user input) | T | P | (position from user input) J-Ks=0.519+/-0.044 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461120.6870,13.60,0.05,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 20260321.1870 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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:31:42.81 +67:24:28.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.52 04:15:10.03 +69:56:55.9
138.83055 13.65260 galactic Cam Second-epoch detections are separated by 0.8" and 3.6 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 | 04:15:10.03 +69:56:55.9 (user input) | T | P | (position from user input) J-Ks=0.740+/-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,2461120.6870,13.52,0.05,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 20260321.1870 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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:15:10.03 +69:56:55.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_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,2461120.6870,13.65,0.05,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 20260321.1870 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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:43:02.44 +68:11:54.8 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.47 04:32:38.20 +65:48:34.9
143.07986 12.02461 galactic Cam Second-epoch detections are separated by 2.3" and 4.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:32:38.20 +65:48:34.9 (user input) | T | P | (position from user input) J-Ks=0.804+/-0.028 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461120.6870,13.47,0.05,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 20260321.1870 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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:32:38.20 +65:48:34.9 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.77 04:05:28.99 +71:05:14.3
137.41689 13.90213 galactic Cam Second-epoch detections are separated by 2.7" 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 | 04:05:28.99 +71:05:14.3 (user input) | T | P | (position from user input) J-Ks=0.594+/-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,2461120.6870,13.77,0.05,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 20260321.1870 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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:05:28.99 +71:05:14.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.79 04:26:54.86 +72:11:01.4
137.81930 15.87596 galactic Cam Second-epoch detections are separated by 0.8" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:26:54.86 +72:11:01.4 (user input) | T | P | (position from user input) J-Ks=0.493+/-0.051 (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,2461120.6870,13.79,0.05,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 20260321.1870 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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:26:54.86 +72:11:01.4 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.72 04:35:52.87 +71:02:49.1
139.19349 15.66934 galactic Cam Second-epoch detections are separated by 1.4" and 3.5 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 | 04:35:52.87 +71:02:49.1 (user input) | T | P | (position from user input) J-Ks=0.453+/-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,2461120.6870,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.1870 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:35:52.87 +71:02:49.1 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_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+685943,2461120.6870,13.77,0.05,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
WISE J042521.6+685943 20260321.1870 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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:25:21.46 +68:59:43.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.70 04:40:47.91 +70:18:41.0
140.05155 15.51643 galactic Cam Second-epoch detections are separated by 1.6" and 3.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:40:47.91 +70:18:41.0 (user input) | T | P | (position from user input) J-Ks=0.703+/-0.034 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461120.6870,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.1870 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:40:47.91 +70:18:41.0 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.58 05:07:01.64 +73:43:55.6
138.37570 19.14956 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 | 05:07:01.64 +73:43:55.6 (user input) | T | P | (position from user input) J-Ks=0.557+/-0.038 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461120.6870,13.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.1870 13.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:07:01.64 +73:43:55.6 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.79 05:37:31.53 +73:12:18.2
139.97841 20.79522 galactic Cam Second-epoch detections are separated by 1.7" 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 | 05:37:31.53 +73:12:18.2 (user input) | T | P | (position from user input) J-Ks=0.480+/-0.044 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461120.6870,13.79,0.05,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 20260321.1870 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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:37:31.53 +73:12:18.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.71 04:58:39.11 +66:34:11.9
144.15806 14.54715 galactic Cam Second-epoch detections are separated by 2.9" and 3.6 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 | 04:58:39.11 +66:34:11.9 (user input) | T | P | (position from user input) J-Ks=0.788+/-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,2461120.6870,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.1870 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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:58:39.11 +66:34:11.9 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 21.1870 2461120.6870 13.72 06:05:41.68 +73:23:53.3
140.60897 22.74049 galactic Cam Second-epoch detections are separated by 2.9" 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 | 06:05:41.68 +73:23:53.3 (user input) | T | P | (position from user input) J-Ks=0.469+/-0.053 (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,2461120.6870,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260321.1870 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:05:41.68 +73:23:53.3 ;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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_fits__*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_2026-03-20_23-29-29_20_00sec_-14_90C_LIGHT_0161_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_2026-03-20_23-28-41_20_00sec_-15_00C_LIGHT_0160_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: 2461120.68726816 21.03.2026 04:29:29.969 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.62
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 14446
Objects passed selection criteria: 14430
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: 13340.2
Average stars matched: 12832.5 (96.1938 %)
Memory usage VmPeak: 119312 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Fri Mar 20 15:05:04 CDT 2026
VaST build number 1.0rc88-352-gfa78ed9d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 20 23:36:25 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: 2461120.68726816 21.03.2026 04:29:29.969 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 445
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: 53 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): 99079
Objects passed selection criteria: 98840
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: 89936.2
Average stars matched: 86251.8 (95.9032 %)
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 Fri Mar 20 15:05:04 CDT 2026
VaST build number 1.0rc88-352-gfa78ed9d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 20 23:38:25 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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.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: 2461120.68670719
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits exists and is non-empty
Saving wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits to local_wcs_cache/
'wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits' -> 'local_wcs_cache/wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits'
wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits exists and is non-empty
Saving wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits to local_wcs_cache/
'wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits' -> 'local_wcs_cache/wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits'
wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits exists and is non-empty
Saving wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits to local_wcs_cache/
'wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits' -> 'local_wcs_cache/wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits'
wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits exists and is non-empty
Saving wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits to local_wcs_cache/
'wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits' -> 'local_wcs_cache/wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.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 04:47:27.309 +70:03:12.83
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 04:47:23.362 +70:03:07.82
Angular distance between the image centers 0.06 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 04:47:27.309 +70:03:12.83
Second-epoch second image center 04:47:23.362 +70:03:07.82
Angular distance between the image centers 0.00578 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.fu00tUn1NH
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.1jELxd0jRN
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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits &> /tmp/tmp.T8kx9sSycU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits &> /tmp/tmp.3sQNXarFH1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.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_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits
2.5 pix fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.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_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits
15.0 mag. fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.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 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.fu00tUn1NH (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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/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.1jELxd0jRN (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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/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.T8kx9sSycU (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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits
Checking if the catalog wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.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_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits
WCS catalog name: wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=963, passed=15355
Got 15355 stars (including 14382 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits.cat
util/solve_plate_with_UCAC5 got 15355 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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: 0.49"
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_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits -region wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.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.3sQNXarFH1 (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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits
Checking if the catalog wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.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_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits
WCS catalog name: wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1015, passed=15252
Got 15252 stars (including 14224 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits.cat
util/solve_plate_with_UCAC5 got 15252 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
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 971 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: 0.50"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits -region wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/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_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits'
