This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx
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,2461083.6074,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.1074 12.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:56:43.91 +01:26:20.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.6074,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.1074 11.27CV 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/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:48:21.76 +01:52:20.8 ;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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.1074 2461083.6074 11.40 06:42:35.41 -03:49:12.1
215.32877 -3.70690 galactic Mon Second-epoch detections are separated by 5.7" 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 | ATO J100.6567-03.8098 | 06:42:37.27 -03:49:19.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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
ATO J100.6567-03.8098,2461083.6074,11.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.6567-03.8098 20260212.1074 11.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:42:35.41 -03:49:12.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.6074,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.1074 11.62CV 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/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:19:16.35 -04:07:29.5 ;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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.1074 2461083.6074 11.73 06:44:52.76 +00:57:20.4
211.33352 -1.02317 galactic Mon Second-epoch detections are separated by 5.8" 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 | ATO J101.2174+00.9629 | 06:44:52.76 +00:57:20.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J101.2174+00.9629,2461083.6074,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.2174+00.9629 20260212.1074 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:44:52.76 +00:57:20.4 ;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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.6074,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.1074 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:08:05.27 +00:45:21.5 ;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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_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 3117374232234391424,2461083.6074,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3117374232234391424 20260212.1074 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:26:46.55 -02:31:31.9 ;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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.1074 2461083.6074 12.09 06:43:19.13 -00:06:06.1
212.09661 -1.85279 galactic Mon Second-epoch detections are separated by 8.2" 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 | CoRoT 102686781 | 06:43:21.83 -00:05:55.3 (Gaia DR3) | EA (local) | 2454400.34390 (local) | Gaia3var=NOT_AVAILABLE SpType: A3V 2012A&A...541A..34S CoRoT 102686288
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CoRoT 102686781,2461083.6074,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CoRoT 102686781 20260212.1074 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:43:19.13 -00:06:06.1 ;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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.1074 2461083.6074 12.06 07:09:39.54 -03:41:35.6
218.29959 2.35924 galactic Mon Second-epoch detections are separated by 2.7" 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 | ATO J107.4073-03.6970 | 07:09:39.54 -03:41:35.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J107.4073-03.6970,2461083.6074,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J107.4073-03.6970 20260212.1074 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:09:39.54 -03:41:35.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.1074 2461083.6074 12.07 06:40:31.88 -01:56:29.4
213.41819 -3.31134 galactic Mon Second-epoch detections are separated by 4.1" 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 3106820501158554240 | 06:40:33.59 -01:56:08.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F? 1949AnHar.112....1C HD 292141
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3106820501158554240,2461083.6074,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 3106820501158554240 20260212.1074 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:40:31.88 -01:56:29.4 ;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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.1074 2461083.6074 12.07 06:32:39.38 +00:00:41.9
210.77671 -4.17255 galactic Mon Second-epoch detections are separated by 5.3" 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 | Gaia DR3 3120059411426840192 | 06:32:41.31 +00:00:33.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B6 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3120059411426840192,2461083.6074,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 3120059411426840192 20260212.1074 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:32:39.38 +00:00:41.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.6074,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.1074 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/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:17:35.85 -06:48:24.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.6074,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.1074 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/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:51:39.44 -05:32:29.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.6074,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.1074 12.12CV 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/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:54:26.26 -06:48:52.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.6074,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.1074 12.12CV 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/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:22:42.68 -04:29:34.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.1074 2461083.6074 12.15 06:52:03.28 -05:41:50.6
218.07577 -2.45785 galactic Mon Second-epoch detections are separated by 1.0" 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 | ATO J103.0078-05.6974 | 06:52:01.89 -05:41:50.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F9IV 2012A&A...543A.125G CoRoT 110677500
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J103.0078-05.6974,2461083.6074,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.0078-05.6974 20260212.1074 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:52:03.28 -05:41:50.6 ;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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.1074 2461083.6074 12.18 06:26:10.15 -04:23:56.9
213.98639 -7.62072 galactic Mon Second-epoch detections are separated by 4.3" 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 | ATO J096.5613-04.4020 | 06:26:12.13 -04:24:04.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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
ATO J096.5613-04.4020,2461083.6074,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J096.5613-04.4020 20260212.1074 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:26:10.15 -04:23:56.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat.ucac5 not found - falling back to uncorrected catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.6074,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.1074 10.29CV 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/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:03:31.94 -06:51:29.4 ;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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.6074,13.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.1074 13.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:27:05.63 -03:40:28.8 ;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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.6074,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.1074 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:27:57.79 -04:38:53.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.1074 2461083.6074 13.49 07:00:54.52 -00:54:42.9
214.82383 1.69079 galactic Mon Second-epoch detections are separated by 4.4" 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 | ATO J105.2246-00.9193 | 07:00:54.52 -00:54:42.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J105.2246-00.9193,2461083.6074,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.2246-00.9193 20260212.1074 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:00:54.52 -00:54:42.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.6074,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.1074 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:29:16.01 -05:22:08.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.1074 2461083.6074 12.93 06:22:01.35 -00:57:21.1
210.41960 -6.97906 galactic Mon Second-epoch detections are separated by 7.4" 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 | ATO J095.5196-00.9515 | 06:22:03.92 -00:57:05.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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
ATO J095.5196-00.9515,2461083.6074,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J095.5196-00.9515 20260212.1074 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/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:22:01.35 -00:57:21.1 ;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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.6074,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.1074 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:23:46.23 -00:49:27.1 ;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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_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 3059406570474894848,2461083.6074,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059406570474894848 20260212.1074 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:11:19.21 -04:50:00.6 ;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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.1074 2461083.6074 12.61 07:15:26.28 -05:02:29.4
220.16251 3.01508 galactic Mon Second-epoch detections are separated by 7.5" 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 | ATO J108.8604-05.0459 | 07:15:26.28 -05:02:29.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J108.8604-05.0459,2461083.6074,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J108.8604-05.0459 20260212.1074 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/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:15:26.28 -05:02:29.4 ;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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.1074 2461083.6074 12.17 06:32:28.29 -06:14:53.5
216.36291 -7.05134 galactic Mon Second-epoch detections are separated by 4.7" 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 | ATO J098.1215-06.2460 | 06:32:28.29 -06:14:53.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J098.1215-06.2460,2461083.6074,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J098.1215-06.2460 20260212.1074 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:32:28.29 -06:14:53.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.6074,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.1074 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:26:45.61 -05:29:39.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.6074,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.1074 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:01:57.23 -04:01:44.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.1074 2461083.6074 10.81 06:45:57.54 -04:51:53.3
216.64332 -3.43220 galactic Mon Second-epoch detections are separated by 3.4" 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 3102224370754086784 | 06:46:00.26 -04:51:50.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1949AnHar.112....1C HD 295492
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3102224370754086784,2461083.6074,10.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3102224370754086784 20260212.1074 10.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:45:57.54 -04:51:53.3 ;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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.1074 2461083.6074 10.71 06:36:42.28 -06:39:03.7
217.20053 -6.29240 galactic Mon Second-epoch detections are separated by 6.5" 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 | Gaia DR3 3100023423352888576 | 06:36:43.42 -06:38:44.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3100023423352888576,2461083.6074,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3100023423352888576 20260212.1074 10.71CV 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/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:36:42.28 -06:39:03.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.1074 2461083.6074 10.95 06:28:22.86 -02:24:26.5
212.44931 -6.22657 galactic Mon Second-epoch detections are separated by 6.8" and 4.1 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 J097.1028-02.4115 | 06:28:24.70 -02:24:10.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F8 1949AnHar.112....1C HD 295059
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J097.1028-02.4115,2461083.6074,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J097.1028-02.4115 20260212.1074 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:28:22.86 -02:24:26.5 ;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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_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 3119794424826044928,2461083.6074,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 3119794424826044928 20260212.1074 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:40:36.79 +00:42:54.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.1074 2461083.6074 11.37 07:03:42.40 -03:12:23.8
217.18494 1.26289 galactic Mon Second-epoch detections are separated by 7.0" 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 | ATO J105.9172-03.2004 | 07:03:42.40 -03:12:23.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J105.9172-03.2004,2461083.6074,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.9172-03.2004 20260212.1074 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:03:42.40 -03:12:23.8 ;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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.6074,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.1074 11.61CV 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/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:03:12.96 -06:38:25.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.6074,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.1074 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:18:23.97 -05:47:39.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.1074 2461083.6074 12.30 06:26:19.83 -03:10:06.0
212.89795 -7.02822 galactic Mon Second-epoch detections are separated by 5.0" 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 | Gaia DR3 3117129036843001984 | 06:26:18.37 -03:09:36.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1949AnHar.112....1C HD 295069
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3117129036843001984,2461083.6074,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3117129036843001984 20260212.1074 12.30CV 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/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:26:19.83 -03:10:06.0 ;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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.1074 2461083.6074 12.31 06:45:00.47 -01:02:29.0
213.12601 -1.90543 galactic Mon Second-epoch detections are separated by 8.7" 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 | ATO J101.2528-01.0498 | 06:45:00.47 -01:02:29.0 (user input) | CBH (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J101.2528-01.0498,2461083.6074,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.2528-01.0498 20260212.1074 12.31CV 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/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:45:00.47 -01:02:29.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.1074 2461083.6074 12.48 06:43:46.29 +01:35:38.6
210.63902 -0.97806 galactic Mon Second-epoch detections are separated by 7.6" 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 | ATO J100.9538+01.5947 | 06:43:46.29 +01:35:38.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J100.9538+01.5947,2461083.6074,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.9538+01.5947 20260212.1074 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:43:46.29 +01:35:38.6 ;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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.1074 2461083.6074 12.44 06:29:51.32 -02:40:55.8
212.86376 -6.02338 galactic Mon Second-epoch detections are separated by 8.2" 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 | Large-amplitude variable Gaia DR2 3117218269082306048 | 06:29:53.56 -02:40:59.6 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3117218269082306048,2461083.6074,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 3117218269082306048 20260212.1074 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:29:51.32 -02:40:55.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.1074 2461083.6074 12.65 07:07:00.24 -03:22:51.2
217.71737 1.91434 galactic Mon Second-epoch detections are separated by 8.6" 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 | ATO J106.7482-03.3849 | 07:07:00.24 -03:22:51.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J106.7482-03.3849,2461083.6074,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.7482-03.3849 20260212.1074 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:07:00.24 -03:22:51.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.1074 2461083.6074 12.55 06:22:25.50 -01:43:06.2
211.14950 -7.23784 galactic Mon Second-epoch detections are separated by 3.3" 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 | ATO J095.6009-01.7118 | 06:22:24.93 -01:42:34.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A5V (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J095.6009-01.7118,2461083.6074,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J095.6009-01.7118 20260212.1074 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:22:25.50 -01:43:06.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.6074,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.1074 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:05:13.44 +00:16:02.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_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 3059155057188876544,2461083.6074,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059155057188876544 20260212.1074 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:11:47.52 -05:22:25.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.6074,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.1074 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:09:43.75 -04:05:45.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.1074 2461083.6074 12.92 06:35:20.75 -05:17:45.1
215.83039 -5.98450 galactic Mon Second-epoch detections are separated by 8.1" 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 3103464959174981120 | 06:35:19.47 -05:17:08.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3103464959174981120,2461083.6074,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 3103464959174981120 20260212.1074 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:35:20.75 -05:17:45.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.1074 2461083.6074 13.24 06:24:07.67 -00:49:42.8
210.54796 -6.45284 galactic Mon Second-epoch detections are separated by 8.6" and 4.1 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 J096.0346-00.8271 | 06:24:09.08 -00:50:15.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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
ATO J096.0346-00.8271,2461083.6074,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J096.0346-00.8271 20260212.1074 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:24:07.67 -00:49:42.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.6074,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.1074 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:44:44.78 +01:05:28.3 ;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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.6074,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.1074 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/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:03:17.93 -01:02:24.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.6074,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.1074 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/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:51:24.83 -02:44:46.9 ;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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.6074,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.1074 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/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:01:09.23 -00:46:26.5 ;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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.1074 2461083.6074 13.44 06:51:23.90 -02:32:46.5
215.19385 -1.16955 galactic Mon Second-epoch detections are separated by 7.4" 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 | ATO J102.8559-02.5439 | 06:51:25.42 -02:32:38.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A0 1956ApJS....2..271M LF 9 -03 163
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J102.8559-02.5439,2461083.6074,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.8559-02.5439 20260212.1074 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/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:51:23.90 -02:32:46.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.1074 2461083.6074 13.40 06:51:28.52 -02:44:47.3
215.38089 -1.24365 galactic Mon Second-epoch detections are separated by 8.1" 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 | ATO J102.8680-02.7440 | 06:51:28.52 -02:44:47.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J102.8680-02.7440,2461083.6074,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.8680-02.7440 20260212.1074 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:51:28.52 -02:44:47.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.6074,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.1074 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/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:51:00.55 -02:21:47.5 ;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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.6074,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.1074 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/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:26:55.37 -03:31:10.4 ;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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.1074 2461083.6074 13.63 06:41:30.90 +02:27:57.4
