This analysis is done by the script util/transients/transient_factory_test31.sh /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 01 09.1091 2461049.6091 13.57 06:43:17.23 -01:32:49.7
213.38051 -2.51867 galactic Mon Second-epoch detections are separated by 8.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J100.8267-01.5477 | 06:43:17.23 -01:32:49.7 (user input) | IRR (ATLAS) | (ATLAS) | (position from user input) SpType: B5V 2012A&A...541A..34S CoRoT 102683571
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J100.8267-01.5477,2461049.6091,13.57,0.05,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
ATO J100.8267-01.5477 20260109.1091 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 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:43:17.23 -01:32:49.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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 3107171584665401984,2461049.6091,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107171584665401984 20260109.1091 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:47:27.75 -01:05:52.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 09.1091 2461049.6091 13.22 06:53:43.23 -01:58:44.2
214.95332 -0.39464 galactic Mon Second-epoch detections are separated by 4.8" and 7.7 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 J103.4280-01.9828 | 06:53:43.23 -01:58:44.2 (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 J103.4280-01.9828,2461049.6091,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.4280-01.9828 20260109.1091 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:53:43.23 -01:58:44.2 ;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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 09.1091 2461049.6091 13.23 06:46:20.64 -02:03:21.6
214.18199 -2.07031 galactic Mon Second-epoch detections are separated by 6.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J101.5853-02.0511 | 06:46:20.64 -02:03:21.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A7V 2012A&A...541A..34S CoRoT 102812123 J-Ks=0.248+/-0.043 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.5853-02.0511,2461049.6091,13.23,0.05,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
ATO J101.5853-02.0511 20260109.1091 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 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:46:20.64 -02:03:21.6 ;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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 09.1091 2461049.6091 12.59 06:22:10.41 +00:08:29.5
209.45492 -6.44258 galactic Mon Second-epoch detections are separated by 6.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3123251255025970944 | 06:22:09.33 +00:08:41.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.504+/-0.031 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3123251255025970944,2461049.6091,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3123251255025970944 20260109.1091 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:22:10.41 +00:08:29.5 ;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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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 3125569957548660864,2461049.6091,12.54,0.05,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
Gaia DR3 3125569957548660864 20260109.1091 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:43:16.41 +00:21:46.5 ;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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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 3102372667384237952,2461049.6091,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3102372667384237952 20260109.1091 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:48:31.57 -04:05:33.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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 3107234982682679808,2461049.6091,12.11,0.05,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 3107234982682679808 20260109.1091 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:41:45.09 -01:18:58.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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 3112276892032630400,2461049.6091,11.32,0.05,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 3112276892032630400 20260109.1091 11.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:53:11.31 -01:33:35.1 ;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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 09.1091 2461049.6091 11.36 07:07:08.48 -01:48:52.0
216.34000 2.66322 galactic Mon Second-epoch detections are separated by 4.7" and 7.6 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 J106.7877-01.8072 | 07:07:08.48 -01:48:52.0 (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 J106.7877-01.8072,2461049.6091,11.36,0.05,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 J106.7877-01.8072 20260109.1091 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:07:08.48 -01:48:52.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 09.1091 2461049.6091 10.79 06:45:58.98 -04:51:49.3
216.64504 -3.42637 galactic Mon Second-epoch detections are separated by 3.5" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3102224370754086784 | 06:46:00.26 -04:51:50.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1949AnHar.112....1C HD 295492 J-Ks=0.081+/-0.035 (A)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3102224370754086784,2461049.6091,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3102224370754086784 20260109.1091 10.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:45:58.98 -04:51:49.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 09.1091 2461049.6091 11.13 06:50:14.52 -00:47:14.3
213.49631 -0.62506 galactic Mon Second-epoch detections are separated by 3.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3113144097467624576 | 06:50:13.96 -00:47:41.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K5 1947AnDea...5....1L DO 1787 J-Ks=0.200+/-0.044 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113144097467624576,2461049.6091,11.13,0.05,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 3113144097467624576 20260109.1091 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:50:14.52 -00:47:14.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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
VARIABLE_NAME,2461049.6091,12.21,0.05,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
VARIABLE_NAME 20260109.1091 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:40:08.69 +01:55:36.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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 3106074070200575616,2461049.6091,12.48,0.05,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
Gaia DR3 3106074070200575616 20260109.1091 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 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:53:07.27 -01:52:43.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 09.1091 2461049.6091 12.62 06:42:39.05 -02:16:11.3
213.95227 -2.98917 galactic Mon Second-epoch detections are separated by 6.7" and 7.5 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 J100.6619-02.2718 | 06:42:39.05 -02:16:11.3 (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 J100.6619-02.2718,2461049.6091,12.62,0.05,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
ATO J100.6619-02.2718 20260109.1091 12.62CV 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 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:42:39.05 -02:16:11.3 ;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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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,2461049.6091,13.06,0.05,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
target 20260109.1091 13.06CV 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 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:27:32.51 +01:54:48.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 09.1091 2461049.6091 12.96 06:21:27.52 -02:10:49.4
211.45329 -7.66328 galactic Mon Second-epoch detections are separated by 7.9" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:21:27.52 -02:10:49.4 (user input) | T | P | (position from user input) SpType: G5 (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