Saving fully-calibrated image wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.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__out21378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21412.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21446.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21496.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21513.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21527.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_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 20882_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
**** FOUND 05:20:16.48 +71:34:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 0.507 498147899176343808 080.06874604936 +71.56802807925 11.8661 11.1532 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.507#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21378_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 21378_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
**** FOUND 04:37:53.96 +71:27:16.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 0.476 500535802212355456 069.47518647410 +71.45454129490 11.9885 11.5352 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.476#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21412_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 21412_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
**** FOUND 04:50:20.57 +68:09:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 0.246 495967984234117504 072.58584113756 +68.15164736946 12.0959 11.3506 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.246#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21446_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 21446_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
**** FOUND 05:15:02.71 +73:00:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.335 499272768290947328 078.76097407482 +73.01458988992 12.0140 11.2520 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.335#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21496_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 21496_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
**** FOUND 04:58:28.92 +70:11:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.430 496466986416075008 074.62084971996 +70.19715214814 12.1331 11.6663 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.430#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21513_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 21513_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
**** FOUND 04:52:33.26 +69:03:26.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.620 496085769416751744 073.13874825646 +69.05725488567 12.1207 11.4710 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.620#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21527_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 21527_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
**** FOUND 05:11:09.20 +70:03:60.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 0.476 497727817015043456 077.78817496843 +70.06654604345 12.3278 11.9209 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.476#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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.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_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits
Creating symlink local_wcs_cache/wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.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_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits exists and is non-empty
wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.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 04:47:27.309 +70:03:12.83
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 04:47:23.362 +70:03:07.82
Angular distance between the image centers 0.06 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 04:47:27.309 +70:03:12.83
Second-epoch second image center 04:47:23.362 +70:03:07.82
Angular distance between the image centers 0.00578 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.USXx3UY9WM
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.FWCxNDsMM7
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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits &> /tmp/tmp.oQrlZa6mcG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits &> /tmp/tmp.84fGf1zRMJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.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 349 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_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits
2.4 pix fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.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_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits
13.9 mag. fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 13.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.USXx3UY9WM (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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/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.FWCxNDsMM7 (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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/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.oQrlZa6mcG (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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits
Checking if the catalog wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.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_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits
WCS catalog name: wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=27, blended=7504, passed=89341
Got 89341 stars (including 81710 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits.cat
util/solve_plate_with_UCAC5 got 89341 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 966 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: 0.51"
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 967 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: 0.48"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits -region wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.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.84fGf1zRMJ (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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits
Checking if the catalog wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.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_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits
WCS catalog name: wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=7549, passed=91073
Got 91073 stars (including 83400 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits.cat
util/solve_plate_with_UCAC5 got 91073 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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: 0.51"
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 968 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: 0.50"
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_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits -region wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/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_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-28-41_20.00sec_-15.00C_LIGHT_0160.fits
Saving fully-calibrated image wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.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_2026-03-20_CI_Cam-06-Q2b1x1_233024_TTUQ2b1x1_32525_jXsro0Yf/wcs_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161.fits
Preparing the HTML report for the field Cam-06-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out131920.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out131969.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out131986.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132005.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132006.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132011.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132019.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134227.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135998.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out136075.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out136202.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out136287.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out136318.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out131939.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131940.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131941.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131942.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131943.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131949.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131955.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131967.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131970.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131972.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131974.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131976.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131979.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131991.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131996.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132004.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132008.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132010.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132013.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132016.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132018.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132020.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132657.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132720.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133365.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133465.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133587.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133591.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133666.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133927.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133985.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134040.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134151.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134402.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134418.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134461.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134484.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134694.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134846.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134848.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134900.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134964.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134982.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135247.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135284.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135286.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135512.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135531.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135554.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135576.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135589.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135773.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135789.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135865.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135881.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135901.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135915.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135920.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135950.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135974.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135994.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135995.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135999.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136037.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136078.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136102.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136106.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136134.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136137.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136164.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136182.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136184.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136200.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136201.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136220.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136233.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136257.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136258.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136297.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136333.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136361.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136444.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136510.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136529.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 121s