209.60570 -1.08107 galactic Mon Second-epoch detections are separated by 8.8" and 4.1 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 3126851468410240896 | 06:41:32.03 +02:28:21.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A 1949AnHar.112....1C HD 288944
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3126851468410240896,2461083.6074,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126851468410240896 20260212.1074 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/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:41:30.90 +02:27:57.4 ;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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.6074,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.1074 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:10:57.08 -05:23:30.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.1074 2461083.6074 13.43 06:25:59.45 -04:36:09.2
214.14938 -7.75212 galactic Mon Second-epoch detections are separated by 6.8" 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 | ATO J096.5075-04.6043 | 06:26:01.96 -04:36:06.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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
ATO J096.5075-04.6043,2461083.6074,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J096.5075-04.6043 20260212.1074 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/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:25:59.45 -04:36:09.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.6074,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.1074 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/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:10:42.50 -04:48:58.8 ;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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.6074,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.1074 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/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:32:47.52 -05:35:10.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.6074,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.1074 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/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:14:25.55 -05:34:56.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.1074 2461083.6074 13.74 07:00:21.19 -00:45:49.8
214.62859 1.63488 galactic Mon Second-epoch detections are separated by 6.3" 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 3112625716393036672 | 07:00:18.42 -00:45:39.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1956ApJS....2..271M LF 9 -01 491
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3112625716393036672,2461083.6074,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112625716393036672 20260212.1074 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:00:21.19 -00:45:49.8 ;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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.6074,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.1074 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/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:48:12.64 +01:01:03.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix.png animation_v2.gif
WARNING from util/transients/report_transient.sh -- UCAC5 catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat.ucac5 not found - falling back to uncorrected catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.6074,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.1074 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:10:14.25 -05:11:56.3 ;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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20_00sec_-15_00C_LIGHT_0040_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20_00sec_-15_00C_LIGHT_0039_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: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
First image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Last image: 2461083.60758603 12.02.2026 02:34:45.433 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 23
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.85
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: 13 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): 36118
Objects passed selection criteria: 36101
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 34615.2
Average stars matched: 33709.8 (97.3841 %)
Memory usage VmPeak: 137244 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Feb 11 20:39:33 CST 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
First image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Last image: 2461083.60758603 12.02.2026 02:34:45.433 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 860
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.54
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: 270 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): 260637
Objects passed selection criteria: 259924
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 249378
Average stars matched: 239361 (95.9833 %)
Memory usage VmPeak: 2444712 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Feb 11 20:59:43 CST 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits
SExtractor catalog cache: saved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.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/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461083.60713390
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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits exists and is non-empty
Saving wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits to local_wcs_cache/
'wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'local_wcs_cache/wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits exists and is non-empty
Saving wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits to local_wcs_cache/
'wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'local_wcs_cache/wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits'
wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.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 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:25.113 -01:57:36.31
Angular distance between the image centers 0.09 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 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:25.850 -01:57:56.90
Angular distance between the image centers 0.08 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 06:51:25.113 -01:57:36.31
Second-epoch second image center 06:51:25.850 -01:57:56.90
Angular distance between the image centers 0.00649 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/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits &> /tmp/tmp.YUpsiW1Rm3
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits &> /tmp/tmp.Gym9oep7TK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits &> /tmp/tmp.6NVwmOWTJy
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits &> /tmp/tmp.Mdyoe3lv6c
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Found non-empty wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
The reference image (wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits) and catalog (wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat) found
'wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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-2 430 out of 36622 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.893894
a=0.000000 b=1.000000 c=22.893894
From vast_summary.log: estimated ref. image limiting mag.: -7.85
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.04
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.04
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 23 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.1 pix Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
2.2 pix fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits
2.2 pix fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits
Limiting magnitude estimates:
15.0 mag. Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
15.0 mag. Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
15.0 mag. fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits
15.0 mag. fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.0 (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.YUpsiW1Rm3 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS-calibrated image found: wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Checking if the catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS catalog name: wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4596, passed=36622
Got 36622 stars (including 31982 good ones) from the SExtractor catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
util/solve_plate_with_UCAC5 got 36622 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.8'
Seting catalog search parameters based on the expected field of view 931.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012942 (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 0.010353 (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 457 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: 10.06"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 16.11"
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 489 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 16.01"
Estimated accuracy of the plate solution: 12.91"
Excluding outliers - 390 stars left (next iteration limit 371)
The image catalog is written to wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits -region wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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.Gym9oep7TK (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS-calibrated image found: wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Checking if the catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS catalog name: wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4657, passed=36412
Got 36412 stars (including 31701 good ones) from the SExtractor catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
util/solve_plate_with_UCAC5 got 36412 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 625.6'
Seting catalog search parameters based on the expected field of view 625.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.008689 (31.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.006951 (25.0 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 20 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Retrying with a larger catalog search radius.
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 73 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: 0.00"
ERROR: the estimated accuracy of the plate solution seems unrealistically small!
Something is very wrong!
ERROR running correct_measured_positions()
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.6NVwmOWTJy (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3959, passed=33171
Got 33171 stars (including 29175 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits.cat
util/solve_plate_with_UCAC5 got 33171 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 930.8'
Seting catalog search parameters based on the expected field of view 930.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012928 (46.5 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010342 (37.2 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 362 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: 10.69"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 14.94"
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 388 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 15.05"
Estimated accuracy of the plate solution: 15.02"
Excluding outliers - 283 stars left (next iteration limit 276)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits -region wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.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.Mdyoe3lv6c (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3996, passed=33090
Got 33090 stars (including 29055 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits.cat
util/solve_plate_with_UCAC5 got 33090 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 930.8'
Seting catalog search parameters based on the expected field of view 930.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012928 (46.5 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010342 (37.2 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 363 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: 12.78"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 17.16"
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 390 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 17.27"
Estimated accuracy of the plate solution: 18.33"
Excluding outliers - 297 stars left (next iteration limit 288)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits -region wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits'
Preparing the HTML report for the field Mon-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out01285.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52520.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52631.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52645.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52654.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52663.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52689.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52701.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52708.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52715.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52718.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52722.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52726.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52727.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52730.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52738.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52744.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52750.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 30s
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: 11s
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Considering the candidate 52520_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 52520_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 52631_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 52631_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 52645_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 52645_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 52654_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 52654_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 52663_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 52663_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 52673_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 52673_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 52689_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 52689_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 52697_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 52697_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 52701_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 52701_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 52708_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 52708_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 52711_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 52711_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 52715_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 52715_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52718_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 52718_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52722_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 52722_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52726_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 52726_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52727_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 52727_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52730_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 52730_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52735_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 52735_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
**** FOUND 06:22:22.09 -01:42:17.9 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52738_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 52738_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52744_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 52744_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52749_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 52749_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (26.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52750_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 52750_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01285_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 01285_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 42s
Prepared the HTML report for the field Mon-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
07:03:31.94 -06:51:29.4
06:56:43.91 +01:26:20.0
06:48:21.76 +01:52:20.8
06:42:35.41 -03:49:12.1
07:19:16.35 -04:07:29.5
06:44:52.76 +00:57:20.4
07:08:05.27 +00:45:21.5
06:26:46.55 -02:31:31.9
06:43:19.13 -00:06:06.1
07:09:39.54 -03:41:35.6
06:40:31.88 -01:56:29.4
06:32:39.38 +00:00:41.9
07:17:35.85 -06:48:24.9
06:51:39.44 -05:32:29.0
06:54:26.26 -06:48:52.4
06:22:42.68 -04:29:34.0
06:52:03.28 -05:41:50.6
06:26:10.15 -04:23:56.9
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits
SExtractor catalog cache: saved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Creating symlink local_wcs_cache/wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits exists and is non-empty
wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits exists and is non-empty
wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits exists and is non-empty
wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.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 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:25.113 -01:57:36.31
Angular distance between the image centers 0.09 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 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:25.850 -01:57:56.90
Angular distance between the image centers 0.08 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 06:51:25.113 -01:57:36.31
Second-epoch second image center 06:51:25.850 -01:57:56.90
Angular distance between the image centers 0.00649 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/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits &> /tmp/tmp.XWAMzxzA4Z
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits &> /tmp/tmp.djdxPXwJp2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits &> /tmp/tmp.9lqVGPFrsJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits &> /tmp/tmp.tHZHLUT6gk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Found non-empty wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
The reference image (wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits) and catalog (wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat) found
'wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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-2 624 out of 254624 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 21.875060
a=0.000000 b=1.000000 c=21.875060
From vast_summary.log: estimated ref. image limiting mag.: -7.54
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.34
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.34
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 790 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.0 pix Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
1.9 pix fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits
1.9 pix fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits
Limiting magnitude estimates:
14.3 mag. Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
14.3 mag. Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
14.2 mag. fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits
14.2 mag. fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 13.5 (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.XWAMzxzA4Z (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS-calibrated image found: wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Checking if the catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS catalog name: wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=59, blended=45640, passed=254565
Got 254565 stars (including 208571 good ones) from the SExtractor catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
util/solve_plate_with_UCAC5 got 254565 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.8'
Seting catalog search parameters based on the expected field of view 931.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012942 (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 0.010353 (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 468 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: 6.77"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 7.43"
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 498 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 7.42"
Estimated accuracy of the plate solution: 6.79"
Excluding outliers - 428 stars left (next iteration limit 402)
The image catalog is written to wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits -region wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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.djdxPXwJp2 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS-calibrated image found: wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Checking if the catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS catalog name: wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=58, blended=46013, passed=257598
Got 257598 stars (including 211206 good ones) from the SExtractor catalog wcs_Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
util/solve_plate_with_UCAC5 got 257598 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 625.6'
Seting catalog search parameters based on the expected field of view 625.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.008689 (31.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.006951 (25.0 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 17 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Retrying with a larger catalog search radius.