target,2461049.6091,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260109.1091 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:21:27.52 -02:10:49.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 09.1091 2461049.6091 13.06 06:49:24.48 -00:56:19.2
213.53600 -0.87962 galactic Mon Second-epoch detections are separated by 7.8" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:49:24.48 -00:56:19.2 (user input) | T | P | (position from user input) J-Ks=0.337+/-0.043 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461049.6091,13.06,0.05,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
target 20260109.1091 13.06CV 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 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:49:24.48 -00:56:19.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 09.1091 2461049.6091 13.14 06:31:35.76 -00:06:55.5
210.76849 -4.46640 galactic Mon Second-epoch detections are separated by 5.7" and 7.6 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 3120062435083960064 | 06:31:34.11 -00:07:14.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G 1949AnHar.112....1C HD 291739
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3120062435083960064,2461049.6091,13.14,0.05,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 3120062435083960064 20260109.1091 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:31:35.76 -00:06:55.5 ;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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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 3105302831513609216,2461049.6091,12.99,0.05,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 3105302831513609216 20260109.1091 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:43:36.79 -04:25:05.4 ;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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 09.1091 2461049.6091 13.04 06:37:40.83 -03:12:19.5
214.22244 -4.51990 galactic Mon Second-epoch detections are separated by 7.9" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:37:40.83 -03:12:19.5 (user input) | T | P | (position from user input) J-Ks=0.539+/-0.035 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461049.6091,13.04,0.05,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 20260109.1091 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:37:40.83 -03:12:19.5 ;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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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
GDS_J0650329-014523,2461049.6091,13.14,0.05,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
GDS_J0650329-014523 20260109.1091 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:50:32.82 -01:45:41.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 09.1091 2461049.6091 13.10 06:51:34.19 -01:39:24.4
214.42154 -0.72604 galactic Mon Second-epoch detections are separated by 4.7" and 7.6 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 J102.9043-01.6544 | 06:51:34.96 -01:38:50.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G0: 1956ApJS....2..271M LF 9 -02 199
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J102.9043-01.6544,2461049.6091,13.10,0.05,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
ATO J102.9043-01.6544 20260109.1091 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:51:34.19 -01:39:24.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 09.1091 2461049.6091 13.24 06:27:42.65 +01:40:00.8
208.73304 -4.51225 galactic Mon Second-epoch detections are separated by 7.7" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3123842040664991744 | 06:27:43.01 +01:40:23.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (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 3123842040664991744,2461049.6091,13.24,0.05,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
Gaia DR3 3123842040664991744 20260109.1091 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 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:27:42.65 +01:40:00.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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 3100691995143597056,2461049.6091,13.25,0.05,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 3100691995143597056 20260109.1091 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:43:44.13 -05:07:48.4 ;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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 09.1091 2461049.6091 13.18 06:35:49.87 -02:34:43.5
213.45198 -4.64682 galactic Mon Second-epoch detections are separated by 4.2" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:35:49.87 -02:34:43.5 (user input) | T | P | (position from user input) J-Ks=0.309+/-0.038 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461049.6091,13.18,0.05,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
target 20260109.1091 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:35:49.87 -02:34:43.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 09.1091 2461049.6091 13.32 06:56:49.45 -05:48:28.7
218.71456 -1.45180 galactic Mon Second-epoch detections are separated by 6.5" and 7.8 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 3101159626880841728 | 06:56:51.32 -05:48:25.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.393+/-0.040 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101159626880841728,2461049.6091,13.32,0.05,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 3101159626880841728 20260109.1091 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:56:49.45 -05:48:28.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 09.1091 2461049.6091 13.43 06:52:50.88 -02:20:53.6
215.18261 -0.75700 galactic Mon Second-epoch detections are separated by 7.9" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3106021564222428032 | 06:52:52.95 -02:21:14.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.438+/-0.043 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106021564222428032,2461049.6091,13.43,0.05,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
Gaia DR3 3106021564222428032 20260109.1091 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 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:52:50.88 -02:20:53.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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 3112525317237727616,2461049.6091,13.40,0.05,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
Gaia DR3 3112525317237727616 20260109.1091 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 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:56:43.91 -00:22:16.1 ;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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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,2461049.6091,13.54,0.05,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 20260109.1091 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 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:36:15.41 -04:30:52.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 09.1091 2461049.6091 13.48 06:43:09.64 -02:13:08.5
213.96501 -2.85265 galactic Mon Second-epoch detections are separated by 8.2" and 7.2 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 3106566475310188032 | 06:43:11.26 -02:12:38.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1949AnHar.112....1C HD 292258 J-Ks=0.295+/-0.040 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106566475310188032,2461049.6091,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106566475310188032 20260109.1091 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:43:09.64 -02:13:08.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Mon-02-Q1b1x1_2025-12-23_01-31-28_20_00sec_-15_00C_LIGHT_0382_fits__*pix.png resample_wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_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_2026-01-08_20-37-17_20_00sec_-14_90C_LIGHT_0050_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_2026-01-08_20-36-35_20_00sec_-14_90C_LIGHT_0049_fits__*pix.png animation_v2.gif
Processing complete!