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: 53s
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Considering the candidate 131920_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 131920_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
**** FOUND 04:53:47.74 +65:49:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 0.888 482359706775462016 073.44933786887 +65.82025981794 14.3360 13.5093 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.888#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 131939_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 131939_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 131940_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 131940_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131941_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 131941_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 131942_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 131942_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 131943_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 131943_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 131949_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 131949_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 131955_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 131955_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 131956_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 131956_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 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 131967_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 131967_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 131969_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 131969_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
**** FOUND 04:08:29.35 +70:08:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 0.407 494185675885332736 062.12245588325 +70.14623738611 14.2849 13.3625 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.407#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 131970_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 131970_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 131972_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 131972_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 131974_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 131974_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 131976_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 131976_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 131979_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 131979_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 131986_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 131986_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
**** FOUND 03:47:18.77 +68:09:15.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 1.218 493572388916360960 056.82905424231 +68.15423695971 14.0478 13.1474 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.218#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 131991_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 131991_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 131996_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 131996_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 131999_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 131999_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 132004_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 132004_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 132005_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 132005_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
**** FOUND 03:41:17.09 +68:14:57.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 1.440 493550570481294336 055.32221297133 +68.24942435779 13.7600 12.8067 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.440#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 132006_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 132006_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
**** FOUND 03:53:01.97 +65:49:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 0.809 489865591620990336 058.25821679420 +65.82621976557 13.3800 12.3463 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.809#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 132008_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 132008_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132010_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 132010_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 132011_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 132011_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
**** FOUND 03:48:56.96 +65:32:21.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 0.578 488357027307740544 057.23722571476 +65.53912352695 13.0320 11.8593 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.578#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 132013_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 132013_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 132015_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 132015_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
**** FOUND 05:52:27.89 +70:32:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 132016_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 132016_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 132018_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 132018_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 132019_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 132019_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
**** FOUND 03:44:31.93 +68:53:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.15, MAG_FAINT_SEARCH_LIMIT=12.13)GAIADR2_OUTPUT=# 0.730 494414713602469888 056.13282875078 +68.88592332499 11.8909 10.8650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.730#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 132020_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 132020_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 132533_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 132533_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 132617_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 132617_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 132657_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 132657_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132710_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 132710_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132717_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 132717_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 132720_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 132720_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132766_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 132766_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132783_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 132783_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 132797_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 132797_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132815_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 132815_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132875_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 132875_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132879_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 132879_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
**** FOUND 04:13:40.81 +72:09:24.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 132881_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 132881_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132886_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 132886_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132893_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 132893_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132918_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 132918_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132932_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 132932_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 132983_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 132983_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132992_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 132992_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133006_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133006_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 133012_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133012_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 133022_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133022_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133032_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133032_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133047_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133047_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133050_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133050_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133085_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133085_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133094_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133094_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (23.6") between the two second-epoch detections
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Considering the candidate 133098_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133098_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133103_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133103_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133152_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133152_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 133161_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133161_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133203_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133203_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133222_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133222_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133245_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133245_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133255_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133255_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (23.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133268_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133268_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133346_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133346_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133357_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133357_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133365_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 133365_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133385_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133385_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133388_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133388_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133392_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133392_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133417_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133417_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133419_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133419_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133431_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133431_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133448_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133448_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133465_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 133465_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133505_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133505_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133515_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133515_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133517_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133517_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133526_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133526_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133550_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133550_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133587_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 133587_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133591_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 133591_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133598_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133598_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133616_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133616_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133638_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133638_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133661_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133661_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133663_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133663_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133666_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 133666_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133675_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133675_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133690_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133690_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133697_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133697_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133766_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133766_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