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 68 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: 0.00"
ERROR: the estimated accuracy of the plate solution seems unrealistically small!
Something is very wrong!
ERROR running correct_measured_positions()
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.9lqVGPFrsJ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=72, blended=39036, passed=244572
Got 244572 stars (including 205171 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits.cat
util/solve_plate_with_UCAC5 got 244572 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 930.8'
Seting catalog search parameters based on the expected field of view 930.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012928 (46.5 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010342 (37.2 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 411 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: 8.26"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 8.29"
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 442 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 8.29"
Estimated accuracy of the plate solution: 7.64"
Excluding outliers - 349 stars left (next iteration limit 335)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits -region wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.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.tHZHLUT6gk (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=86, blended=39102, passed=245424
Got 245424 stars (including 205987 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits.cat
util/solve_plate_with_UCAC5 got 245424 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 930.8'
Seting catalog search parameters based on the expected field of view 930.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012928 (46.5 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010342 (37.2 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 414 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: 8.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 9.07"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 439 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 9.07"
Estimated accuracy of the plate solution: 6.44"
Excluding outliers - 350 stars left (next iteration limit 350)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits -region wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-06_20.00sec_-15.00C_LIGHT_0039.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Mon-02-Q1b1x1_203529_TTUQ1b1x1_8625_O2JTEpSx/wcs_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040.fits
Preparing the HTML report for the field Mon-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out289952.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out288681.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288723.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288840.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289071.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289125.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289131.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289148.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289208.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289230.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289257.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289258.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289275.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289277.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289440.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289468.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289483.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289544.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289726.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289763.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289790.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289864.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289908.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289918.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289942.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289953.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290055.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290113.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290254.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290524.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290567.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290686.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290703.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290791.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290850.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290914.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out290922.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291025.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291125.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291220.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291242.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291434.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291495.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291619.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291864.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out291997.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46140.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 102s
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: 29s
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Considering the candidate 288656_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288656_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (40.3") between the two second-epoch detections
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Considering the candidate 288660_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288660_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (27.6") between the two second-epoch detections
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Considering the candidate 288672_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288672_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 288681_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 288681_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 288684_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288684_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 288690_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288690_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 288694_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288694_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 288696_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288696_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (37.6") between the two second-epoch detections
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Considering the candidate 288704_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288704_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 288705_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288705_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (44.7") between the two second-epoch detections
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Considering the candidate 288707_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288707_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 288709_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288709_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 288710_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288710_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 288713_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288713_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 288714_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288714_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 288716_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288716_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 288722_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288722_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 288723_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 288723_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 288726_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288726_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 288732_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288732_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 288734_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288734_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 288741_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288741_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 288742_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288742_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 288745_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288745_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 288746_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288746_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 288749_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288749_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 288751_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288751_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 288755_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288755_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 288760_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288760_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 288771_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288771_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 288780_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288780_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 288787_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288787_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 288788_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288788_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (27.9") between the two second-epoch detections
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Considering the candidate 288791_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288791_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (28.3") between the two second-epoch detections
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Considering the candidate 288800_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288800_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (44.4") between the two second-epoch detections
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Considering the candidate 288802_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288802_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (27.5") between the two second-epoch detections
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Considering the candidate 288803_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288803_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 288804_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288804_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 288809_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288809_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (36.5") between the two second-epoch detections
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Considering the candidate 288814_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288814_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 288817_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288817_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 288819_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288819_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (46.5") between the two second-epoch detections
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Considering the candidate 288833_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288833_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 288834_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288834_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (25.4") between the two second-epoch detections
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Considering the candidate 288840_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 288840_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 288841_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288841_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 288842_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288842_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (26.9") between the two second-epoch detections
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Considering the candidate 288849_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288849_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (33.1") between the two second-epoch detections
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Considering the candidate 288850_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288850_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 288853_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288853_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 288863_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288863_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (52.0") between the two second-epoch detections
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Considering the candidate 288874_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288874_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (39.9") between the two second-epoch detections
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Considering the candidate 288876_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288876_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 288877_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288877_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (39.1") between the two second-epoch detections
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Considering the candidate 288878_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288878_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 288885_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288885_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (45.6") between the two second-epoch detections
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Considering the candidate 288888_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288888_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 288890_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288890_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (40.3") between the two second-epoch detections
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Considering the candidate 288898_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288898_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (32.9") between the two second-epoch detections
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Considering the candidate 288899_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288899_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (24.3") between the two second-epoch detections
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Considering the candidate 288903_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288903_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (44.0") between the two second-epoch detections
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Considering the candidate 288905_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288905_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (25.7") between the two second-epoch detections
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Considering the candidate 288907_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288907_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (41.5") between the two second-epoch detections
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Considering the candidate 288909_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288909_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 288910_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288910_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 288917_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288917_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 288918_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288918_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 288919_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288919_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 288926_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288926_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 288932_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288932_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 288938_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288938_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (33.4") between the two second-epoch detections
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Considering the candidate 288939_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288939_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 288951_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288951_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 288955_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288955_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 288958_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288958_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (44.5") between the two second-epoch detections
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Considering the candidate 288959_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288959_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 288960_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288960_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (47.3") between the two second-epoch detections
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Considering the candidate 288963_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288963_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (44.5") between the two second-epoch detections
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Considering the candidate 288971_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288971_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 288972_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288972_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (27.4") between the two second-epoch detections
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Considering the candidate 288973_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288973_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 288974_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288974_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (24.9") between the two second-epoch detections
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Considering the candidate 288976_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288976_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 288979_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288979_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 288985_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288985_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 288987_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288987_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 288992_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288992_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (26.1") between the two second-epoch detections
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Considering the candidate 288993_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288993_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (38.5") between the two second-epoch detections
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Considering the candidate 288995_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 288995_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 289002_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289002_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 289004_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289004_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289009_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289009_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289015_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289015_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (29.4") between the two second-epoch detections
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Considering the candidate 289020_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289020_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (35.5") between the two second-epoch detections
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Considering the candidate 289021_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289021_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289022_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289022_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (39.6") between the two second-epoch detections
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Considering the candidate 289026_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289026_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (74.8") between the two second-epoch detections
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Considering the candidate 289030_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289030_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 289036_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289036_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 289037_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289037_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (36.4") between the two second-epoch detections
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Considering the candidate 289038_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289038_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (32.8") between the two second-epoch detections
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Considering the candidate 289041_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289041_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (30.1") between the two second-epoch detections
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Considering the candidate 289045_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289045_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (44.8") between the two second-epoch detections
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Considering the candidate 289046_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289046_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (38.6") between the two second-epoch detections
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Considering the candidate 289047_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289047_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 289052_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289052_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 289058_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289058_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 289060_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289060_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (38.7") between the two second-epoch detections
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Considering the candidate 289062_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289062_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (32.7") between the two second-epoch detections
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Considering the candidate 289065_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289065_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (37.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289070_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289070_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289071_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 289071_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 289075_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289075_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 289080_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289080_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289081_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289081_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 289083_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289083_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289084_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289084_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (36.7") between the two second-epoch detections
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Considering the candidate 289085_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289085_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (62.2") between the two second-epoch detections
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Considering the candidate 289087_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289087_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 289088_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289088_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (43.5") between the two second-epoch detections
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Considering the candidate 289089_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289089_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289091_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289091_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 289093_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289093_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289103_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289103_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 289105_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289105_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (53.4") between the two second-epoch detections