Total number of candidates identified: 31
Processing log:
## 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 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//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 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Last image: 2461049.60935078 09.01.2026 02:37:17.907 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
Estimated ref. image limiting mag.: -10.72
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: 1
User-specified moving object: none
Computation time: 59 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): 34008
Objects passed selection criteria: 33953
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 30517.5
Average stars matched: 29839.2 (97.7775 %)
Memory usage VmPeak: 134116 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Thu Jan 8 15:05:04 -00 2026
VaST build number 1.0rc88-133-gdb8b9ae6
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-01-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jan 9 04:55:24 -00 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 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//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 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Last image: 2461049.60935078 09.01.2026 02:37:17.907 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 367
Estimated ref. image limiting mag.: -8.14
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: 1
User-specified moving object: none
Computation time: 859 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 2.1 # or , in mag.arcsec-2
ANALYSIS_THRESH 2.1 # or , in mag.arcsec-2
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): 239345
Objects passed selection criteria: 238854
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 219743
Average stars matched: 213082 (96.9685 %)
Memory usage VmPeak: 2366384 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Thu Jan 8 15:05:04 -00 2026
VaST build number 1.0rc88-133-gdb8b9ae6
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-01-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jan 9 05:11:07 -00 2026
Host name: tau
############################################################
Filtering log:
######## Processing parameters ########
AAVSO_COMMENT_STRING= NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
ASTCHECK_ASTEROID_SEARCH_RADIUS_ARCSEC=
BAD_REGION_FILE= /var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst
CAMERA_SETTINGS= TTUQ1b1x1
CHECK_POINTING_ACCURACY= yes
DARK_FRAMES_DIR= /var/www/nmw_calibration/TTUQ1b1x1/darks
EXCLUSION_LIST= ../exclusion_list_TTUQ1.txt
FILTER_BAD_IMG__MAX_APERTURE_STAR_SIZE_PIX= 12.5
FILTER_BAD_IMG__MAX_ELONGATION_AminusB_PIX= 0.55
FILTER_BAD_IMG__MIN_APERTURE_STAR_SIZE_PIX= 2.0
FILTER_BRIGHT_MAG_CUTOFF_TRANSIENT_SEARCH= -5
FILTER_FAINT_MAG_CUTOFF_TRANSIENT_SEARCH= 14.5
FLAT_FIELD_FILE= /var/www/nmw_calibration/TTUQ1b1x1/flats/mff_TTUQ1b1x1_2025-12-22.fit
FRAME_EDGE_OFFSET_PIX= 50
GAIA_BAND_FOR_CATALOGED_SOURCE_CHECK=
MAX_NEW_TO_REF_MEAN_IMG_VALUE_RATIO= 100
MAX_NEW_IMG_MEAN_VALUE= 25000
MAX_SD_RATIO_OF_SECOND_EPOCH_IMGS= 0.18
MAX_SD_RATIO_OF_SECOND_EPOCH_IMGS_SOFT_LIMIT= 0.12
MPC_CODE= 500
NMW_CALIBRATION= /var/www/nmw_calibration
NUMBER_OF_DETECTED_TRANSIENTS_BEFORE_FILTERING_HARD_LIMIT= 3000
NUMBER_OF_DETECTED_TRANSIENTS_BEFORE_FILTERING_SOFT_LIMIT= 2000
OMP_NUM_THREADS=
ONLINE_MPCHECKER_BUTTON_ASTEROID_SEARCH_RADIUS_ARCMIN=
PHOTOMETRIC_CALIBRATION=
REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES= no
SEXTRACTOR_CONFIG_BRIGHTSTARPASS= default.sex.telephoto_lens_onlybrightstars_v1
SEXTRACTOR_CONFIG_FILES= default.sex.telephoto_lens_onlybrightstars_v1 default.sex.telephoto_lens_vSTL
STARMATCH_RADIUS_PIX= 3.5
SYSREM_ITERATIONS= 1
TELESCOP=
TELESCOP_NAME_KNOWN_TO_VaST_FOR_FOV_DETERMINATION=
UCAC5_PLATESOLVE_ITERATIONS= 2
#######################################
HOSTNAME= tau
USER=
HOME=
#######################################
Reference image directory is set to /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved/
VIZIER_SITE=vizier.cds.unistra.fr
INFO: MAKE_PNG_PLOTS is set to yes
FITS_FILE_EXT=fits
CALIBRATION_STATUS_PREFIX=
Fields in the data directory:
Mon-02-Q1b1x1
#######################################
########### Starting Mon-02-Q1b1x1 ###########
Processing Mon-02-Q1b1x1
server tau has sufficient free disk space available: 586675 MB at /mnt/usb2/NMW-TexasTech/workdir
server tau has sufficient free disk space available: 586675 MB at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
REFERENCE_EPOCH__SECOND_IMAGE= /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.png' -> 'transient_report/Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits_preview.png'
Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits
renamed 'Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.png' -> 'transient_report/Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits_preview.png'
Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
Read-check the input FITS images... read-check OK
Blank image check the input FITS images... blank-image-check OK
Read date check the input FITS images... read-date-check OK
Mean value check the input FITS images... OK, at least two new images have mean values below the threshold.