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Considering the candidate 133770_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133770_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 133779_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133779_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 133780_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133780_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 133810_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133810_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 133825_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133825_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (24.1") between the two second-epoch detections
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Considering the candidate 133828_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133828_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (23.7") between the two second-epoch detections
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Considering the candidate 133876_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133876_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 133885_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133885_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 133906_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133906_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
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Considering the candidate 133927_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 133927_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 133960_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 133960_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 133985_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 133985_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 134019_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134019_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 134033_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134033_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 134040_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 134040_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 134048_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134048_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
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Considering the candidate 134052_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134052_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (23.6") between the two second-epoch detections
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Considering the candidate 134055_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134055_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 134103_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134103_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 134119_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134119_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
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Considering the candidate 134128_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134128_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 134141_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134141_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 134151_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 134151_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 134152_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134152_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 134172_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134172_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 134179_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134179_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 134197_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134197_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 134200_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134200_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 134202_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134202_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 134210_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134210_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 134212_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134212_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 134227_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134227_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
**** FOUND 04:17:16.37 +66:57:58.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 2.969 489701042833419648 064.31682306768 +66.96573963736 12.3157 10.3326 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.969#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134258_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134258_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 134276_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134276_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
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Considering the candidate 134298_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134298_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 134307_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134307_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 134308_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134308_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
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Considering the candidate 134312_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134312_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 134316_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134316_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (23.4") between the two second-epoch detections
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Considering the candidate 134319_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134319_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
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Considering the candidate 134362_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134362_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 134399_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134399_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
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Considering the candidate 134402_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 134402_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134408_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134408_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134418_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 134418_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134446_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134446_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 134461_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 134461_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134483_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134483_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 134484_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 134484_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134504_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134504_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134531_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134531_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 134547_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134547_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 134558_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134558_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
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Considering the candidate 134608_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134608_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 134615_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134615_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134621_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134621_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134632_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134632_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 134636_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134636_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134640_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134640_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 134642_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134642_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 134681_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134681_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 134686_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134686_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 134694_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 134694_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 134697_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134697_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 134716_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134716_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 134725_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134725_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 134728_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134728_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 134733_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134733_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
**** FOUND 04:55:32.97 +66:54:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 134744_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134744_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 134745_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134745_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
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Considering the candidate 134752_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134752_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 134754_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134754_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
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Considering the candidate 134784_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134784_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 134786_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134786_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 134791_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134791_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 134803_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134803_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 134804_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134804_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 134810_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134810_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
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Considering the candidate 134845_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134845_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 134846_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 134846_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 134848_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 134848_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 134853_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 134853_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 134879_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134879_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