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Considering the candidate 289107_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289107_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289115_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289115_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289118_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289118_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (25.5") between the two second-epoch detections
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Considering the candidate 289121_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289121_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (28.6") between the two second-epoch detections
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Considering the candidate 289123_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289123_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 289125_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 289125_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 289131_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 289131_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 289135_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289135_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 289141_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289141_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (38.8") between the two second-epoch detections
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Considering the candidate 289143_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289143_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 289144_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289144_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (43.2") between the two second-epoch detections
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Considering the candidate 289148_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 289148_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 289149_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289149_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289150_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289150_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289151_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289151_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289152_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289152_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289156_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289156_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 289160_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289160_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289164_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289164_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (37.7") between the two second-epoch detections
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Considering the candidate 289173_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289173_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 289176_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289176_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 289177_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289177_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 289182_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289182_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (41.5") between the two second-epoch detections
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Considering the candidate 289189_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289189_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 289194_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289194_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (33.5") between the two second-epoch detections
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Considering the candidate 289197_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289197_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 289198_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289198_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 289202_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289202_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 289205_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289205_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (24.4") between the two second-epoch detections
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Considering the candidate 289208_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 289208_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 289212_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289212_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 289215_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289215_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 289217_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289217_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289219_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289219_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 289223_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289223_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 289225_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289225_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (35.1") between the two second-epoch detections
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Considering the candidate 289230_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 289230_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 289233_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289233_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 289236_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289236_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (30.3") between the two second-epoch detections
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Considering the candidate 289238_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289238_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 289239_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289239_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (30.9") between the two second-epoch detections
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Considering the candidate 289241_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289241_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289246_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289246_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289247_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289247_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (41.8") between the two second-epoch detections
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Considering the candidate 289248_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289248_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289250_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289250_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (36.7") between the two second-epoch detections
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Considering the candidate 289254_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289254_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 289255_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289255_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 289257_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 289257_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 289258_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 289258_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 289265_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289265_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 289267_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289267_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (51.0") between the two second-epoch detections
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Considering the candidate 289268_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289268_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (24.2") between the two second-epoch detections
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Considering the candidate 289271_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289271_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (31.6") between the two second-epoch detections
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Considering the candidate 289273_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289273_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 289275_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 289275_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 289276_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289276_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 289277_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 289277_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 289353_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289353_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 289394_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289394_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 289415_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289415_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 289440_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 289440_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 289448_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289448_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289455_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289455_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 289468_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 289468_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 289469_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289469_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289475_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289475_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (30.7") between the two second-epoch detections
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Considering the candidate 289480_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289480_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 289483_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 289483_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 289533_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289533_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289542_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289542_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289544_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 289544_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 289568_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289568_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 289569_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289569_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 289583_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289583_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 289616_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289616_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (44.6") between the two second-epoch detections
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Considering the candidate 289617_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289617_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 289627_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289627_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 289635_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289635_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 289637_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289637_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289659_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289659_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 289664_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289664_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 289665_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289665_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (24.3") between the two second-epoch detections
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Considering the candidate 289668_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289668_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (30.7") between the two second-epoch detections
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Considering the candidate 289681_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289681_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 289683_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289683_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (30.9") between the two second-epoch detections
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Considering the candidate 289697_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289697_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (41.4") between the two second-epoch detections
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Considering the candidate 289708_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289708_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (44.2") between the two second-epoch detections
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Considering the candidate 289722_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289722_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289723_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289723_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 289726_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 289726_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 289729_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289729_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289736_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289736_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (43.5") between the two second-epoch detections
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Considering the candidate 289740_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289740_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289741_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289741_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289748_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289748_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289751_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289751_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289752_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289752_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289756_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289756_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289763_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 289763_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 289778_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289778_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (24.4") between the two second-epoch detections
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Considering the candidate 289788_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289788_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289790_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 289790_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 289793_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289793_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 289799_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289799_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 289800_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289800_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 289801_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289801_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 289803_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289803_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 289806_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289806_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289807_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289807_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 289808_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289808_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (26.7") between the two second-epoch detections
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Considering the candidate 289811_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289811_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 289815_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289815_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289817_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289817_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (26.8") between the two second-epoch detections
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Considering the candidate 289818_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289818_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 289838_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289838_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (41.0") between the two second-epoch detections
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Considering the candidate 289860_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289860_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (34.0") between the two second-epoch detections
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Considering the candidate 289864_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 289864_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 289872_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289872_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (44.0") between the two second-epoch detections
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Considering the candidate 289877_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289877_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (43.3") between the two second-epoch detections
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Considering the candidate 289885_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289885_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 289892_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289892_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 289903_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289903_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (30.1") between the two second-epoch detections
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Considering the candidate 289906_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289906_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289908_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 289908_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 289918_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 289918_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 289924_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289924_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (25.9") between the two second-epoch detections
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Considering the candidate 289942_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 289942_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 289952_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289952_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
**** FOUND 06:21:33.83 -01:09:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 4.619 3118511470854723968 095.39050427534 -01.15318877958 11.3201 10.5555 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.619#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289953_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 289953_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 289960_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289960_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 289961_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289961_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289965_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289965_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 289970_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289970_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (29.8") between the two second-epoch detections
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Considering the candidate 289973_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289973_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 289979_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289979_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (42.9") between the two second-epoch detections
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Considering the candidate 289984_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289984_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 289989_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289989_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 289993_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 289993_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 290000_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290000_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290002_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290002_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290014_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290014_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 290018_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290018_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (36.3") between the two second-epoch detections
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Considering the candidate 290028_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290028_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 290034_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290034_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (40.8") between the two second-epoch detections
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Considering the candidate 290038_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290038_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (26.1") between the two second-epoch detections
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Considering the candidate 290040_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290040_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 290042_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290042_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290055_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 290055_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 290059_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290059_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290061_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290061_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (26.0") between the two second-epoch detections
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Considering the candidate 290066_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290066_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (26.3") between the two second-epoch detections
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Considering the candidate 290070_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290070_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 290074_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290074_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (49.3") between the two second-epoch detections
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Considering the candidate 290078_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290078_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 290083_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290083_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (48.8") between the two second-epoch detections
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Considering the candidate 290087_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290087_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (36.2") between the two second-epoch detections
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Considering the candidate 290089_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290089_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290091_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290091_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290099_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290099_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 290103_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290103_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290105_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290105_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290110_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290110_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 290113_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 290113_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 290116_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290116_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 290130_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290130_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 290140_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290140_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290147_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290147_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (53.2") between the two second-epoch detections
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Considering the candidate 290152_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290152_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (53.3") between the two second-epoch detections
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Considering the candidate 290158_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290158_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (26.1") between the two second-epoch detections