----------------------------------------------
INFO: REFERENCE_EPOCH__FIRST_IMAGE_MEAN_VALUE= 792.3781
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 934.5946
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 1840.5133
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 915.5422
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 1836.4142
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 916.5566
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 2.32277
INFO: SECOND_EPOCH__SD_ratio= 0.001
----------------------------------------------
Calibration settings: DARK_FRAMES_DIR=/var/www/nmw_calibration/TTUQ1b1x1/darks FLAT_FIELD_FILE=/var/www/nmw_calibration/TTUQ1b1x1/flats/mff_TTUQ1b1x1_2025-12-22.fit
EXPTIME = 20.0 / [s] Exposure duration
SET-TEMP= -15.0 / [degC] CCD temperature setpoint
CCD-TEMP= -14.9 / [degC] CCD temperature
Exploring image header: /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits
CCD-TEMP= -14.900000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits
SET-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits
Header: 61 keys total, 10 keys left
Record 0: "" status=0
Record 1: "SIMPLE = T / C# FITS" status=0
Record 2: "BITPIX = 16" status=0
Record 3: "NAXIS = 2 / Dimensionality" status=0
Record 4: "NAXIS1 = 9576" status=0
Record 5: "NAXIS2 = 6388" status=0
Record 6: "BZERO = 32768" status=0
Record 7: "EXTEND = T / Extensions are permitted" status=0
Record 8: "IMAGETYP= 'LIGHT' / Type of exposure" status=0
Record 9: "EXPOSURE= 20.0 / [s] Exposure duration" status=0
Record 10: "EXPTIME = 20.0 / [s] Exposure duration" status=0
Record 11: "DATE-LOC= '2026-01-08T20:36:35.9794642' / Time of observation (local)" status=0
Record 12: "DATE-OBS= '2026-01-09T02:36:35.9794642' / Time of observation (UTC)" status=0
Record 13: "MJD-OBS = 61049.1087497571 / Modified Julian Date of observation" status=0
Record 14: "DATE-AVG= '2026-01-09T02:36:45.8797390' / Averaged midpoint time (UTC)" status=0
Record 15: "MJD-AVG = 61049.1088643405 / Modified Julian Date of averaged midpoint" status=0
Record 16: "XBINNING= 1 / X axis binning factor" status=0
Record 17: "YBINNING= 1 / Y axis binning factor" status=0
Record 18: "GAIN = 30 / Sensor gain" status=0
Record 19: "OFFSET = 30 / Sensor gain offset" status=0
Record 20: "XPIXSZ = 3.76 / [um] Pixel X axis size" status=0
Record 21: "YPIXSZ = 3.76 / [um] Pixel Y axis size" status=0
Record 22: "INSTRUME= 'QHY600M' / Imaging instrument name" status=0
Record 23: "CAMERAID= 'QHY600M-33d3d743814b8b447' / Imaging instrument identifier" status=0
Record 24: "SET-TEMP= -15.0 / [degC] CCD temperature setpoint" status=0
Record 25: "CCD-TEMP= -14.9 / [degC] CCD temperature" status=0
Record 26: "READOUTM= '2CMS-0' / Sensor readout mode" status=0
Record 27: "USBLIMIT= 50 / Camera-specific USB setting" status=0
Record 28: "TELESCOP= 'QHY600M-TTU1' / Name of telescope" status=0
Record 29: "FOCALLEN= 135.0 / [mm] Focal length" status=0
Record 30: "FOCRATIO= 2.2 / Focal ratio" status=0
Record 31: "RA = 102.855959817735 / [deg] RA of telescope" status=0
Record 32: "DEC = -1.99981709059101 / [deg] Declination of telescope" status=0
Record 33: "CENTALT = 25.4447222222222 / [deg] Altitude of telescope" status=0
Record 34: "CENTAZ = 111.413055555556 / [deg] Azimuth of telescope" status=0
Record 35: "AIRMASS = 2.31760302516814 / Airmass at frame center (Gueymard 1993)" status=0
Record 36: "PIERSIDE= 'West' / Telescope pointing state" status=0
Record 37: "SITEELEV= 1013.0 / [m] Observation site elevation" status=0
Record 38: "SITELAT = 33.748239 / [deg] Observation site latitude" status=0
Record 39: "SITELONG= -101.958391 / [deg] Observation site longitude" status=0
Record 40: "OBSERVER= 'Sokolovsky' / Observer name" status=0
Record 41: "OBSERVAT= 'TTU Skyview' / Observatory name" status=0
Record 42: "SITENAME= '' / Observatory site name" status=0
Record 43: "FWHEEL = 'Simulator' / Filter Wheel name" status=0
Record 44: "FILTER = 'CV' / Active filter name" status=0
Record 45: "OBJECT = 'Mon-02' / Name of the object of interest" status=0
Record 46: "OBJCTRA = '06 51 26' / [H M S] RA of imaged object" status=0
Record 47: "OBJCTDEC= '-02 00 00' / [D M S] Declination of imaged object" status=0
Record 48: "OBJCTROT= 0.0 / [deg] planned rotation of imaged object" status=0
Record 49: "ROWORDER= 'TOP-DOWN' / FITS Image Orientation" status=0
Record 50: "EQUINOX = 2000.0 / Equinox of celestial coordinate system" status=0
Record 51: "SWCREATE= 'N.I.N.A. 3.2.0.9001 (x64)' / Software that created this file" status=0
Record 52: "QHY_EXP = 20.000096 / [s] Actual exposure time" status=0
Record 53: "QHY_PP = 13888.0 / [ps] pixelPeriod" status=0
Record 54: "QHY_LP = 85000.0 / [ns] linePeriod" status=0
Record 55: "GPS_LP = 85000.0 / [ns] linePeriod" status=0
Record 56: "QHY_FP = 20000160.0 / [us] framePeriod" status=0
Record 57: "QHY_CPL = 6120.0 / clocksPerLine" status=0
Record 58: "QHY_LPF = 235295.0 / linesPerFrame" status=0
Record 59: "QHY_AET = 20000096.0 / [us] actualExposureTime" status=0
Record 60: "QHY_LEM = T / isLongExposureMode" status=0
Record 61: "QHY_OFF0= 3767.777 / [us] RollingShutterEndOffset row 0" status=0
Allocating memory for image, dark and result arrays...