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Considering the candidate 134884_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134884_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 134891_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134891_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 134894_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134894_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.9") between the two second-epoch detections
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Considering the candidate 134900_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 134900_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 134916_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134916_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 134917_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134917_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
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Considering the candidate 134919_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134919_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.9") between the two second-epoch detections
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Considering the candidate 134925_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134925_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 134936_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134936_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
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Considering the candidate 134964_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 134964_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 134971_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134971_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 134982_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 134982_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 134996_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 134996_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 135012_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135012_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
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Considering the candidate 135033_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135033_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 135068_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135068_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 135073_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135073_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 135084_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135084_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 135088_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135088_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 135107_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135107_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (24.0") between the two second-epoch detections
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Considering the candidate 135124_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135124_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 135139_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135139_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 135159_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135159_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 135183_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135183_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
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Considering the candidate 135210_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135210_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135223_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135223_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135226_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135226_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 135228_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135228_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 135236_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135236_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (23.7") between the two second-epoch detections
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Considering the candidate 135244_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135244_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135247_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 135247_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135284_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 135284_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135286_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 135286_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135306_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135306_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 135323_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135323_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 135324_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135324_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 135344_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135344_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 135353_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135353_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 135360_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135360_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 135368_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135368_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 135424_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135424_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 135429_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135429_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
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Considering the candidate 135443_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135443_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 135484_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135484_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (23.6") between the two second-epoch detections
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Considering the candidate 135495_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135495_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (23.0") between the two second-epoch detections
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Considering the candidate 135496_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135496_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 135512_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 135512_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 135531_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 135531_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 135541_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135541_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 135554_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 135554_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 135556_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135556_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 135572_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135572_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
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Considering the candidate 135576_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 135576_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 135582_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135582_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 135589_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 135589_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 135626_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135626_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 135637_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135637_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 135638_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135638_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
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Considering the candidate 135666_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135666_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
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Considering the candidate 135669_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135669_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
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Considering the candidate 135680_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135680_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 135701_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135701_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 135707_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135707_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 135714_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135714_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 135715_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135715_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 135724_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135724_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
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Considering the candidate 135747_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135747_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 135766_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135766_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 135773_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 135773_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 135781_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135781_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 135789_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 135789_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 135802_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135802_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 135812_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135812_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 135816_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135816_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 135845_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135845_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 135852_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135852_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 135855_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135855_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 135857_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135857_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 135859_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135859_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 135865_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 135865_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135869_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135869_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 135881_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 135881_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 135895_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135895_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 135901_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 135901_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135912_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135912_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 135915_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 135915_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 135916_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135916_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 135920_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 135920_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135931_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135931_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 135933_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135933_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135942_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135942_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135950_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 135950_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 135974_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 135974_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 135994_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 135994_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135995_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 135995_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 135998_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 135998_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