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Considering the candidate 290173_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290173_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290177_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290177_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290194_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290194_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 290216_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290216_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290221_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290221_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 290224_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290224_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 290227_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290227_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (28.5") between the two second-epoch detections
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Considering the candidate 290228_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290228_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (70.7") between the two second-epoch detections
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Considering the candidate 290239_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290239_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290243_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290243_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290254_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 290254_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 290261_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290261_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (43.1") between the two second-epoch detections
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Considering the candidate 290263_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290263_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 290265_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290265_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 290270_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290270_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 290272_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290272_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (32.1") between the two second-epoch detections
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Considering the candidate 290274_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290274_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290275_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290275_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290280_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290280_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (32.2") between the two second-epoch detections
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Considering the candidate 290284_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290284_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 290290_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290290_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (46.3") between the two second-epoch detections
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Considering the candidate 290291_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290291_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 290292_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290292_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 290307_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290307_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 290314_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290314_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 290316_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290316_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290319_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290319_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 290321_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290321_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 290329_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290329_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290330_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290330_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 290331_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290331_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (44.1") between the two second-epoch detections
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Considering the candidate 290332_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290332_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (24.7") between the two second-epoch detections
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Considering the candidate 290333_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290333_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (30.1") between the two second-epoch detections
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Considering the candidate 290334_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290334_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (34.4") between the two second-epoch detections
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Considering the candidate 290336_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290336_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 290339_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290339_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290342_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290342_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290344_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290344_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 290358_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290358_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290360_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290360_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 290361_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290361_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 290364_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290364_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 290365_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290365_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (33.9") between the two second-epoch detections
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Considering the candidate 290379_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290379_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (34.4") between the two second-epoch detections
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Considering the candidate 290383_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290383_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (55.9") between the two second-epoch detections
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Considering the candidate 290384_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290384_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 290387_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290387_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 290391_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290391_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (39.9") between the two second-epoch detections
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Considering the candidate 290393_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290393_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290398_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290398_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 290401_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290401_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (46.3") between the two second-epoch detections
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Considering the candidate 290410_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290410_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 290411_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290411_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 290414_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290414_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 290415_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290415_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290433_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290433_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 290434_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290434_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 290436_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290436_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290437_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290437_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290441_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290441_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290444_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290444_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (31.2") between the two second-epoch detections
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Considering the candidate 290451_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290451_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290454_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290454_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (56.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290456_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290456_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290458_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290458_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290462_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290462_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (36.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290465_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290465_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290468_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290468_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290473_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290473_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (29.9") between the two second-epoch detections
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Considering the candidate 290478_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290478_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290486_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290486_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (40.6") between the two second-epoch detections
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Considering the candidate 290489_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290489_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 290492_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290492_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 290493_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290493_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290494_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290494_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (33.5") between the two second-epoch detections
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Considering the candidate 290496_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290496_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (56.5") between the two second-epoch detections
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Considering the candidate 290502_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290502_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 290505_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290505_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290513_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290513_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 290517_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290517_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290518_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290518_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (61.6") between the two second-epoch detections
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Considering the candidate 290521_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290521_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 290522_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290522_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (23.9") between the two second-epoch detections
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Considering the candidate 290524_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 290524_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 290530_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290530_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 290535_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290535_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (43.1") between the two second-epoch detections
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Considering the candidate 290539_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290539_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (41.8") between the two second-epoch detections
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Considering the candidate 290546_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290546_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 290551_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290551_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 290558_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290558_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 290562_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290562_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (44.9") between the two second-epoch detections
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Considering the candidate 290566_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290566_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 290567_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 290567_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 290570_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290570_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 290574_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290574_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 290575_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290575_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290577_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290577_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 290578_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290578_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 290584_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290584_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (50.8") between the two second-epoch detections
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Considering the candidate 290587_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290587_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290588_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290588_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (36.5") between the two second-epoch detections
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Considering the candidate 290590_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290590_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 290594_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290594_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (25.1") between the two second-epoch detections
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Considering the candidate 290597_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290597_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 290601_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290601_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (34.9") between the two second-epoch detections
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Considering the candidate 290608_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290608_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (45.1") between the two second-epoch detections
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Considering the candidate 290616_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290616_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 290618_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290618_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290620_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290620_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290623_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290623_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290636_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290636_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (41.2") between the two second-epoch detections
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Considering the candidate 290639_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290639_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (37.4") between the two second-epoch detections
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Considering the candidate 290644_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290644_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (31.1") between the two second-epoch detections
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Considering the candidate 290645_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290645_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 290646_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290646_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (32.9") between the two second-epoch detections
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Considering the candidate 290653_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290653_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290661_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290661_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (23.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290665_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290665_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290677_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290677_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (23.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290680_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290680_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290681_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290681_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290686_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 290686_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290690_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290690_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (44.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290699_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290699_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290701_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290701_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (33.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290703_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 290703_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290715_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290715_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290717_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290717_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (26.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290721_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290721_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (26.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290726_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290726_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 290727_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290727_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290732_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290732_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (28.4") between the two second-epoch detections
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Considering the candidate 290733_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290733_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 290734_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290734_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (33.4") between the two second-epoch detections
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Considering the candidate 290735_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290735_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290742_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290742_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 290747_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290747_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 290756_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290756_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (42.7") between the two second-epoch detections
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Considering the candidate 290758_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290758_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 290759_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290759_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (40.0") between the two second-epoch detections
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Considering the candidate 290760_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290760_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (44.7") between the two second-epoch detections
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Considering the candidate 290765_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290765_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 290767_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290767_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290768_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290768_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 290771_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290771_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (26.3") between the two second-epoch detections
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Considering the candidate 290772_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290772_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (29.1") between the two second-epoch detections
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Considering the candidate 290773_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290773_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (30.5") between the two second-epoch detections
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Considering the candidate 290775_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290775_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (25.8") between the two second-epoch detections
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Considering the candidate 290777_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290777_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (27.3") between the two second-epoch detections
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Considering the candidate 290780_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290780_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 290786_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290786_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (51.8") between the two second-epoch detections
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Considering the candidate 290790_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290790_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290791_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 290791_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 290792_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290792_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 290795_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290795_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 290800_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290800_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (32.9") between the two second-epoch detections
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Considering the candidate 290801_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290801_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 290802_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290802_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 290819_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290819_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (47.8") between the two second-epoch detections
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Considering the candidate 290823_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290823_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290827_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290827_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290828_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290828_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290829_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290829_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (32.3") between the two second-epoch detections
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Considering the candidate 290846_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290846_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290847_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290847_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290850_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 290850_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 290851_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290851_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (25.5") between the two second-epoch detections