Reading image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits 9576 6388 16 bitpix
SET-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits
SET-TEMP= -15.000000 for /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2026-01-08.fit
CCD-TEMP= -14.900000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits
CCD-TEMP= -15.000000 for /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2026-01-08.fit
Reading dark frame /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2026-01-08.fit 9576 6388 16 bitpix
Dark frame is subtracted, output is written to /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/d_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits :)
Spent 0.431514 seconds
renamed 'mdark_TTUQ1b1x1_-15C_20s_2026-01-08.png' -> 'transient_report/dark.png'
MegaDivider v7
Reading image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/d_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits 9576 6388 16 bitpix
Reading flat /var/www/nmw_calibration/TTUQ1b1x1/flats/mff_TTUQ1b1x1_2025-12-22.fit 9576 6388 16 bitpix
Avarage count on flat field image: 38918.354428
Minimal real count (from overscan): 5
Output is written to /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits :)
No overscan detected - all values seem high! (left_median=27736.5, right_median=26453.5)
renamed 'mff_TTUQ1b1x1_2025-12-22.png' -> 'transient_report/flat.png'
Using calibrated image CALIBRATED_SECOND_EPOCH__FIRST_IMAGE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits
EXPTIME = 20.0 / [s] Exposure duration
SET-TEMP= -15.0 / [degC] CCD temperature setpoint
CCD-TEMP= -14.9 / [degC] CCD temperature
Exploring image header: /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
CCD-TEMP= -14.900000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
SET-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
Header: 61 keys total, 10 keys left
Record 0: "" status=0
Record 1: "SIMPLE = T / C# FITS" status=0
Record 2: "BITPIX = 16" status=0
Record 3: "NAXIS = 2 / Dimensionality" status=0
Record 4: "NAXIS1 = 9576" status=0
Record 5: "NAXIS2 = 6388" status=0
Record 6: "BZERO = 32768" status=0
Record 7: "EXTEND = T / Extensions are permitted" status=0
Record 8: "IMAGETYP= 'LIGHT' / Type of exposure" status=0
Record 9: "EXPOSURE= 20.0 / [s] Exposure duration" status=0
Record 10: "EXPTIME = 20.0 / [s] Exposure duration" status=0
Record 11: "DATE-LOC= '2026-01-08T20:37:17.9077791' / Time of observation (local)" status=0
Record 12: "DATE-OBS= '2026-01-09T02:37:17.9077791' / Time of observation (UTC)" status=0
Record 13: "MJD-OBS = 61049.1092350348 / Modified Julian Date of observation" status=0
Record 14: "DATE-AVG= '2026-01-09T02:37:27.8115833' / Averaged midpoint time (UTC)" status=0
Record 15: "MJD-AVG = 61049.1093496643 / Modified Julian Date of averaged midpoint" status=0
Record 16: "XBINNING= 1 / X axis binning factor" status=0
Record 17: "YBINNING= 1 / Y axis binning factor" status=0
Record 18: "GAIN = 30 / Sensor gain" status=0
Record 19: "OFFSET = 30 / Sensor gain offset" status=0
Record 20: "XPIXSZ = 3.76 / [um] Pixel X axis size" status=0
Record 21: "YPIXSZ = 3.76 / [um] Pixel Y axis size" status=0
Record 22: "INSTRUME= 'QHY600M' / Imaging instrument name" status=0
Record 23: "CAMERAID= 'QHY600M-33d3d743814b8b447' / Imaging instrument identifier" status=0
Record 24: "SET-TEMP= -15.0 / [degC] CCD temperature setpoint" status=0
Record 25: "CCD-TEMP= -14.9 / [degC] CCD temperature" status=0
Record 26: "READOUTM= '2CMS-0' / Sensor readout mode" status=0
Record 27: "USBLIMIT= 50 / Camera-specific USB setting" status=0
Record 28: "TELESCOP= 'QHY600M-TTU1' / Name of telescope" status=0
Record 29: "FOCALLEN= 135.0 / [mm] Focal length" status=0
Record 30: "FOCRATIO= 2.2 / Focal ratio" status=0
Record 31: "RA = 102.855959814398 / [deg] RA of telescope" status=0
Record 32: "DEC = -1.99981707019217 / [deg] Declination of telescope" status=0
Record 33: "CENTALT = 25.5802777777778 / [deg] Altitude of telescope" status=0
Record 34: "CENTAZ = 111.536111111111 / [deg] Azimuth of telescope" status=0
Record 35: "AIRMASS = 2.3062650114001 / Airmass at frame center (Gueymard 1993)" status=0
Record 36: "PIERSIDE= 'West' / Telescope pointing state" status=0
Record 37: "SITEELEV= 1013.0 / [m] Observation site elevation" status=0
Record 38: "SITELAT = 33.748239 / [deg] Observation site latitude" status=0
Record 39: "SITELONG= -101.958391 / [deg] Observation site longitude" status=0
Record 40: "OBSERVER= 'Sokolovsky' / Observer name" status=0
Record 41: "OBSERVAT= 'TTU Skyview' / Observatory name" status=0
Record 42: "SITENAME= '' / Observatory site name" status=0
Record 43: "FWHEEL = 'Simulator' / Filter Wheel name" status=0
Record 44: "FILTER = 'CV' / Active filter name" status=0
Record 45: "OBJECT = 'Mon-02' / Name of the object of interest" status=0
Record 46: "OBJCTRA = '06 51 26' / [H M S] RA of imaged object" status=0
Record 47: "OBJCTDEC= '-02 00 00' / [D M S] Declination of imaged object" status=0
Record 48: "OBJCTROT= 0.0 / [deg] planned rotation of imaged object" status=0
Record 49: "ROWORDER= 'TOP-DOWN' / FITS Image Orientation" status=0
Record 50: "EQUINOX = 2000.0 / Equinox of celestial coordinate system" status=0
Record 51: "SWCREATE= 'N.I.N.A. 3.2.0.9001 (x64)' / Software that created this file" status=0
Record 52: "QHY_EXP = 20.000096 / [s] Actual exposure time" status=0
Record 53: "QHY_PP = 13888.0 / [ps] pixelPeriod" status=0
Record 54: "QHY_LP = 85000.0 / [ns] linePeriod" status=0
Record 55: "GPS_LP = 85000.0 / [ns] linePeriod" status=0
Record 56: "QHY_FP = 20000160.0 / [us] framePeriod" status=0
Record 57: "QHY_CPL = 6120.0 / clocksPerLine" status=0
Record 58: "QHY_LPF = 235295.0 / linesPerFrame" status=0
Record 59: "QHY_AET = 20000096.0 / [us] actualExposureTime" status=0
Record 60: "QHY_LEM = T / isLongExposureMode" status=0
Record 61: "QHY_OFF0= 3767.777 / [us] RollingShutterEndOffset row 0" status=0
Allocating memory for image, dark and result arrays...