**** FOUND 04:03:17.81 +65:30:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 0.742 489136100015514240 060.82469204865 +65.50364747065 14.4786 13.3441 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.742#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135999_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 135999_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136014_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136014_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 136024_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136024_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 136037_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 136037_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 136048_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136048_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (23.8") between the two second-epoch detections
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Considering the candidate 136052_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136052_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 136062_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136062_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 136065_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136065_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 136072_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136072_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 136074_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136074_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 136075_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136075_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
**** FOUND 03:51:34.95 +65:23:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 0.691 489837416635996928 057.89582782613 +65.39596637669 14.2935 13.1166 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.691#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 136077_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136077_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 136078_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 136078_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136082_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136082_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 136102_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 136102_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136104_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136104_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 136106_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 136106_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 136134_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 136134_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 136137_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 136137_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136164_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 136164_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136171_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136171_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 136179_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136179_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 136182_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 136182_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 136184_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 136184_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136192_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136192_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 136193_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136193_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 136200_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 136200_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136201_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 136201_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
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Considering the candidate 136202_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136202_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
**** FOUND 03:48:04.32 +68:12:25.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 1.719 493574347421415296 057.01916667667 +68.20728455154 14.5286 13.6605 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.719#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 136203_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136203_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 136206_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136206_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 136220_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 136220_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136221_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136221_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 136233_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 136233_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136235_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136235_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136243_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136243_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 136257_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 136257_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136258_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 136258_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136263_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136263_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 136269_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136269_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (23.7") between the two second-epoch detections
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Considering the candidate 136272_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136272_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 136287_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136287_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
**** FOUND 04:12:01.86 +69:32:11.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 1.716 493955637436367232 063.00738969218 +69.53601244593 14.7315 14.0700 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.716#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 136297_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 136297_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136313_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136313_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 136314_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136314_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 136317_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136317_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136318_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136318_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
**** FOUND 04:09:32.90 +67:08:45.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 1.714 490364460661824384 062.38810030451 +67.14629341569 14.5131 13.5144 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.714#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136323_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136323_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 136333_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 136333_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136349_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136349_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136361_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 136361_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136381_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136381_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136383_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136383_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136388_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136388_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136408_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136408_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136428_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136428_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136434_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136434_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 136439_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136439_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136444_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 136444_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136445_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136445_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 136446_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136446_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
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Considering the candidate 136450_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136450_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
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Considering the candidate 136459_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136459_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 136464_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136464_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (23.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136480_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136480_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136495_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136495_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136510_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 136510_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136526_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136526_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136529_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
Preparing report for the candidate 136529_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136538_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136538_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136539_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 136539_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112822_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 112822_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131793_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 131793_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (22.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10857_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161
The candidate 10857_fd_Cam-06-Q2b1x1_2026-03-20_23-29-29_20.00sec_-14.90C_LIGHT_0161 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 14s
make_report_in_HTML.sh TOTAL: 188s
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 ####
04:04:36.09 +71:33:20.2
05:24:32.24 +69:38:27.5
04:19:02.82 +69:20:51.4
04:57:16.02 +73:02:51.4
04:33:03.45 +69:49:44.5
06:05:53.75 +69:33:17.2
05:01:49.86 +70:06:53.6
06:20:35.55 +72:57:45.6
05:21:25.28 +71:32:27.7
04:32:12.99 +69:46:34.3
05:18:16.06 +66:05:23.4
04:38:01.11 +66:00:41.1
04:24:13.63 +70:35:39.2
05:14:20.56 +69:52:36.6
05:13:00.03 +68:41:27.9
03:43:43.33 +68:04:22.1
04:38:14.21 +70:27:31.8
04:18:01.09 +71:13:56.3
03:58:02.50 +65:53:36.8
03:45:59.28 +68:33:52.8
04:05:44.49 +69:16:49.5
03:59:23.96 +65:26:37.4
04:54:16.93 +73:02:38.9
04:00:27.51 +68:34:40.2
04:26:19.32 +74:06:02.1
03:49:46.57 +66:14:45.6
04:10:08.79 +68:21:09.3
03:56:30.26 +68:51:28.1
04:28:40.27 +74:01:13.3
03:57:23.86 +71:25:01.7
04:27:18.61 +71:47:16.4
04:50:16.29 +72:56:17.8
04:50:22.39 +72:53:49.4
04:56:31.08 +72:51:35.0
04:23:02.74 +73:36:55.4
04:16:55.60 +69:09:49.6
04:31:57.95 +73:36:35.2
04:59:57.60 +74:15:19.6
04:16:23.60 +68:59:10.4
03:50:02.10 +71:09:27.0
04:20:01.37 +68:13:25.4
04:03:35.35 +73:53:16.2
04:14:47.78 +68:29:36.4
04:45:28.73 +74:16:15.1
03:53:26.08 +65:59:37.1
05:14:11.77 +67:27:38.8
05:15:56.62 +70:34:25.9
04:49:15.17 +71:09:23.8
05:01:54.86 +72:32:10.6
04:19:44.63 +71:35:09.3
04:47:41.42 +69:27:49.6
04:01:41.20 +70:12:59.8
03:57:02.42 +65:33:01.0
03:55:46.78 +71:26:45.2
03:53:27.41 +67:28:19.7
04:00:25.53 +72:21:14.7
03:46:42.55 +68:52:22.3
04:37:06.45 +72:47:26.4
04:02:25.42 +66:01:49.3
04:01:23.92 +70:57:53.8
04:57:48.03 +69:48:33.5
04:34:11.51 +71:53:50.0
03:57:19.80 +70:44:20.3
04:03:06.81 +66:46:17.9
05:45:34.69 +71:22:41.0
05:24:15.26 +73:29:09.8
05:58:13.93 +73:13:57.9
03:51:13.06 +68:31:52.7
04:00:49.42 +66:52:15.9
04:36:54.55 +73:15:54.2
04:24:03.30 +72:08:32.3
05:46:20.36 +71:28:21.1
04:31:42.81 +67:24:28.7