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Considering the candidate 290857_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290857_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (45.8") between the two second-epoch detections
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Considering the candidate 290861_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290861_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (31.3") between the two second-epoch detections
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Considering the candidate 290873_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290873_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290884_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290884_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 290892_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290892_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 290893_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290893_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290894_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290894_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290898_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290898_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (26.5") between the two second-epoch detections
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Considering the candidate 290899_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290899_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290902_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290902_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (25.5") between the two second-epoch detections
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Considering the candidate 290905_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290905_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290914_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 290914_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290918_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290918_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290922_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 290922_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290927_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290927_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290932_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290932_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 290934_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290934_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (35.2") between the two second-epoch detections
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Considering the candidate 290936_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290936_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (25.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290939_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290939_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290940_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290940_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290943_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290943_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290946_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290946_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290947_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290947_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 290954_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290954_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290961_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290961_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 290966_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290966_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 290970_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290970_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 290972_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290972_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (23.9") between the two second-epoch detections
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Considering the candidate 290974_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290974_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (26.6") between the two second-epoch detections
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Considering the candidate 290978_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290978_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (48.7") between the two second-epoch detections
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Considering the candidate 290980_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290980_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (51.3") between the two second-epoch detections
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Considering the candidate 290982_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290982_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290985_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290985_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 290992_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290992_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290993_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290993_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290995_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290995_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 290999_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 290999_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 291008_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291008_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (41.7") between the two second-epoch detections
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Considering the candidate 291012_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291012_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 291016_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291016_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (25.3") between the two second-epoch detections
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Considering the candidate 291020_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291020_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291021_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291021_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (71.0") between the two second-epoch detections
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Considering the candidate 291022_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291022_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291025_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 291025_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 291029_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291029_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (24.4") between the two second-epoch detections
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Considering the candidate 291034_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291034_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 291040_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291040_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 291042_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291042_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 291043_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291043_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 291047_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291047_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 291053_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291053_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 291054_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291054_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (24.7") between the two second-epoch detections
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Considering the candidate 291066_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291066_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291068_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291068_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 291070_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291070_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 291074_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291074_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (26.1") between the two second-epoch detections
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Considering the candidate 291078_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291078_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291085_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291085_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291090_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291090_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 291091_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291091_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 291099_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291099_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 291102_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291102_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (29.8") between the two second-epoch detections
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Considering the candidate 291106_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291106_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291118_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291118_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 291120_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291120_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 291125_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 291125_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 291127_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291127_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (26.8") between the two second-epoch detections
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Considering the candidate 291130_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291130_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 291140_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291140_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291149_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291149_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 291151_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291151_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291157_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291157_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 291158_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291158_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291161_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291161_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291166_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291166_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291167_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291167_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (24.2") between the two second-epoch detections
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Considering the candidate 291172_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291172_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 291173_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291173_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291178_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291178_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (42.9") between the two second-epoch detections
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Considering the candidate 291179_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291179_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (43.7") between the two second-epoch detections
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Considering the candidate 291181_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291181_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291182_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291182_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 291191_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291191_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (36.2") between the two second-epoch detections
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Considering the candidate 291193_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291193_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 291196_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291196_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 291202_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291202_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291206_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291206_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 291207_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291207_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291210_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291210_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 291212_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291212_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291220_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 291220_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 291221_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291221_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291242_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 291242_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 291245_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291245_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (30.6") between the two second-epoch detections
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Considering the candidate 291248_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291248_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291250_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291250_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (43.4") between the two second-epoch detections
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Considering the candidate 291251_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291251_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 291258_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291258_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291261_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291261_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 291267_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291267_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 291274_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291274_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 291275_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291275_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 291277_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291277_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 291288_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291288_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (28.0") between the two second-epoch detections
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Considering the candidate 291291_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291291_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291296_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291296_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (24.2") between the two second-epoch detections
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Considering the candidate 291297_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291297_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 291301_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291301_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (25.8") between the two second-epoch detections
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Considering the candidate 291302_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291302_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (27.0") between the two second-epoch detections
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Considering the candidate 291303_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291303_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (45.7") between the two second-epoch detections
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Considering the candidate 291304_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291304_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 291311_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291311_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 291312_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291312_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291317_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291317_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 291318_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291318_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291319_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291319_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291320_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291320_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (72.4") between the two second-epoch detections
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Considering the candidate 291321_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291321_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (24.2") between the two second-epoch detections
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Considering the candidate 291328_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291328_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 291334_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291334_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291343_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291343_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291346_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291346_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (25.5") between the two second-epoch detections
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Considering the candidate 291351_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291351_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 291352_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291352_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (24.3") between the two second-epoch detections
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Considering the candidate 291354_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291354_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (24.3") between the two second-epoch detections
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Considering the candidate 291356_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291356_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 291357_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291357_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 291358_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291358_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (25.6") between the two second-epoch detections
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Considering the candidate 291359_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291359_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 291363_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291363_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 291366_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291366_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291380_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291380_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291383_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291383_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 291384_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291384_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 291385_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291385_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291387_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291387_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (51.0") between the two second-epoch detections
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Considering the candidate 291394_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291394_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (25.2") between the two second-epoch detections
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Considering the candidate 291396_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291396_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291398_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291398_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291403_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291403_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291404_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291404_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291409_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291409_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (32.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291412_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291412_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (25.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291419_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291419_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (24.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291427_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291427_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291429_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291429_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (29.0") between the two second-epoch detections
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Considering the candidate 291434_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 291434_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 291441_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291441_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 291446_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291446_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (28.0") between the two second-epoch detections
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Considering the candidate 291447_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291447_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291448_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291448_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 291451_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291451_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (26.2") between the two second-epoch detections
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Considering the candidate 291452_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291452_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (24.4") between the two second-epoch detections
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Considering the candidate 291458_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291458_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291459_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291459_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291460_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291460_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (28.5") between the two second-epoch detections
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Considering the candidate 291472_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291472_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291479_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291479_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 291483_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291483_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (28.9") between the two second-epoch detections
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Considering the candidate 291485_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291485_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291495_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 291495_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 291500_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291500_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 291518_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291518_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291520_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291520_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 291521_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291521_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (33.5") between the two second-epoch detections
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Considering the candidate 291526_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291526_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 291529_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291529_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 291531_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291531_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (30.5") between the two second-epoch detections
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Considering the candidate 291537_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291537_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (40.6") between the two second-epoch detections
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Considering the candidate 291538_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291538_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (34.8") between the two second-epoch detections