Reading image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits 9576 6388 16 bitpix
SET-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
SET-TEMP= -15.000000 for /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2026-01-08.fit
CCD-TEMP= -14.900000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
CCD-TEMP= -15.000000 for /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2026-01-08.fit
Reading dark frame /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2026-01-08.fit 9576 6388 16 bitpix
Dark frame is subtracted, output is written to /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/d_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits :)
Spent 0.435313 seconds
renamed 'mdark_TTUQ1b1x1_-15C_20s_2026-01-08.png' -> 'transient_report/dark.png'
MegaDivider v7
Reading image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/d_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits 9576 6388 16 bitpix
Reading flat /var/www/nmw_calibration/TTUQ1b1x1/flats/mff_TTUQ1b1x1_2025-12-22.fit 9576 6388 16 bitpix
Avarage count on flat field image: 38918.354428
Minimal real count (from overscan): 5
Output is written to /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits :)
No overscan detected - all values seem high! (left_median=27736.5, right_median=26453.5)
renamed 'mff_TTUQ1b1x1_2025-12-22.png' -> 'transient_report/flat.png'
Using calibrated image CALIBRATED_SECOND_EPOCH__SECOND_IMAGE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
Dark frame used to calibrate the second-epoch images:
Flat field used to calibrate the second-epoch images:
after the calibration attempt:
SECOND_EPOCH__FIRST_IMAGE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits
SECOND_EPOCH__SECOND_IMAGE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
Previews of the CALIBRATED second-epoch images:
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 --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 1 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.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: 2461049.60886550
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_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits'
wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.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 06:51:39.379 -01:58:29.12
Angular distance between the image centers 0.03 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 06:51:43.546 -01:58:28.73
Angular distance between the image centers 0.03 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits &> /tmp/tmp.oXJtkNS15R
Parallel run for /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//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 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits &> /tmp/tmp.QvTXIFxQ0W
Parallel run for /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//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 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits &> /tmp/tmp.W03Ipcus7t
Parallel run for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits &> /tmp/tmp.BXrbLN8ZtM
Parallel run for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.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.: -10.72
Updating vast_summary.log: Estimated ref. image limiting mag.: 12.17
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 12.17
____ End of magnitude calibration ____
Filter-out faint candidates...
Filter-out suspiciously bright candidates...
Filter-out candidates with large difference between measured mags in one epoch...
Filter-out small-amplitude flares...
Preparing the exclusion lists for this field
Done with filtering
Found 7 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix 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_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits
2.2 pix fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
All-image limiting magnitude estimate: 11.7 with default.sex.telephoto_lens_onlybrightstars_v1
(80th percentile of magnitude distribution of stars detected on all four images)
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.oXJtkNS15R (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate...
/mnt/usb2/NMW-TexasTech/workdir/vast_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits 568.0
Entering WCS image calibration mode.
DEBUG: ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
DEBUG: FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
DEBUG: FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
verification OK: /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//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 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//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...
'/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//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'
DEBUG: FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
DEBUG: 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 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//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
The fraction of blended stars is high!
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!
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!
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 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//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.QvTXIFxQ0W (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate...
/mnt/usb2/NMW-TexasTech/workdir/vast_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits 568.0
Entering WCS image calibration mode.
DEBUG: ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
DEBUG: FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
DEBUG: FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
verification OK: /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//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 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//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...
'/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//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'
DEBUG: FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
DEBUG: 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 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//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
The fraction of blended stars is high!
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!
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.
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.W03Ipcus7t (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...
/mnt/usb2/NMW-TexasTech/workdir/vast_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits 605.0
Entering WCS image calibration mode.
DEBUG: ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits
DEBUG: FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits
DEBUG: FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits
verification OK: /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
DEBUG: FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits
DEBUG: WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.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_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits.cat
The fraction of blended stars is high!
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2427, passed=24900
Got 24900 stars (including 22445 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits.cat
util/solve_plate_with_UCAC5 got 24900 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 929.1'
Seting catalog search parameters based on the expected field of view 929.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012904 (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 0.010323 (37.2 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 573 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: 3.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 3.40"
ITERATION 02 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 606 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 3.31"
Estimated accuracy of the plate solution: 2.31"
Excluding outliers - 537 stars left (next iteration limit 531)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits -region wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.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.BXrbLN8ZtM (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...
/mnt/usb2/NMW-TexasTech/workdir/vast_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits 605.0
Entering WCS image calibration mode.
DEBUG: ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
DEBUG: FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
DEBUG: FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
verification OK: /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
DEBUG: FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
DEBUG: WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.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_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits.cat
The fraction of blended stars is high!
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2382, passed=24870
Got 24870 stars (including 22467 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits.cat
util/solve_plate_with_UCAC5 got 24870 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.1'
Seting catalog search parameters based on the expected field of view 931.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012932 (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 0.010346 (37.2 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 578 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: 4.06"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 5.64"
ITERATION 02 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 608 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 5.52"
Estimated accuracy of the plate solution: 2.89"
Excluding outliers - 533 stars left (next iteration limit 547)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits -region wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.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_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits
'wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits.fz' -> '/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits.fz'
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
'wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits.fz' -> '/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits.fz'
Preparing the HTML report for the field Mon-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out52643.dat to exclusion_list_gaiadr2.txt
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52569_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 52569_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 52592_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 52592_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (99.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52643_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 52643_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (91.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52657_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 52657_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (55.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52658_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 52658_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52665_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 52665_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (124.8") between the two second-epoch detections
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 ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 1 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.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_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Creating symlink local_wcs_cache/exclusion_list_bsc.txt
Creating symlink local_wcs_cache/exclusion_list_tycho2.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_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits exists and is non-empty
wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.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 06:51:39.379 -01:58:29.12
Angular distance between the image centers 0.03 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 06:51:43.546 -01:58:28.73
Angular distance between the image centers 0.03 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits &> /tmp/tmp.dlS9BUhaCL
Parallel run for /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//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 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits &> /tmp/tmp.y1cBjeLccF
Parallel run for /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//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 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits &> /tmp/tmp.xcjmwQdm2M
Parallel run for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits &> /tmp/tmp.NVwYBk8cPX
Parallel run for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.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.: -8.14
Updating vast_summary.log: Estimated ref. image limiting mag.: 13.74
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 13.74
____ End of magnitude calibration ____
Filter-out faint candidates...