04:15:10.03 +69:56:55.9
03:43:02.44 +68:11:54.8
04:32:38.20 +65:48:34.9
04:05:28.99 +71:05:14.3
04:26:54.86 +72:11:01.4
04:35:52.87 +71:02:49.1
04:25:21.46 +68:59:43.5
04:40:47.91 +70:18:41.0
05:07:01.64 +73:43:55.6
05:37:31.53 +73:12:18.2
04:58:39.11 +66:34:11.9
06:05:41.68 +73:23:53.3
########### Completed Cam-06-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
04:04:36.09 +71:33:20.2
05:24:32.24 +69:38:27.5
04:19:02.82 +69:20:51.4
04:57:16.02 +73:02:51.4
04:33:03.45 +69:49:44.5
06:05:53.75 +69:33:17.2
05:01:49.86 +70:06:53.6
06:20:35.55 +72:57:45.6
05:21:25.28 +71:32:27.7
04:32:12.99 +69:46:34.3
05:18:16.06 +66:05:23.4
04:38:01.11 +66:00:41.1
04:24:13.63 +70:35:39.2
05:14:20.56 +69:52:36.6
05:13:00.03 +68:41:27.9
03:43:43.33 +68:04:22.1
04:38:14.21 +70:27:31.8
04:18:01.09 +71:13:56.3
03:58:02.50 +65:53:36.8
03:45:59.28 +68:33:52.8
04:05:44.49 +69:16:49.5
03:59:23.96 +65:26:37.4
04:54:16.93 +73:02:38.9
04:00:27.51 +68:34:40.2
04:26:19.32 +74:06:02.1
03:49:46.57 +66:14:45.6
04:10:08.79 +68:21:09.3
03:56:30.26 +68:51:28.1
04:28:40.27 +74:01:13.3
03:57:23.86 +71:25:01.7
04:27:18.61 +71:47:16.4
04:50:16.29 +72:56:17.8
04:50:22.39 +72:53:49.4
04:56:31.08 +72:51:35.0
04:23:02.74 +73:36:55.4
04:16:55.60 +69:09:49.6
04:31:57.95 +73:36:35.2
04:59:57.60 +74:15:19.6
04:16:23.60 +68:59:10.4
03:50:02.10 +71:09:27.0
04:20:01.37 +68:13:25.4
04:03:35.35 +73:53:16.2
04:14:47.78 +68:29:36.4
04:45:28.73 +74:16:15.1
03:53:26.08 +65:59:37.1
05:14:11.77 +67:27:38.8
05:15:56.62 +70:34:25.9
04:49:15.17 +71:09:23.8
05:01:54.86 +72:32:10.6
04:19:44.63 +71:35:09.3
04:47:41.42 +69:27:49.6
04:01:41.20 +70:12:59.8
03:57:02.42 +65:33:01.0
03:55:46.78 +71:26:45.2
03:53:27.41 +67:28:19.7
04:00:25.53 +72:21:14.7
03:46:42.55 +68:52:22.3
04:37:06.45 +72:47:26.4
04:02:25.42 +66:01:49.3
04:01:23.92 +70:57:53.8
04:57:48.03 +69:48:33.5
04:34:11.51 +71:53:50.0
03:57:19.80 +70:44:20.3
04:03:06.81 +66:46:17.9
05:45:34.69 +71:22:41.0
05:24:15.26 +73:29:09.8
05:58:13.93 +73:13:57.9
03:51:13.06 +68:31:52.7
04:00:49.42 +66:52:15.9
04:36:54.55 +73:15:54.2
04:24:03.30 +72:08:32.3
05:46:20.36 +71:28:21.1
04:31:42.81 +67:24:28.7
04:15:10.03 +69:56:55.9
03:43:02.44 +68:11:54.8
04:32:38.20 +65:48:34.9
04:05:28.99 +71:05:14.3
04:26:54.86 +72:11:01.4
04:35:52.87 +71:02:49.1
04:25:21.46 +68:59:43.5
04:40:47.91 +70:18:41.0
05:07:01.64 +73:43:55.6
05:37:31.53 +73:12:18.2
04:58:39.11 +66:34:11.9
06:05:41.68 +73:23:53.3
###################################################################################
04:04:36.09 +71:33:20.2 -- not an asteroid (will add it to exclusion list)
05:24:32.24 +69:38:27.5 -- not an asteroid (will add it to exclusion list)
04:19:02.82 +69:20:51.4 -- not an asteroid (will add it to exclusion list)
04:57:16.02 +73:02:51.4 -- not an asteroid (will add it to exclusion list)
04:33:03.45 +69:49:44.5 -- not an asteroid (will add it to exclusion list)
06:05:53.75 +69:33:17.2 -- not an asteroid (will add it to exclusion list)
05:01:49.86 +70:06:53.6 -- not an asteroid (will add it to exclusion list)
06:20:35.55 +72:57:45.6 -- not an asteroid (will add it to exclusion list)
05:21:25.28 +71:32:27.7 -- not an asteroid (will add it to exclusion list)
04:32:12.99 +69:46:34.3 -- not an asteroid (will add it to exclusion list)
05:18:16.06 +66:05:23.4 -- not an asteroid (will add it to exclusion list)
04:38:01.11 +66:00:41.1 -- not an asteroid (will add it to exclusion list)
04:24:13.63 +70:35:39.2 -- not an asteroid (will add it to exclusion list)
05:14:20.56 +69:52:36.6 -- not an asteroid (will add it to exclusion list)
05:13:00.03 +68:41:27.9 -- not an asteroid (will add it to exclusion list)
03:43:43.33 +68:04:22.1 -- not an asteroid (will add it to exclusion list)
04:38:14.21 +70:27:31.8 -- not an asteroid (will add it to exclusion list)
04:18:01.09 +71:13:56.3 -- not an asteroid (will add it to exclusion list)
03:58:02.50 +65:53:36.8 -- not an asteroid (will add it to exclusion list)
03:45:59.28 +68:33:52.8 -- not an asteroid (will add it to exclusion list)
04:05:44.49 +69:16:49.5 -- not an asteroid (will add it to exclusion list)
03:59:23.96 +65:26:37.4 -- not an asteroid (will add it to exclusion list)
04:54:16.93 +73:02:38.9 -- not an asteroid (will add it to exclusion list)
04:00:27.51 +68:34:40.2 -- not an asteroid (will add it to exclusion list)
04:26:19.32 +74:06:02.1 -- not an asteroid (will add it to exclusion list)
03:49:46.57 +66:14:45.6 -- not an asteroid (will add it to exclusion list)
04:10:08.79 +68:21:09.3 -- not an asteroid (will add it to exclusion list)
03:56:30.26 +68:51:28.1 -- not an asteroid (will add it to exclusion list)
04:28:40.27 +74:01:13.3 -- not an asteroid (will add it to exclusion list)
03:57:23.86 +71:25:01.7 -- not an asteroid (will add it to exclusion list)
04:27:18.61 +71:47:16.4 -- not an asteroid (will add it to exclusion list)
04:50:16.29 +72:56:17.8 -- not an asteroid (will add it to exclusion list)
04:50:22.39 +72:53:49.4 -- not an asteroid (will add it to exclusion list)
04:56:31.08 +72:51:35.0 -- not an asteroid (will add it to exclusion list)
04:23:02.74 +73:36:55.4 -- not an asteroid (will add it to exclusion list)
04:16:55.60 +69:09:49.6 -- not an asteroid (will add it to exclusion list)
04:31:57.95 +73:36:35.2 -- not an asteroid (will add it to exclusion list)
04:59:57.60 +74:15:19.6 -- not an asteroid (will add it to exclusion list)
04:16:23.60 +68:59:10.4 -- not an asteroid (will add it to exclusion list)
03:50:02.10 +71:09:27.0 -- not an asteroid (will add it to exclusion list)
04:20:01.37 +68:13:25.4 -- not an asteroid (will add it to exclusion list)
04:03:35.35 +73:53:16.2 -- not an asteroid (will add it to exclusion list)
04:14:47.78 +68:29:36.4 -- not an asteroid (will add it to exclusion list)
04:45:28.73 +74:16:15.1 -- not an asteroid (will add it to exclusion list)
03:53:26.08 +65:59:37.1 -- not an asteroid (will add it to exclusion list)
05:14:11.77 +67:27:38.8 -- not an asteroid (will add it to exclusion list)
05:15:56.62 +70:34:25.9 -- not an asteroid (will add it to exclusion list)
04:49:15.17 +71:09:23.8 -- not an asteroid (will add it to exclusion list)
05:01:54.86 +72:32:10.6 -- not an asteroid (will add it to exclusion list)
04:19:44.63 +71:35:09.3 -- not an asteroid (will add it to exclusion list)
04:47:41.42 +69:27:49.6 -- not an asteroid (will add it to exclusion list)
04:01:41.20 +70:12:59.8 -- not an asteroid (will add it to exclusion list)
03:57:02.42 +65:33:01.0 -- not an asteroid (will add it to exclusion list)
03:55:46.78 +71:26:45.2 -- not an asteroid (will add it to exclusion list)
03:53:27.41 +67:28:19.7 -- not an asteroid (will add it to exclusion list)
04:00:25.53 +72:21:14.7 -- not an asteroid (will add it to exclusion list)
03:46:42.55 +68:52:22.3 -- not an asteroid (will add it to exclusion list)
04:37:06.45 +72:47:26.4 -- not an asteroid (will add it to exclusion list)
04:02:25.42 +66:01:49.3 -- not an asteroid (will add it to exclusion list)
04:01:23.92 +70:57:53.8 -- not an asteroid (will add it to exclusion list)
04:57:48.03 +69:48:33.5 -- not an asteroid (will add it to exclusion list)
04:34:11.51 +71:53:50.0 -- not an asteroid (will add it to exclusion list)
03:57:19.80 +70:44:20.3 -- not an asteroid (will add it to exclusion list)
04:03:06.81 +66:46:17.9 -- not an asteroid (will add it to exclusion list)
05:45:34.69 +71:22:41.0 -- not an asteroid (will add it to exclusion list)
05:24:15.26 +73:29:09.8 -- not an asteroid (will add it to exclusion list)
05:58:13.93 +73:13:57.9 -- not an asteroid (will add it to exclusion list)
03:51:13.06 +68:31:52.7 -- not an asteroid (will add it to exclusion list)
04:00:49.42 +66:52:15.9 -- not an asteroid (will add it to exclusion list)
04:36:54.55 +73:15:54.2 -- not an asteroid (will add it to exclusion list)
04:24:03.30 +72:08:32.3 -- not an asteroid (will add it to exclusion list)
05:46:20.36 +71:28:21.1 -- not an asteroid (will add it to exclusion list)
04:31:42.81 +67:24:28.7 -- not an asteroid (will add it to exclusion list)
04:15:10.03 +69:56:55.9 -- not an asteroid (will add it to exclusion list)
03:43:02.44 +68:11:54.8 -- not an asteroid (will add it to exclusion list)
04:32:38.20 +65:48:34.9 -- not an asteroid (will add it to exclusion list)
04:05:28.99 +71:05:14.3 -- not an asteroid (will add it to exclusion list)
04:26:54.86 +72:11:01.4 -- not an asteroid (will add it to exclusion list)
04:35:52.87 +71:02:49.1 -- not an asteroid (will add it to exclusion list)
04:25:21.46 +68:59:43.5 -- not an asteroid (will add it to exclusion list)
04:40:47.91 +70:18:41.0 -- not an asteroid (will add it to exclusion list)
05:07:01.64 +73:43:55.6 -- not an asteroid (will add it to exclusion list)
05:37:31.53 +73:12:18.2 -- not an asteroid (will add it to exclusion list)
04:58:39.11 +66:34:11.9 -- not an asteroid (will add it to exclusion list)
06:05:41.68 +73:23:53.3 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
03:43:02.44 +68:11:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:43:43.33 +68:04:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:45:59.28 +68:33:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:46:42.55 +68:52:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:49:46.57 +66:14:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:50:02.10 +71:09:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:13.06 +68:31:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:53:26.08 +65:59:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:53:27.41 +67:28:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:55:46.78 +71:26:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:56:30.26 +68:51:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:57:02.42 +65:33:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:57:19.80 +70:44:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:57:23.86 +71:25:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:58:02.50 +65:53:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:59:23.96 +65:26:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:00:25.53 +72:21:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:00:27.51 +68:34:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:00:49.42 +66:52:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:01:23.92 +70:57:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:01:41.20 +70:12:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:02:25.42 +66:01:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:03:06.81 +66:46:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:03:35.35 +73:53:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:04:36.09 +71:33:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:05:28.99 +71:05:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:05:44.49 +69:16:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:10:08.79 +68:21:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:14:47.78 +68:29:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:15:10.03 +69:56:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:16:23.60 +68:59:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:16:55.60 +69:09:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:18:01.09 +71:13:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:19:02.82 +69:20:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:19:44.63 +71:35:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:20:01.37 +68:13:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:23:02.74 +73:36:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:03.30 +72:08:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:13.63 +70:35:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:25:21.46 +68:59:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:26:19.32 +74:06:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:26:54.86 +72:11:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:27:18.61 +71:47:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:28:40.27 +74:01:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:31:42.81 +67:24:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:31:57.95 +73:36:35.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:32:12.99 +69:46:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:32:38.20 +65:48:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:33:03.45 +69:49:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:34:11.51 +71:53:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:35:52.87 +71:02:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:36:54.55 +73:15:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:37:06.45 +72:47:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:38:01.11 +66:00:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:38:14.21 +70:27:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:40:47.91 +70:18:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:45:28.73 +74:16:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:47:41.42 +69:27:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:49:15.17 +71:09:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:50:16.29 +72:56:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:50:22.39 +72:53:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:16.93 +73:02:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:31.08 +72:51:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:16.02 +73:02:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:48.03 +69:48:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:39.11 +66:34:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:57.60 +74:15:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:49.86 +70:06:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:54.86 +72:32:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:01.64 +73:43:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:13:00.03 +68:41:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:14:11.77 +67:27:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:14:20.56 +69:52:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:15:56.62 +70:34:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:16.06 +66:05:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:25.28 +71:32:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:24:15.26 +73:29:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:24:32.24 +69:38:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:31.53 +73:12:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:34.69 +71:22:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:20.36 +71:28:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:13.93 +73:13:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:05:41.68 +73:23:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:05:53.75 +69:33:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:35.55 +72:57:45.6 -- 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)