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Considering the candidate 291540_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291540_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 291543_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291543_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (41.7") between the two second-epoch detections
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Considering the candidate 291546_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291546_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (31.9") between the two second-epoch detections
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Considering the candidate 291554_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291554_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 291557_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291557_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (38.7") between the two second-epoch detections
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Considering the candidate 291560_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291560_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 291563_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291563_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291565_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291565_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291576_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291576_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291580_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291580_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 291583_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291583_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 291586_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291586_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291593_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291593_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291596_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291596_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291598_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291598_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (49.0") between the two second-epoch detections
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Considering the candidate 291599_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291599_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (40.7") between the two second-epoch detections
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Considering the candidate 291602_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291602_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291610_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291610_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 291619_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 291619_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 291621_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291621_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291623_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291623_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 291628_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291628_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 291629_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291629_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (30.7") between the two second-epoch detections
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Considering the candidate 291631_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291631_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 291633_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291633_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 291635_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291635_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (62.1") between the two second-epoch detections
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Considering the candidate 291637_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291637_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 291643_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291643_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (73.5") between the two second-epoch detections
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Considering the candidate 291644_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291644_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 291646_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291646_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291651_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291651_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (33.4") between the two second-epoch detections
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Considering the candidate 291654_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291654_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (33.8") between the two second-epoch detections
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Considering the candidate 291656_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291656_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (45.8") between the two second-epoch detections
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Considering the candidate 291669_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291669_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291678_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291678_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291684_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291684_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291690_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291690_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 291697_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291697_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (50.4") between the two second-epoch detections
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Considering the candidate 291698_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291698_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (26.6") between the two second-epoch detections
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Considering the candidate 291701_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291701_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (31.4") between the two second-epoch detections
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Considering the candidate 291702_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291702_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291705_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291705_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (33.5") between the two second-epoch detections
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Considering the candidate 291706_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291706_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (27.9") between the two second-epoch detections
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Considering the candidate 291710_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291710_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291713_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291713_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291715_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291715_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (26.7") between the two second-epoch detections
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Considering the candidate 291718_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291718_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291719_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291719_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291725_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291725_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 291727_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291727_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291730_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291730_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 291732_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291732_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (57.1") between the two second-epoch detections
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Considering the candidate 291738_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291738_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291740_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291740_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (31.8") between the two second-epoch detections
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Considering the candidate 291742_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291742_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (35.8") between the two second-epoch detections
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Considering the candidate 291745_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291745_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (26.9") between the two second-epoch detections
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Considering the candidate 291746_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291746_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (62.0") between the two second-epoch detections
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Considering the candidate 291747_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291747_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291752_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291752_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (51.2") between the two second-epoch detections
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Considering the candidate 291754_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291754_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (37.2") between the two second-epoch detections
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Considering the candidate 291755_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291755_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (24.5") between the two second-epoch detections
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Considering the candidate 291766_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291766_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291768_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291768_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (24.7") between the two second-epoch detections
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Considering the candidate 291769_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291769_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (25.5") between the two second-epoch detections
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Considering the candidate 291771_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291771_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291774_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291774_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291775_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291775_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291783_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291783_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 291785_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291785_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 291786_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291786_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (32.6") between the two second-epoch detections
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Considering the candidate 291789_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291789_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 291790_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291790_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 291792_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291792_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 291793_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291793_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (50.2") between the two second-epoch detections
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Considering the candidate 291794_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291794_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 291801_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291801_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (55.4") between the two second-epoch detections
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Considering the candidate 291807_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291807_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 291812_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291812_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (26.2") between the two second-epoch detections
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Considering the candidate 291815_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291815_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291816_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291816_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (23.9") between the two second-epoch detections
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Considering the candidate 291817_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291817_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (28.0") between the two second-epoch detections
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Considering the candidate 291819_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291819_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 291823_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291823_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 291825_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291825_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (64.3") between the two second-epoch detections
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Considering the candidate 291827_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291827_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 291833_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291833_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291834_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291834_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291836_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291836_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291846_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291846_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (24.8") between the two second-epoch detections
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Considering the candidate 291857_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291857_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291862_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291862_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (25.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291864_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 291864_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 291866_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291866_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291872_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291872_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (44.3") between the two second-epoch detections
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Considering the candidate 291877_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291877_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (29.5") between the two second-epoch detections
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Considering the candidate 291879_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291879_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (25.6") between the two second-epoch detections
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Considering the candidate 291880_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291880_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291882_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291882_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (32.0") between the two second-epoch detections
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Considering the candidate 291884_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291884_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291887_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291887_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 291889_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291889_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (26.6") between the two second-epoch detections
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Considering the candidate 291898_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291898_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (72.4") between the two second-epoch detections
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Considering the candidate 291899_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291899_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 291905_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291905_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 291911_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291911_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291919_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291919_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (24.3") between the two second-epoch detections
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Considering the candidate 291920_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291920_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 291922_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291922_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 291923_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291923_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (25.4") between the two second-epoch detections
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Considering the candidate 291924_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291924_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (52.6") between the two second-epoch detections
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Considering the candidate 291925_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291925_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291927_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291927_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (44.8") between the two second-epoch detections
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Considering the candidate 291931_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291931_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291938_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291938_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291949_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291949_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291950_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291950_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 291951_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291951_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (50.9") between the two second-epoch detections
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Considering the candidate 291955_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291955_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291956_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291956_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 291957_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291957_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291965_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291965_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (49.8") between the two second-epoch detections
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Considering the candidate 291966_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291966_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291971_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291971_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291972_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291972_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291976_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291976_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 291978_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291978_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291979_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291979_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (28.9") between the two second-epoch detections
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Considering the candidate 291986_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291986_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 291997_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 291997_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 291998_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291998_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 291999_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 291999_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 292001_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 292001_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 292002_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 292002_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 292003_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 292003_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 292004_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 292004_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 292010_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 292010_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 292012_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 292012_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 292013_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 292013_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 292020_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 292020_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 292022_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 292022_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (24.6") between the two second-epoch detections
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Considering the candidate 292036_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 292036_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 292038_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 292038_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 292039_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 292039_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (24.8") between the two second-epoch detections
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Considering the candidate 292061_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 292061_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (32.5") between the two second-epoch detections
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Considering the candidate 292062_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 292062_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (43.6") between the two second-epoch detections
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Considering the candidate 292063_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 292063_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 292096_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 292096_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 270041_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 270041_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 46140_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
Preparing report for the candidate 46140_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
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Considering the candidate 228912_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 228912_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 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 43402_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 43402_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 199360_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 199360_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 165339_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 165339_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (28.4") between the two second-epoch detections
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Considering the candidate 129229_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 129229_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 09353_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 09353_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (29.0") between the two second-epoch detections
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Considering the candidate 101915_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 101915_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 52172_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 52172_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 71226_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040
The candidate 71226_fd_Mon-02-Q1b1x1_2026-02-11_20-34-45_20.00sec_-15.00C_LIGHT_0040 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 16s
make_report_in_HTML.sh TOTAL: 147s
Prepared the HTML report for the field Mon-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
07:03:31.94 -06:51:29.4
06:56:43.91 +01:26:20.0
06:48:21.76 +01:52:20.8
06:42:35.41 -03:49:12.1
07:19:16.35 -04:07:29.5