Filter-out suspiciously bright candidates...
Filter-out candidates with large difference between measured mags in one epoch...
Filter-out small-amplitude flares...
Preparing the exclusion lists for this field
Done with filtering
Found 349 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
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
2.1 pix fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits
2.1 pix fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
All-image limiting magnitude estimate: 13.2 with default.sex.telephoto_lens_vSTL
(80th percentile of magnitude distribution of stars detected on all four images)
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.dlS9BUhaCL (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate...
/mnt/usb2/NMW-TexasTech/workdir/vast_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits 568.0
Entering WCS image calibration mode.
DEBUG: ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
DEBUG: FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
DEBUG: FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
verification OK: /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//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 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//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...
'/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//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'
DEBUG: FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
DEBUG: 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 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//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
The fraction of blended stars is high!
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!
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!
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 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//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.y1cBjeLccF (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate...
/mnt/usb2/NMW-TexasTech/workdir/vast_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits 568.0
Entering WCS image calibration mode.
DEBUG: ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
DEBUG: FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
DEBUG: FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
verification OK: /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//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 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//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...
'/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//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'
DEBUG: FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Mon-02-Q1b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
DEBUG: 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 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//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
The fraction of blended stars is high!
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!
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.
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.xcjmwQdm2M (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...
/mnt/usb2/NMW-TexasTech/workdir/vast_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits 605.0
Entering WCS image calibration mode.
DEBUG: ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits
DEBUG: FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits
DEBUG: FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits
verification OK: /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
DEBUG: FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits
DEBUG: WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.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_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits.cat
The fraction of blended stars is high!
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=23122, passed=184807
Got 184807 stars (including 161431 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits.cat
util/solve_plate_with_UCAC5 got 184807 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 929.1'
Seting catalog search parameters based on the expected field of view 929.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012904 (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 0.010323 (37.2 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 561 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: 2.65"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.81"
ITERATION 02 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 589 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 2.81"
Estimated accuracy of the plate solution: 1.75"
Excluding outliers - 525 stars left (next iteration limit 531)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits -region wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.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.NVwYBk8cPX (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...
/mnt/usb2/NMW-TexasTech/workdir/vast_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits 605.0
Entering WCS image calibration mode.
DEBUG: ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
DEBUG: FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
DEBUG: FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
verification OK: /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
DEBUG: FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
DEBUG: WCS_IMAGE_NAME=wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
Checking if the catalog wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits.cat corresponding to the image wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.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_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
WCS catalog name: wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits.cat
The fraction of blended stars is high!
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=34, blended=23402, passed=186032
Got 186032 stars (including 162356 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits.cat
util/solve_plate_with_UCAC5 got 186032 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.1'
Seting catalog search parameters based on the expected field of view 931.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012932 (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 0.010346 (37.2 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 584 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: 4.02"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 4.54"
ITERATION 02 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 610 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 4.53"
Estimated accuracy of the plate solution: 2.69"
Excluding outliers - 555 stars left (next iteration limit 562)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits -region wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.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_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits
The destination file is already there - not rewriting /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.fits.fz
Saving fully-calibrated image wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits
The destination file is already there - not rewriting /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Mon-02-Q1b1x1_222524_TTUQ1b1x1_17903_7c1Tn6pC/wcs_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.fits.fz
Preparing the HTML report for the field Mon-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out288220.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288264.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288285.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288297.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288305.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288323.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288324.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288348.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288354.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288356.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288393.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288406.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288417.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288418.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288438.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288443.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288458.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288476.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288676.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288684.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288698.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288746.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288759.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288786.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288820.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288873.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288895.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288935.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out288978.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289018.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289034.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289039.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289171.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289210.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289228.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289231.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289232.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289271.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289310.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289359.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289374.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289393.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289429.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289462.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289475.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289481.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289516.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289540.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289553.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289620.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289683.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289690.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289779.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289788.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289841.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289871.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out289962.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290001.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out290043.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out288310.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out289473.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out288208.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288243.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288320.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288329.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288421.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288424.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288426.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288453.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288474.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288475.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288478.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288627.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288855.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289061.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289095.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289454.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289474.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289519.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289527.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289550.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289559.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289582.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289597.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289631.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289724.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289768.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289781.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289829.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289877.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289904.dat to exclusion_list_local.txt
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Considering the candidate 288181_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288181_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 288191_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288191_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 288194_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288194_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 288205_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288205_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 288208_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Preparing report for the candidate 288208_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Successfully moved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.png to transient_report/288208_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_reference.png
Successfully moved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.png to transient_report/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits_preview.png
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.png to transient_report/288208_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery1.png
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.png to transient_report/288208_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery2.png
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Considering the candidate 288214_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288214_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 288220_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288220_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 288239_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288239_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 288241_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288241_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 288243_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Preparing report for the candidate 288243_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Successfully moved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.png to transient_report/288243_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_reference.png
The output file transient_report/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits_preview.png already exist
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.png to transient_report/288243_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery1.png
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.png to transient_report/288243_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery2.png
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Considering the candidate 288245_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288245_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (35.9") between the two second-epoch detections
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Considering the candidate 288262_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288262_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288264_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288264_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 288272_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288272_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 288273_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288273_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 288280_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288280_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 288285_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288285_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
**** FOUND 06:39:52.99 -03:15:01.7 in Gaia DR2 blend (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.21, BLEND_MAG_FAINT_SEARCH_LIMIT=, VIZIER_COMMAND=#lib/vizquery -site=vizier.cds.unistra.fr -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..14.19 -c=06:39:52.99 -03:15:01.7 -c.rs=14.50 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)
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Considering the candidate 288297_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288297_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 288305_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288305_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 288310_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288310_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
**** FOUND 06:47:49.93 -07:08:38.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)
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Considering the candidate 288314_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288314_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 288315_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288315_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (50.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288320_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Preparing report for the candidate 288320_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Successfully moved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.png to transient_report/288320_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_reference.png
The output file transient_report/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits_preview.png already exist
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.png to transient_report/288320_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery1.png
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.png to transient_report/288320_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery2.png
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Considering the candidate 288323_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288323_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 288328_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288328_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288329_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Preparing report for the candidate 288329_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Successfully moved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.png to transient_report/288329_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_reference.png
The output file transient_report/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits_preview.png already exist
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.png to transient_report/288329_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery1.png
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.png to transient_report/288329_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288330_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288330_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (69.8") between the two second-epoch detections