03:43:02.44 +68:11:54.8 -- not a known variable star
03:43:43.33 +68:04:22.1 -- a known variable star
03:45:59.28 +68:33:52.8 -- not a known variable star
03:46:42.55 +68:52:22.3 -- not a known variable star
03:49:46.57 +66:14:45.6 -- not a known variable star
03:50:02.10 +71:09:27.0 -- a known variable star
03:51:13.06 +68:31:52.7 -- not a known variable star
03:53:26.08 +65:59:37.1 -- not a known variable star
03:53:27.41 +67:28:19.7 -- not a known variable star
03:55:46.78 +71:26:45.2 -- not a known variable star
03:56:30.26 +68:51:28.1 -- not a known variable star
03:57:02.42 +65:33:01.0 -- not a known variable star
03:57:19.80 +70:44:20.3 -- not a known variable star
03:57:23.86 +71:25:01.7 -- not a known variable star
03:58:02.50 +65:53:36.8 -- not a known variable star
03:59:23.96 +65:26:37.4 -- not a known variable star
04:00:25.53 +72:21:14.7 -- not a known variable star
04:00:27.51 +68:34:40.2 -- not a known variable star
04:00:49.42 +66:52:15.9 -- a known variable star
04:01:23.92 +70:57:53.8 -- not a known variable star
04:01:41.20 +70:12:59.8 -- not a known variable star
04:02:25.42 +66:01:49.3 -- a known variable star
04:03:06.81 +66:46:17.9 -- not a known variable star
04:03:35.35 +73:53:16.2 -- not a known variable star
04:04:36.09 +71:33:20.2 -- not a known variable star
04:05:28.99 +71:05:14.3 -- not a known variable star
04:05:44.49 +69:16:49.5 -- not a known variable star
04:10:08.79 +68:21:09.3 -- not a known variable star
04:14:47.78 +68:29:36.4 -- not a known variable star
04:15:10.03 +69:56:55.9 -- not a known variable star
04:16:23.60 +68:59:10.4 -- a known variable star
04:16:55.60 +69:09:49.6 -- not a known variable star
04:18:01.09 +71:13:56.3 -- a known variable star
04:19:02.82 +69:20:51.4 -- not a known variable star
04:19:44.63 +71:35:09.3 -- a known variable star
04:20:01.37 +68:13:25.4 -- not a known variable star
04:23:02.74 +73:36:55.4 -- a known variable star
04:24:03.30 +72:08:32.3 -- a known variable star
04:24:13.63 +70:35:39.2 -- not a known variable star
04:25:21.46 +68:59:43.5 -- a known variable star
04:26:19.32 +74:06:02.1 -- not a known variable star
04:26:54.86 +72:11:01.4 -- not a known variable star
04:27:18.61 +71:47:16.4 -- not a known variable star
04:28:40.27 +74:01:13.3 -- not a known variable star
04:31:42.81 +67:24:28.7 -- not a known variable star
04:31:57.95 +73:36:35.2 -- not a known variable star
04:32:12.99 +69:46:34.3 -- not a known variable star
04:32:38.20 +65:48:34.9 -- not a known variable star
04:33:03.45 +69:49:44.5 -- not a known variable star
04:34:11.51 +71:53:50.0 -- not a known variable star
04:35:52.87 +71:02:49.1 -- not a known variable star
04:36:54.55 +73:15:54.2 -- not a known variable star
04:37:06.45 +72:47:26.4 -- not a known variable star
04:38:01.11 +66:00:41.1 -- not a known variable star
04:38:14.21 +70:27:31.8 -- not a known variable star
04:40:47.91 +70:18:41.0 -- not a known variable star
04:45:28.73 +74:16:15.1 -- not a known variable star
04:47:41.42 +69:27:49.6 -- a known variable star
04:49:15.17 +71:09:23.8 -- not a known variable star
04:50:16.29 +72:56:17.8 -- not a known variable star
04:50:22.39 +72:53:49.4 -- not a known variable star
04:54:16.93 +73:02:38.9 -- not a known variable star
04:56:31.08 +72:51:35.0 -- not a known variable star
04:57:16.02 +73:02:51.4 -- not a known variable star
04:57:48.03 +69:48:33.5 -- not a known variable star
04:58:39.11 +66:34:11.9 -- not a known variable star
04:59:57.60 +74:15:19.6 -- not a known variable star
05:01:49.86 +70:06:53.6 -- not a known variable star
05:01:54.86 +72:32:10.6 -- a known variable star
05:07:01.64 +73:43:55.6 -- not a known variable star
05:13:00.03 +68:41:27.9 -- not a known variable star
05:14:11.77 +67:27:38.8 -- not a known variable star
05:14:20.56 +69:52:36.6 -- not a known variable star
05:15:56.62 +70:34:25.9 -- a known variable star
05:18:16.06 +66:05:23.4 -- not a known variable star
05:21:25.28 +71:32:27.7 -- not a known variable star
05:24:15.26 +73:29:09.8 -- not a known variable star
05:24:32.24 +69:38:27.5 -- not a known variable star
05:37:31.53 +73:12:18.2 -- not a known variable star
05:45:34.69 +71:22:41.0 -- not a known variable star
05:46:20.36 +71:28:21.1 -- not a known variable star
05:58:13.93 +73:13:57.9 -- not a known variable star
06:05:41.68 +73:23:53.3 -- not a known variable star
06:05:53.75 +69:33:17.2 -- not a known variable star
06:20:35.55 +72:57:45.6 -- not a known variable star
Found 72 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
85 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 85 (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)2461120.68670719 -observatory 500
22:37:46.77 -07:41:21.0 Mercury (1.0mag)
01:07:25.52 +06:14:34.6 Venus (-3.9mag)
23:03:42.77 -07:10:54.2 Mars (1.2mag)
07:04:47.32 +22:57:58.9 Jupiter (-2.3mag)
00:17:26.06 -00:25:37.4 Saturn (0.9mag)
03:42:57.83 +19:31:58.2 Uranus (5.8mag)
00:07:18.96 -00:37:52.1 Neptune (7.8mag)
20:32:01.33 -22:53:46.2 Pluto (14.5mag)
01:39:31.14 +14:37:54.2 Moon (-8.8mag)
-rw-r--r-- 1 apache apache 361 Mar 20 23:36 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461120.68670719:
07:04:52.96 +22:57:46.0 Io (5.6mag)
07:04:33.63 +22:58:25.6 Europa (5.7mag)
07:04:25.68 +22:58:37.7 Ganymede (5.2mag)
07:04:11.08 +22:59:01.5 Callisto (6.4mag)
07:08:48.60 +22:59:29.2 Himalia (15.2mag)
07:04:50.66 +22:57:54.1 Thebe (16.0mag)
07:08:23.68 +23:22:51.0 Elara (17.2mag)
07:01:56.06 +23:51:33.9 Pasiphae (17.2mag)
07:13:34.61 +22:52:28.3 Carme (18.3mag)
00:17:20.77 -00:25:33.8 Titan (8.8mag)
00:17:31.32 -00:25:36.2 Rhea (10.1mag)
00:17:55.63 -00:23:34.7 Iapetus (11.5mag)
00:17:41.23 -00:25:42.4 Hyperion (14.8mag)
00:19:20.10 -00:14:22.1 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Mar 20 23:36 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461120.68670719:
12:51:27.24 +08:39:26.1 JWST
16:24:44.07 +48:22:14.9 Chandra
08:00:22.52 -30:36:14.8 XMM-Newton
-rw-r--r-- 1 apache apache 96 Mar 20 23:36 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461120.68670719 -observatory 500
18:35:34.33 -27:28:12.3 14.1mag P/2010 H2 (Vales)
04:51:14.87 -71:01:21.6 17.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:28:44.62 +31:17:56.1 17.0mag C/2017 K2 (PANSTARRS)
17:29:39.97 +07:25:38.8 17.6mag C/2021 G2 (ATLAS)
23:01:37.94 +28:26:22.1 16.9mag C/2022 E2 (ATLAS)
04:00:41.19 +25:17:58.3 15.7mag C/2022 N2 (PANSTARRS)
09:01:52.04 +31:27:23.3 16.0mag C/2022 QE78 (ATLAS)
08:30:10.49 -03:09:13.6 17.2mag C/2022 R6 (PANSTARRS)
18:56:30.07 +16:18:27.6 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:46:20.41 -11:50:38.5 17.6mag P/2023 B1 (PANSTARRS)
09:24:22.30 -16:17:41.9 17.4mag C/2023 F3 (ATLAS)
21:21:58.77 +61:42:10.1 17.4mag C/2023 H5 (Lemmon)
19:33:09.32 -03:31:15.7 14.5mag C/2023 R1 (PANSTARRS)
21:36:31.85 +82:52:19.1 17.7mag C/2023 X2 (Lemmon)
06:15:19.96 +63:47:00.5 16.8mag C/2024 A1 (ATLAS)
04:07:00.46 +05:20:34.6 9.1mag C/2024 E1 (Wierzchos)
11:22:28.98 +02:46:03.7 18.0mag C/2024 G2 (ATLAS)
16:32:12.77 +02:11:38.3 17.5mag C/2024 G6 (ATLAS)
20:10:09.47 +08:48:24.7 14.9mag C/2024 J3 (ATLAS)
03:04:50.63 -26:37:14.7 16.5mag C/2024 T5 (ATLAS)
04:57:38.72 +52:32:46.5 17.6mag C/2025 J1 (Borisov)
15:13:16.92 +17:43:07.9 14.4mag C/2025 L1 (ATLAS)
02:48:45.40 -22:36:08.1 17.6mag C/2025 Q3 (ATLAS)
22:33:01.95 +19:01:40.1 12.5mag C/2025 R3 (PANSTARRS)
13:04:59.81 +01:19:28.1 17.6mag C/2025 Y1 (ATLAS)
02:09:19.96 -06:15:00.6 14.1mag C/2026 A1 (MAPS)
22:39:32.67 +31:05:59.4 13.7mag C/2026 B2 (Sun-Gao)
17:52:26.35 -10:50:10.0 13.3mag 10P/Tempel
15:26:42.30 +05:07:39.7 11.8mag 24P/Schaumasse
11:11:55.09 -02:28:26.1 15.6mag 29P/Schwassmann-Wachmann
17:43:51.59 -10:38:19.1 17.3mag 40P/Vaisala
10:45:03.00 -06:32:50.4 16.4mag 43P/Wolf-Harrington
01:09:14.35 +12:57:24.0 17.0mag 47P/Ashbrook-Jackson
06:28:49.94 +42:18:43.2 17.1mag 63P/Wild
22:54:27.68 -14:43:04.0 15.7mag 65P/Gunn
02:58:53.54 +11:23:59.8 15.9mag 76P/West-Kohoutek-Ikemura
00:09:54.40 +03:05:08.7 14.6mag 78P/Gehrels
21:39:23.51 -16:41:43.8 14.5mag 88P/Howell
01:01:13.91 +13:16:55.5 15.2mag 93P/Lovas
04:10:52.61 +30:41:50.7 16.5mag 123P/West-Hartley
08:07:49.80 +50:10:58.5 16.2mag 124P/Mrkos
01:54:36.33 +11:22:34.8 16.4mag 128P/Shoemaker-Holt
01:57:45.12 +11:03:34.3 17.4mag 131P/Mueller
23:20:54.74 +03:10:22.5 12.9mag 141P/Machholz
23:31:01.68 -04:22:21.7 13.0mag 141P-A/Machholz
22:31:39.78 -06:55:47.4 16.1mag 141P-D/Machholz
23:50:55.25 -14:03:45.5 15.5mag 162P/SidingSpring
10:39:13.17 +32:02:05.4 17.5mag 164P/Christensen
05:50:02.66 +24:44:12.5 17.5mag 198P/ODAS
15:33:06.97 -03:20:54.5 16.9mag 210P/Christensen
20:12:32.76 -17:30:28.5 17.2mag 218P/LINEAR
16:59:28.50 -16:39:37.7 16.3mag 235P/LINEAR
04:41:47.55 +32:01:26.4 16.3mag 240P/NEAT
07:29:54.48 -08:20:53.6 17.5mag 242P/Spahr
15:48:34.08 +05:07:04.7 17.7mag 391P/Kowalski
07:28:00.41 +21:06:38.0 17.5mag 450P/LONEOS
05:01:10.78 +46:36:17.9 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K Mar 20 23:36 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
11:44:44.19 -62:10:45.50 ASASSN-26bq 2026-03-15.03 15.31
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 -0.22
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
00:12:55.45 +33:21:25.90 SN2026cbh 2026-02-7.09 16.33
08:02:12.64 -04:14:20.90 SN 2026auh 2026-02-7.11 16.64
18:03:52.67 -31:27:26.00 TCP J18035290-3127298 2026-02-7.37 15.76
12:18:03.59 +50:27:10.20 SN 2026bjz 2026-02-7.25 16.48
07:51:51.12 +55:05:27.60 SN 2026ail 2026-02-6.21 16.85
08:10:56.38 +36:49:42.80 AT2026bsa 2026-02-6.29 17.47
04:43:45.47 -15:49:01.00 SN2026azr 2026-02-5.24 16.96
06:14:48.48 -34:20:08.90 ASASSN-26ap 2026-02-5.2 13.77
02:42:33.90 -27:21:02.60 SN 2026aip 2026-02-4.09 15.85
00:43:12.26 +38:35:47.90 AT2026brt 2026-02-3.12 14.92
14:34:27.21 +21:56:59.90 SN2026atb 2026-01-29.32 15.59
13:12:04.11 -60:56:12.40 ASASSN-26ao 2026-01-28.35 15.61
13:00:36.49 -06:28:26.00 SN2026azd 2026-01-28.23 15.69
10:33:50.27 -31:00:53.40 SN 2026ayz 2026-01-25.11 15.3
05:14:22.36 -60:47:20.70 SN 2026apb 2026-01-24.08 17.35
06:39:26.57 -21:49:19.60 AT2026afe 2026-01-23.11 16.17
09:27:23.48 -32:00:31.10 SN 2023kuy 2026-01-21.24 15.33
09:38:44.42 -20:00:54.30 SN2026afi 2026-01-20.24 17.43
06:30:51.41 -74:35:46.80 AT2026ahr 2026-01-20.09 16.98
13:33:03.15 -16:14:28.70 SN2026amc 2026-01-20.29 16.9
06:57:11.13 -17:24:42.80 ASASSN-26an 2026-01-19.31 13.99
17:41:29.59 +68:57:34.90 2026abj 2026-01-18.64 17.02
10:22:25.13 +04:00:01.40 SN 2026kc 2026-01-18.24 16.4
12:42:03.30 +00:41:41.80 SN 2026pg 2026-01-18.5 17.44
03:36:21.80 -31:44:39.30 AT2025aibn 2026-01-17.04 16.7
13:45:00.71 -32:34:53.00 AT2026yi 2026-01-17.26 16.22
09:27:07.17 +62:45:24.20 AT2026nu 2026-01-17.29 17.09
12:38:41.73 +07:36:37.40 SN 2025afcr 2026-01-17.49 17.11
12:12:12.65 +13:13:18.50 SN 2026acd 2026-01-17.3 16.15
16:21:54.73 -63:36:53.10 ASASSN-26al 2026-01-17.36 15.34
15:33:45.22 -22:11:07.90 ASASSN-26aj 2026-01-16.51 14
12:27:08.33 -58:19:36.10 ASASSN-26ak 2026-01-16.2 13.94
17:21:53.10 +04:39:07.10 ASASSN-26ai 2026-01-16.67 14.83
-rw-r--r-- 1 apache apache 5.7K Mar 20 23:36 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
14:47:33.95 -10:02:56.8 TCP J14473395-1002568 2026-01-13.8185 14.0mag
15:33:45.28 -22:11:07.3 TCP J15334528-2211073 2026-01-16.8451 14.9mag
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
-rw-r--r-- 1 apache apache 187K Mar 20 23:36 tocp_transients_list.txt