06:44:52.76 +00:57:20.4
07:08:05.27 +00:45:21.5
06:26:46.55 -02:31:31.9
06:43:19.13 -00:06:06.1
07:09:39.54 -03:41:35.6
06:40:31.88 -01:56:29.4
06:32:39.38 +00:00:41.9
07:17:35.85 -06:48:24.9
06:51:39.44 -05:32:29.0
06:54:26.26 -06:48:52.4
06:22:42.68 -04:29:34.0
06:52:03.28 -05:41:50.6
06:26:10.15 -04:23:56.9
06:27:05.63 -03:40:28.8
06:27:57.79 -04:38:53.1
07:00:54.52 -00:54:42.9
06:29:16.01 -05:22:08.1
06:22:01.35 -00:57:21.1
06:23:46.23 -00:49:27.1
07:11:19.21 -04:50:00.6
07:15:26.28 -05:02:29.4
06:32:28.29 -06:14:53.5
06:26:45.61 -05:29:39.8
07:01:57.23 -04:01:44.4
06:45:57.54 -04:51:53.3
06:36:42.28 -06:39:03.7
06:28:22.86 -02:24:26.5
06:40:36.79 +00:42:54.7
07:03:42.40 -03:12:23.8
07:03:12.96 -06:38:25.5
07:18:23.97 -05:47:39.4
06:26:19.83 -03:10:06.0
06:45:00.47 -01:02:29.0
06:43:46.29 +01:35:38.6
06:29:51.32 -02:40:55.8
07:07:00.24 -03:22:51.2
06:22:25.50 -01:43:06.2
07:05:13.44 +00:16:02.7
07:11:47.52 -05:22:25.6
07:09:43.75 -04:05:45.4
06:35:20.75 -05:17:45.1
06:24:07.67 -00:49:42.8
06:44:44.78 +01:05:28.3
07:03:17.93 -01:02:24.2
06:51:24.83 -02:44:46.9
07:01:09.23 -00:46:26.5
06:51:23.90 -02:32:46.5
06:51:28.52 -02:44:47.3
06:51:00.55 -02:21:47.5
06:26:55.37 -03:31:10.4
06:41:30.90 +02:27:57.4
07:10:57.08 -05:23:30.6
06:25:59.45 -04:36:09.2
07:10:42.50 -04:48:58.8
06:32:47.52 -05:35:10.3
07:14:25.55 -05:34:56.1
07:00:21.19 -00:45:49.8
06:48:12.64 +01:01:03.7
07:10:14.25 -05:11:56.3
########### Completed Mon-02-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
06:56:43.91 +01:26:20.0
06:48:21.76 +01:52:20.8
06:42:35.41 -03:49:12.1
07:19:16.35 -04:07:29.5
06:44:52.76 +00:57:20.4
07:08:05.27 +00:45:21.5
06:26:46.55 -02:31:31.9
06:43:19.13 -00:06:06.1
07:09:39.54 -03:41:35.6
06:40:31.88 -01:56:29.4
06:32:39.38 +00:00:41.9
07:17:35.85 -06:48:24.9
06:51:39.44 -05:32:29.0
06:54:26.26 -06:48:52.4
06:22:42.68 -04:29:34.0
06:52:03.28 -05:41:50.6
06:26:10.15 -04:23:56.9
07:03:31.94 -06:51:29.4
06:27:05.63 -03:40:28.8
06:27:57.79 -04:38:53.1
07:00:54.52 -00:54:42.9
06:29:16.01 -05:22:08.1
06:22:01.35 -00:57:21.1
06:23:46.23 -00:49:27.1
07:11:19.21 -04:50:00.6
07:15:26.28 -05:02:29.4
06:32:28.29 -06:14:53.5
06:26:45.61 -05:29:39.8
07:01:57.23 -04:01:44.4
06:45:57.54 -04:51:53.3
06:36:42.28 -06:39:03.7
06:28:22.86 -02:24:26.5
06:40:36.79 +00:42:54.7
07:03:42.40 -03:12:23.8
07:03:12.96 -06:38:25.5
07:18:23.97 -05:47:39.4
06:26:19.83 -03:10:06.0
06:45:00.47 -01:02:29.0
06:43:46.29 +01:35:38.6
06:29:51.32 -02:40:55.8
07:07:00.24 -03:22:51.2
06:22:25.50 -01:43:06.2
07:05:13.44 +00:16:02.7
07:11:47.52 -05:22:25.6
07:09:43.75 -04:05:45.4
06:35:20.75 -05:17:45.1
06:24:07.67 -00:49:42.8
06:44:44.78 +01:05:28.3
07:03:17.93 -01:02:24.2
06:51:24.83 -02:44:46.9
07:01:09.23 -00:46:26.5
06:51:23.90 -02:32:46.5
06:51:28.52 -02:44:47.3
06:51:00.55 -02:21:47.5
06:26:55.37 -03:31:10.4
06:41:30.90 +02:27:57.4
07:10:57.08 -05:23:30.6
06:25:59.45 -04:36:09.2
07:10:42.50 -04:48:58.8
06:32:47.52 -05:35:10.3
07:14:25.55 -05:34:56.1
07:00:21.19 -00:45:49.8
06:48:12.64 +01:01:03.7
07:10:14.25 -05:11:56.3
###################################################################################
06:56:43.91 +01:26:20.0 -- not an asteroid (will add it to exclusion list)
06:48:21.76 +01:52:20.8 -- not an asteroid (will add it to exclusion list)
06:42:35.41 -03:49:12.1 -- not an asteroid (will add it to exclusion list)
07:19:16.35 -04:07:29.5 -- not an asteroid (will add it to exclusion list)
06:44:52.76 +00:57:20.4 -- not an asteroid (will add it to exclusion list)
07:08:05.27 +00:45:21.5 -- not an asteroid (will add it to exclusion list)
06:26:46.55 -02:31:31.9 -- not an asteroid (will add it to exclusion list)
06:43:19.13 -00:06:06.1 -- not an asteroid (will add it to exclusion list)
07:09:39.54 -03:41:35.6 -- not an asteroid (will add it to exclusion list)
06:40:31.88 -01:56:29.4 -- not an asteroid (will add it to exclusion list)
06:32:39.38 +00:00:41.9 -- not an asteroid (will add it to exclusion list)
07:17:35.85 -06:48:24.9 -- not an asteroid (will add it to exclusion list)
06:51:39.44 -05:32:29.0 -- not an asteroid (will add it to exclusion list)
06:54:26.26 -06:48:52.4 -- not an asteroid (will add it to exclusion list)
06:22:42.68 -04:29:34.0 -- not an asteroid (will add it to exclusion list)
06:52:03.28 -05:41:50.6 -- not an asteroid (will add it to exclusion list)
06:26:10.15 -04:23:56.9 -- not an asteroid (will add it to exclusion list)
07:03:31.94 -06:51:29.4 -- not an asteroid (will add it to exclusion list)
06:27:05.63 -03:40:28.8 -- not an asteroid (will add it to exclusion list)
06:27:57.79 -04:38:53.1 -- not an asteroid (will add it to exclusion list)
07:00:54.52 -00:54:42.9 -- not an asteroid (will add it to exclusion list)
06:29:16.01 -05:22:08.1 -- not an asteroid (will add it to exclusion list)
06:22:01.35 -00:57:21.1 -- not an asteroid (will add it to exclusion list)
06:23:46.23 -00:49:27.1 -- not an asteroid (will add it to exclusion list)
07:11:19.21 -04:50:00.6 -- not an asteroid (will add it to exclusion list)
07:15:26.28 -05:02:29.4 -- not an asteroid (will add it to exclusion list)
06:32:28.29 -06:14:53.5 -- not an asteroid (will add it to exclusion list)
06:26:45.61 -05:29:39.8 -- not an asteroid (will add it to exclusion list)
07:01:57.23 -04:01:44.4 -- not an asteroid (will add it to exclusion list)
06:45:57.54 -04:51:53.3 -- not an asteroid (will add it to exclusion list)
06:36:42.28 -06:39:03.7 -- not an asteroid (will add it to exclusion list)
06:28:22.86 -02:24:26.5 -- not an asteroid (will add it to exclusion list)
06:40:36.79 +00:42:54.7 -- not an asteroid (will add it to exclusion list)
07:03:42.40 -03:12:23.8 -- not an asteroid (will add it to exclusion list)
07:03:12.96 -06:38:25.5 -- not an asteroid (will add it to exclusion list)
07:18:23.97 -05:47:39.4 -- not an asteroid (will add it to exclusion list)
06:26:19.83 -03:10:06.0 -- not an asteroid (will add it to exclusion list)
06:45:00.47 -01:02:29.0 -- not an asteroid (will add it to exclusion list)
06:43:46.29 +01:35:38.6 -- not an asteroid (will add it to exclusion list)
06:29:51.32 -02:40:55.8 -- not an asteroid (will add it to exclusion list)
07:07:00.24 -03:22:51.2 -- not an asteroid (will add it to exclusion list)
06:22:25.50 -01:43:06.2 -- not an asteroid (will add it to exclusion list)
07:05:13.44 +00:16:02.7 -- not an asteroid (will add it to exclusion list)
07:11:47.52 -05:22:25.6 -- not an asteroid (will add it to exclusion list)
07:09:43.75 -04:05:45.4 -- not an asteroid (will add it to exclusion list)
06:35:20.75 -05:17:45.1 -- not an asteroid (will add it to exclusion list)
06:24:07.67 -00:49:42.8 -- not an asteroid (will add it to exclusion list)
06:44:44.78 +01:05:28.3 -- not an asteroid (will add it to exclusion list)
07:03:17.93 -01:02:24.2 -- not an asteroid (will add it to exclusion list)
06:51:24.83 -02:44:46.9 -- not an asteroid (will add it to exclusion list)
07:01:09.23 -00:46:26.5 -- not an asteroid (will add it to exclusion list)
06:51:23.90 -02:32:46.5 -- not an asteroid (will add it to exclusion list)
06:51:28.52 -02:44:47.3 -- not an asteroid (will add it to exclusion list)
06:51:00.55 -02:21:47.5 -- not an asteroid (will add it to exclusion list)
06:26:55.37 -03:31:10.4 -- not an asteroid (will add it to exclusion list)
06:41:30.90 +02:27:57.4 -- not an asteroid (will add it to exclusion list)
07:10:57.08 -05:23:30.6 -- not an asteroid (will add it to exclusion list)
06:25:59.45 -04:36:09.2 -- not an asteroid (will add it to exclusion list)
07:10:42.50 -04:48:58.8 -- not an asteroid (will add it to exclusion list)
06:32:47.52 -05:35:10.3 -- not an asteroid (will add it to exclusion list)
07:14:25.55 -05:34:56.1 -- not an asteroid (will add it to exclusion list)
07:00:21.19 -00:45:49.8 -- not an asteroid (will add it to exclusion list)
06:48:12.64 +01:01:03.7 -- not an asteroid (will add it to exclusion list)
07:10:14.25 -05:11:56.3 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
06:22:01.35 -00:57:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:25.50 -01:43:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:42.68 -04:29:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:23:46.23 -00:49:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:24:07.67 -00:49:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:59.45 -04:36:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:10.15 -04:23:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:19.83 -03:10:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:45.61 -05:29:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:46.55 -02:31:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:55.37 -03:31:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:05.63 -03:40:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:57.79 -04:38:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:28:22.86 -02:24:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:29:16.01 -05:22:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:29:51.32 -02:40:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:32:28.29 -06:14:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:32:39.38 +00:00:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:32:47.52 -05:35:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:20.75 -05:17:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:36:42.28 -06:39:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:31.88 -01:56:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:36.79 +00:42:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:30.90 +02:27:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:35.41 -03:49:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:19.13 -00:06:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:46.29 +01:35:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:44.78 +01:05:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:52.76 +00:57:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:00.47 -01:02:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:57.54 -04:51:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:12.64 +01:01:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:21.76 +01:52:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:00.55 -02:21:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:23.90 -02:32:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:24.83 -02:44:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:28.52 -02:44:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:39.44 -05:32:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:03.28 -05:41:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:26.26 -06:48:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:43.91 +01:26:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:21.19 -00:45:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:54.52 -00:54:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:09.23 -00:46:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:57.23 -04:01:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:12.96 -06:38:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:17.93 -01:02:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:31.94 -06:51:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:42.40 -03:12:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:13.44 +00:16:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:00.24 -03:22:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:05.27 +00:45:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:39.54 -03:41:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:43.75 -04:05:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:14.25 -05:11:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:42.50 -04:48:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:10:57.08 -05:23:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:19.21 -04:50:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:11:47.52 -05:22:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:14:25.55 -05:34:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:15:26.28 -05:02:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:17:35.85 -06:48:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:18:23.97 -05:47:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:19:16.35 -04:07:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
06:22:01.35 -00:57:21.1 -- not a known variable star
06:22:25.50 -01:43:06.2 -- not a known variable star
06:22:42.68 -04:29:34.0 -- not a known variable star
06:23:46.23 -00:49:27.1 -- not a known variable star
06:24:07.67 -00:49:42.8 -- not a known variable star
06:25:59.45 -04:36:09.2 -- not a known variable star
06:26:10.15 -04:23:56.9 -- not a known variable star
06:26:19.83 -03:10:06.0 -- not a known variable star
06:26:45.61 -05:29:39.8 -- not a known variable star
06:26:46.55 -02:31:31.9 -- a known variable star
06:26:55.37 -03:31:10.4 -- not a known variable star
06:27:05.63 -03:40:28.8 -- not a known variable star
06:27:57.79 -04:38:53.1 -- not a known variable star
06:28:22.86 -02:24:26.5 -- not a known variable star
06:29:16.01 -05:22:08.1 -- not a known variable star
06:29:51.32 -02:40:55.8 -- not a known variable star
06:32:28.29 -06:14:53.5 -- not a known variable star
06:32:39.38 +00:00:41.9 -- not a known variable star
06:32:47.52 -05:35:10.3 -- not a known variable star
06:35:20.75 -05:17:45.1 -- not a known variable star
06:36:42.28 -06:39:03.7 -- not a known variable star
06:40:31.88 -01:56:29.4 -- not a known variable star
06:40:36.79 +00:42:54.7 -- a known variable star
06:41:30.90 +02:27:57.4 -- not a known variable star
06:42:35.41 -03:49:12.1 -- not a known variable star
06:43:19.13 -00:06:06.1 -- not a known variable star
06:43:46.29 +01:35:38.6 -- not a known variable star
06:44:44.78 +01:05:28.3 -- not a known variable star
06:44:52.76 +00:57:20.4 -- not a known variable star
06:45:00.47 -01:02:29.0 -- not a known variable star
06:45:57.54 -04:51:53.3 -- not a known variable star
06:48:12.64 +01:01:03.7 -- not a known variable star
06:48:21.76 +01:52:20.8 -- not a known variable star
06:51:00.55 -02:21:47.5 -- not a known variable star
06:51:23.90 -02:32:46.5 -- not a known variable star
06:51:24.83 -02:44:46.9 -- not a known variable star
06:51:28.52 -02:44:47.3 -- not a known variable star
06:51:39.44 -05:32:29.0 -- not a known variable star
06:52:03.28 -05:41:50.6 -- not a known variable star
06:54:26.26 -06:48:52.4 -- not a known variable star
06:56:43.91 +01:26:20.0 -- not a known variable star
07:00:21.19 -00:45:49.8 -- not a known variable star
07:00:54.52 -00:54:42.9 -- not a known variable star
07:01:09.23 -00:46:26.5 -- not a known variable star
07:01:57.23 -04:01:44.4 -- not a known variable star
07:03:12.96 -06:38:25.5 -- not a known variable star
07:03:17.93 -01:02:24.2 -- not a known variable star
07:03:31.94 -06:51:29.4 -- not a known variable star
07:03:42.40 -03:12:23.8 -- not a known variable star
07:05:13.44 +00:16:02.7 -- not a known variable star
07:07:00.24 -03:22:51.2 -- not a known variable star
07:08:05.27 +00:45:21.5 -- not a known variable star
07:09:39.54 -03:41:35.6 -- not a known variable star
07:09:43.75 -04:05:45.4 -- not a known variable star
07:10:14.25 -05:11:56.3 -- not a known variable star
07:10:42.50 -04:48:58.8 -- not a known variable star
07:10:57.08 -05:23:30.6 -- not a known variable star
07:11:19.21 -04:50:00.6 -- a known variable star
07:11:47.52 -05:22:25.6 -- a known variable star
07:14:25.55 -05:34:56.1 -- not a known variable star
07:15:26.28 -05:02:29.4 -- not a known variable star
07:17:35.85 -06:48:24.9 -- not a known variable star
07:18:23.97 -05:47:39.4 -- not a known variable star
07:19:16.35 -04:07:29.5 -- not a known variable star
Found 60 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
64 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 64 (excluding asteroids and hot pixels), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is 500
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461083.60713390 -observatory 500
22:41:02.11 -08:54:43.5 Mercury (-1.1mag)
22:17:06.18 -12:13:17.2 Venus (-3.9mag)
21:11:28.29 -17:20:18.3 Mars (1.1mag)
07:09:08.49 +22:48:37.0 Jupiter (-2.6mag)
00:01:19.02 -02:12:11.4 Saturn (1.0mag)
03:39:31.09 +19:19:57.7 Uranus (5.7mag)
00:02:27.84 -01:09:43.6 Neptune (7.8mag)
20:27:50.36 -23:02:39.5 Pluto (14.6mag)
17:19:26.90 -28:15:27.1 Moon (-9.6mag)
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Positions of selected moons from JPL HORIZONS for JD(UT)2461083.60713390:
07:09:12.13 +22:48:26.5 Io (5.3mag)
07:09:20.71 +22:48:09.6 Europa (5.5mag)
07:09:01.94 +22:48:40.6 Ganymede (4.8mag)
07:09:14.59 +22:48:12.5 Callisto (6.0mag)
07:11:24.16 +23:08:59.3 Himalia (15.0mag)
07:09:11.82 +22:48:32.0 Thebe (15.8mag)
07:11:01.90 +23:11:38.4 Elara (17.0mag)
07:04:13.98 +24:01:47.2 Pasiphae (17.0mag)
07:18:09.53 +22:33:27.3 Carme (18.0mag)
00:01:14.94 -02:11:51.9 Titan (8.7mag)
00:01:19.18 -02:12:06.5 Rhea (10.1mag)
00:00:53.94 -02:13:54.7 Iapetus (11.5mag)
00:01:22.48 -02:11:57.9 Hyperion (14.7mag)
00:03:24.97 -01:58:46.3 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Feb 11 20:39 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461083.60713390:
07:39:28.19 +22:54:25.8 JWST
16:20:21.08 +48:48:35.7 Chandra
14:29:10.50 -63:10:20.1 XMM-Newton
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Positions of bright comets (listed at http://astro.vanbuitenen.nl/comets and http://aerith.net/comet/weekly/current.html ) from JPL HORIZONS for JD(UT)2461083.60713390 at 500
16:40:21.08 -10:50:59.3 17.7mag 10P/Tempel
03:28:48.24 +28:25:26.2 18.1mag 123P/West-Hartley
20:47:30.62 -10:12:28.7 22.4mag 141P/Machholz
00:59:14.77 +09:01:56.9 17.6mag 145P/Shoemaker-Levy 5
11:12:08.95 +29:15:51.1 17.8mag 164P/Christensen
09:38:52.91 -34:07:51.9 18.0mag 195P/Hill
15:50:57.33 -07:26:18.2 18.5mag 210P/Christensen
17:29:29.73 -21:38:10.5 17.4mag 218P/LINEAR
16:03:37.40 -18:17:28.7 15.2mag 235P/LINEAR
03:43:09.33 +25:49:05.0 17.5mag 240P/NEAT
15:02:30.15 +07:31:24.7 14.6mag 24P/Schaumasse
23:53:53.79 +04:16:18.8 18.1mag 261P/Larson
11:27:19.55 -03:35:56.5 17.4mag 29P/Schwassmann-Wachmann 1
01:07:02.77 +01:24:33.1 18.9mag 302P/Lemmon-PanSTARRS
07:06:43.55 +27:16:59.6 19.7mag 407P/PanSTARRS-Fuls
16:49:30.74 -11:18:32.9 17.5mag 40P/Vaisala 1
11:08:16.00 -09:16:11.5 16.6mag 43P/Wolf-Harrington
13:22:44.31 -05:07:02.6 19.4mag 489P/Denning
04:27:57.22 +49:25:36.5 17.7mag 493P/2024 Q2 (LONEOS)
06:02:40.28 +49:19:27.3 17.8mag 63P/Wild 1
22:54:50.20 -03:55:15.4 16.3mag 78P/Gehrels 2
19:23:43.53 -23:29:49.2 15.1mag 88P/Howell
15:21:56.24 -28:09:47.3 18.7mag P/2023 S1 (PanSTARRS)
04:43:16.03 -73:09:43.8 16.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:31:42.58 +31:11:06.5 18.1mag C/2017 K2 (PanSTARRS)
20:00:42.60 -64:56:03.0 18.1mag C/2020 V2 (ZTF)
17:17:00.66 +03:20:51.9 16.3mag C/2021 G2 (ATLAS)
22:45:43.69 +28:37:04.6 16.8mag C/2022 E2 (ATLAS)
03:28:12.85 +24:26:26.2 15.7mag C/2022 N2 (PANSTARRS)
09:11:55.60 +28:56:34.9 15.3mag C/2022 QE78 (ATLAS)
08:38:59.56 -07:45:39.3 16.6mag C/2022 R6 (PanSTARRS)
23:40:30.27 +48:06:21.5 17.9mag C/2023 C2 (ATLAS)
10:02:21.79 -22:06:48.3 17.5mag C/2023 F3 (ATLAS)
20:13:40.62 +61:17:22.1 17.2mag C/2023 H5 (Lemmon)
19:32:53.15 -03:17:35.8 16.1mag C/2023 R1 (PANSTARRS)
02:45:54.78 +35:47:19.6 18.5mag C/2023 RS61 (PanSTARRS)
20:43:13.98 +81:15:37.6 18.0mag C/2023 X2 (Lemmon)
06:55:45.68 +63:24:50.1 17.2mag C/2024 A1 (ATLAS)
00:29:10.38 -37:01:31.4 10.8mag C/2024 E1 (Wierzchos)
11:52:30.11 -04:24:25.4 18.1mag C/2024 G2 (ATLAS)
19:18:26.24 +00:21:01.3 19.0mag C/2024 G4 (PanSTARRS)
16:36:58.18 -02:57:46.6 17.8mag C/2024 G6 (ATLAS)
19:46:21.80 +01:29:30.8 15.7mag C/2024 J3 (ATLAS)
02:42:26.86 -33:28:53.4 15.4mag C/2024 T5 (ATLAS)
16:46:38.28 -54:17:42.8 15.3mag C/2025 A6 (Lemmon)
04:55:20.62 +66:17:41.9 16.7mag C/2025 J1 (Borisov)
00:00:00.00 +00:00:00.0 cannot get JPL HORIZONS ephemerides for non-periodic comet C/2025 K1 (ATLAS)
16:01:12.16 -20:17:19.7 15.0mag C/2025 L1 (ATLAS)
02:12:34.49 -17:35:45.5 16.6mag C/2025 Q3 (ATLAS)
01:56:42.11 +16:18:31.6 20.7mag C/2025 R2 (SWAN)
22:17:23.73 +17:32:38.7 16.8mag C/2025 R3 (PANSTARRS)
21:35:02.58 -14:38:52.7 20.4mag C/2025 T1 (ATLAS)
03:31:31.64 -25:12:44.2 17.4mag C/2026 A1 (MAPS)
20:25:16.67 +16:10:37.4 16.6mag C/2026 B2 (Sun-Gao)
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
18:16:39.86 -19:51:57.30 TCP J06282145-1950371 2026-02-9.38 15.25
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
00:12:55.45 +33:21:25.90 SN2026cbh 2026-02-7.09 16.33
08:02:12.64 -04:14:20.90 SN 2026auh 2026-02-7.11 16.64
18:03:52.67 -31:27:26.00 TCP J18035290-3127298 2026-02-7.37 15.76
12:18:03.59 +50:27:10.20 SN 2026bjz 2026-02-7.25 16.48
07:51:51.12 +55:05:27.60 SN 2026ail 2026-02-6.21 16.85
08:10:56.38 +36:49:42.80 AT2026bsa 2026-02-6.29 17.47
04:43:45.47 -15:49:01.00 SN2026azr 2026-02-5.24 16.96
06:14:48.48 -34:20:08.90 ASASSN-26ap 2026-02-5.2 13.77
02:42:33.90 -27:21:02.60 SN 2026aip 2026-02-4.09 15.85
00:43:12.26 +38:35:47.90 AT2026brt 2026-02-3.12 14.92
14:34:27.21 +21:56:59.90 SN2026atb 2026-01-29.32 15.59
13:12:04.11 -60:56:12.40 ASASSN-26ao 2026-01-28.35 15.61
13:00:36.49 -06:28:26.00 SN2026azd 2026-01-28.23 15.69
10:33:50.27 -31:00:53.40 SN 2026ayz 2026-01-25.11 15.3
05:14:22.36 -60:47:20.70 SN 2026apb 2026-01-24.08 17.35
06:39:26.57 -21:49:19.60 AT2026afe 2026-01-23.11 16.17
09:27:23.49 -32:00:30.90 SN 2023kuy 2026-01-21.16 15.43
09:38:44.42 -20:00:54.30 SN2026afi 2026-01-20.24 17.43
06:30:51.72 -74:35:50.10 AT2026ahr 2026-01-20.19 17.09
13:33:03.15 -16:14:28.70 SN2026amc 2026-01-20.29 16.9
06:57:11.13 -17:24:42.80 ASASSN-26an 2026-01-19.31 13.99
17:41:29.59 +68:57:34.90 2026abj 2026-01-18.64 17.02
10:22:24.99 +04:00:02.20 SN 2026kc 2026-01-18.61 16.1
12:42:03.30 +00:41:41.80 SN 2026pg 2026-01-18.5 17.44
03:36:21.80 -31:44:39.30 AT2025aibn 2026-01-17.04 16.7
13:45:00.71 -32:34:53.00 AT2026yi 2026-01-17.26 16.22
09:27:07.17 +62:45:24.20 AT2026nu 2026-01-17.29 17.09
12:38:41.73 +07:36:37.40 SN 2025afcr 2026-01-17.49 17.11
12:12:12.65 +13:13:18.50 SN 2026acd 2026-01-17.3 16.15
16:21:54.73 -63:36:53.10 ASASSN-26al 2026-01-17.36 15.34
15:33:45.22 -22:11:07.90 ASASSN-26aj 2026-01-16.51 14
12:27:08.33 -58:19:36.10 ASASSN-26ak 2026-01-16.2 13.94
17:21:53.10 +04:39:07.10 ASASSN-26ai 2026-01-16.67 14.83
14:46:54.08 -64:04:30.10 ASASSN-26ah 2026-01-15.07 16.84
23:02:43.24 +20:04:53.00 SN2025ajvh 2026-01-15.07 16.03
14:12:27.38 -30:12:29.10 ASASSN-26ag 2026-01-14.27 15.35
14:33:53.58 +05:27:35.40 SN 2025ajnc 2026-01-14.32 15.79
01:43:00.31 -34:11:40.60 AT2025afcm 2026-01-13.08 0.45
00:26:17.71 -52:11:38.60 AT2025ahal 2026-01-11.06 17.57
00:51:36.17 +29:42:40.10 SN2025ahxd 2026-01-11.21 15
10:19:19.14 -37:54:58.30 AT2025ahrt 2026-01-10.26 -0.54
14:37:48.78 +15:51:04.20 SN2025ajng 2026-01-9.42 16.35
05:01:03.70 -08:34:13.20 SN2026A 2026-01-9.28 16.83
00:02:52.11 +13:05:42.90 SN2025ajvg 2026-01-9.13 15.89
08:37:09.62 -02:18:08.80 SN2025aigm 2026-01-9.55 17.66
09:52:50.71 +39:36:55.70 SN2025ahyt 2026-01-9.37 16.97
11:22:19.08 -27:21:40.90 AT2026ta 2026-01-9.32 15.88
14:35:00.21 +00:59:11.40 SN 2025ahsa 2026-01-8.35 -2
09:25:42.42 +22:20:06.10 SN2025ahkt 2026-01-8.03 15.88
22:39:53.44 +34:53:50.00 SN 2025aikz 2026-01-7.09 16.3
08:21:20.95 +20:52:01.60 SN 2025aiks 2026-01-7.13 15.82
07:35:31.38 +09:10:32.40 AT2025ajvk 2026-01-7.12 -1.82
02:50:07.71 -16:37:02.30 AT2026nl 2026-01-7.16 14.19
14:05:12.75 -33:46:00.80 SN 2025ajmj 2026-01-7.31 14.93
12:35:08.33 +28:03:22.70 SN 2025aiaj 2026-01-5.44 15.76
05:30:00.47 -66:43:29.40 ASASSN-26af 2026-01-5.12 14.38
14:05:05.13 -44:14:24.00 ASASSN-26ac 2026-01-5.3 16.01
11:29:16.57 +20:35:09.00 AT2025alco 2026-01-4.39 15.93
16:42:59.28 +26:21:02.80 ASASSN-26ae 2026-01-4.52 14.31
04:13:46.60 -05:02:16.60 ASASSN-26ad 2026-01-4.32 14.58
05:00:01.32 -57:14:29.70 ASASSN-25fj/ASASSN-26ab 2026-01-1.19 13.38
13:53:51.35 -17:55:38.10 ASASSN-25fg 2025-12-23.33 16.66
06:18:15.27 +15:47:38.10 AT2025ahtd 2025-12-23.31 16.96
07:20:53.12 -33:02:58.20 SN 2025agvw 2025-12-23.32 16.84
02:58:15.63 +44:47:45.80 ASASSN-25fh 2025-12-23.13 15.63
04:51:03.78 -36:13:59.00 AT2025aftm 2025-12-20.14 17.35
03:12:59.31 +17:41:45.20 SN2025afzm 2025-12-20.15 17.22
13:33:14.27 -46:03:33.90 ASASSN-25fc 2025-12-19.32 SDSS
07:07:30.84 +24:37:55.60 SN2025agie 2025-12-19.19 16.96
12:31:24.34 -59:07:09.00 ASASSN-25fd 2025-12-19.06 14.94
14:02:20.59 -20:28:28.70 ASASSN-25fe 2025-12-19.34 SDSS
08:08:51.65 -16:39:31.50 ASASSN-25ff 2025-12-19.22 SDSS
00:34:05.69 +05:21:07.50 SN2025afty 2025-12-18.21 16.92
01:35:25.55 -05:40:42.00 AT2025agsf 2025-12-18.12 17.67
06:12:00.84 -46:50:40.70 AT2025aetd 2025-12-15.08 17.32
11:07:12.05 -55:12:59.00 ASASSN-25fa 2025-12-14.25 16.07
02:48:09.78 +37:45:17.90 AT2025afje 2025-12-13.28 17.65
08:17:38.99 +59:57:25.90 SN2025afcy 2025-12-13.43 16.8
22:58:25.70 +26:38:19.80 SN 2025afve 2025-12-12.1 16.63
03:44:52.10 -59:08:22.80 SN 2025aegk 2025-12-12.1 SDSS
04:55:47.45 -18:56:49.70 SN 2025aetg 2025-12-11.36 16.92
23:15:07.77 +13:10:19.80 SN 2025afwb 2025-12-11.2 17.13
02:19:39.33 -45:39:00.60 SN 2025aeqg 2025-12-10.07 16.77
02:03:03.89 +04:14:37.30 SN2025afih 2025-12-8.1 16.49
22:23:03.49 -56:35:57.50 AT2025aeei 2025-12-8.03 16.01
07:40:22.22 -10:00:59.30 AT2025aftz 2025-12-8.46 15.46
18:44:55.93 +47:57:37.60 ASASSN-25ez 2025-12-3.07 15.16
22:41:03.48 +38:58:01.90 ASASSN-25ey 2025-11-26.08 15.68
05:50:46.62 +58:54:53.50 SN 2025aedz 2025-11-24.25 16.66
06:35:50.19 -71:30:42.00 SN 2025adwn 2025-11-24.11 17.58
02:21:35.59 -14:18:04.90 AT2025aeft 2025-11-23.13 16.82
01:42:47.75 +12:31:45.10 AT2025aduf 2025-11-23.15 17.49
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:28.44 +41:18:24.5 TCP J00422844+4118245 2025-12-22.8736 18.5mag
16:42:59.22 +26:21:02.0 TCP J16425922+2621020 2025-12-26.8538 13.0mag
08:08:08.72 -19:48:46.5 TCP J08080872-1948465 2025-12-27.7904 16.66Cmag
00:42:58.48 +41:08:11.4 PNV J00425848+4108114 2025-12-28.7654 18.9mag
07:35:31.47 +09:10:34.1 TCP J07353147+0910341 2025-12-29.7527 14.77Cmag
14:45:58.45 +39:05:10.3 TCP J14455845+3905103 2025-12-30.8196 14.1mag
00:43:23.44 +41:24:35.7 PNV J00432344+4124357 2025-12-11.684 19.7mag
00:41:01.11 +41:59:28.2 PNV J00410111+4159282 2026-01-06.1994 18.7mag
00:42:52.01 +41:14:29.2 PNV J00425201+4114292 2026-01-08.7863 18.37Cmag
02:50:07.72 -16:37:02.3 TCP J02500772-1637023 2026-01-06.6352 14.53Cmag
00:42:58.52 +41:14:44.2 PNV J00425852+4114442 2026-01-13.4991 16.89Cmag
14:47:33.95 -10:02:56.8 TCP J14473395-1002568 2026-01-13.8185 14.0mag
15:33:45.28 -22:11:07.3 TCP J15334528-2211073 2026-01-16.8451 14.9mag
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
-rw-r--r-- 1 apache apache 186K Feb 11 20:39 tocp_transients_list.txt