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Considering the candidate 288332_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288332_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (137.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288334_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288334_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (35.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288335_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288335_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (25.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288336_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288336_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (55.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288340_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288340_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (48.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288341_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288341_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (55.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288348_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288348_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288354_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288354_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (124.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288360_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288360_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (159.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288361_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288361_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288363_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288363_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288376_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288376_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (73.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288377_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288377_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288378_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288378_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (29.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288388_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288388_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (55.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288389_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288389_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (50.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288390_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288390_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (108.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288391_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288391_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288393_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288393_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288400_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288400_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (140.9") between the two second-epoch detections
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Considering the candidate 288401_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288401_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (264.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288402_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288402_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (36.9") between the two second-epoch detections
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Considering the candidate 288406_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288406_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (123.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288417_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288417_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (47.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288421_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Preparing report for the candidate 288421_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Successfully moved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.png to transient_report/288421_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_reference.png
The output file transient_report/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits_preview.png already exist
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.png to transient_report/288421_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery1.png
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.png to transient_report/288421_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288422_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288422_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288423_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288423_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288424_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Preparing report for the candidate 288424_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Successfully moved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.png to transient_report/288424_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_reference.png
The output file transient_report/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits_preview.png already exist
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.png to transient_report/288424_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery1.png
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.png to transient_report/288424_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288426_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Preparing report for the candidate 288426_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Successfully moved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.png to transient_report/288426_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_reference.png
The output file transient_report/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits_preview.png already exist
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.png to transient_report/288426_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery1.png
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.png to transient_report/288426_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery2.png
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Considering the candidate 288436_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288436_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (217.1") between the two second-epoch detections
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Considering the candidate 288437_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288437_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (137.2") between the two second-epoch detections
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Considering the candidate 288438_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288438_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (134.2") between the two second-epoch detections
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Considering the candidate 288443_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288443_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (45.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288450_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288450_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (150.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288452_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288452_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
**** FOUND 06:54:08.18 -05:53:01.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 288453_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Preparing report for the candidate 288453_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Successfully moved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.png to transient_report/288453_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_reference.png
The output file transient_report/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits_preview.png already exist
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.png to transient_report/288453_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery1.png
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.png to transient_report/288453_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288454_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288454_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (416.9") between the two second-epoch detections
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Considering the candidate 288458_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288458_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 288471_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288471_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (257.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288472_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288472_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (55.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288473_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288473_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (91.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288474_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Preparing report for the candidate 288474_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Successfully moved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.png to transient_report/288474_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_reference.png
The output file transient_report/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits_preview.png already exist
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.png to transient_report/288474_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery1.png
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.png to transient_report/288474_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288475_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Preparing report for the candidate 288475_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Successfully moved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.png to transient_report/288475_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_reference.png
The output file transient_report/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits_preview.png already exist
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.png to transient_report/288475_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery1.png
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.png to transient_report/288475_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288476_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288476_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (64.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288478_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Preparing report for the candidate 288478_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Successfully moved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.png to transient_report/288478_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_reference.png
The output file transient_report/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits_preview.png already exist
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.png to transient_report/288478_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery1.png
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.png to transient_report/288478_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288552_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288552_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (134.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288627_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Preparing report for the candidate 288627_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Successfully moved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.png to transient_report/288627_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_reference.png
The output file transient_report/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits_preview.png already exist
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.png to transient_report/288627_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery1.png
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.png to transient_report/288627_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288633_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288633_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (141.2") between the two second-epoch detections
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Considering the candidate 288643_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288643_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (105.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288657_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288657_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (76.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288676_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288676_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
**** FOUND 06:52:25.34 -05:17:27.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288725_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288725_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (65.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288726_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288726_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (68.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288746_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288746_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (59.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288786_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288786_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288791_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288791_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (71.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288804_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288804_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (229.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288807_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288807_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
**** FOUND 06:27:08.90 +00:16:34.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288812_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288812_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 288820_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288820_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (63.3") between the two second-epoch detections
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Considering the candidate 288825_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288825_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (98.4") between the two second-epoch detections
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Considering the candidate 288837_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288837_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (575.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288840_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288840_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (126.7") between the two second-epoch detections
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Considering the candidate 288855_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Preparing report for the candidate 288855_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Successfully moved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.png to transient_report/288855_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_reference.png
The output file transient_report/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits_preview.png already exist
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.png to transient_report/288855_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery1.png
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.png to transient_report/288855_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery2.png
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Considering the candidate 288869_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288869_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (27.2") between the two second-epoch detections
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Considering the candidate 288870_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288870_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (52.1") between the two second-epoch detections
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Considering the candidate 288873_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288873_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (99.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288889_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288889_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (122.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288895_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288895_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (645.3") between the two second-epoch detections
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Considering the candidate 288907_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288907_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (101.3") between the two second-epoch detections
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Considering the candidate 288919_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288919_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (93.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288929_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288929_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (640.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288932_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288932_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (43.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288935_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288935_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (359.7") between the two second-epoch detections
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Considering the candidate 288940_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288940_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (120.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288941_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288941_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 288944_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288944_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (60.4") between the two second-epoch detections
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Considering the candidate 288947_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288947_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (168.7") between the two second-epoch detections
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Considering the candidate 288951_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288951_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 288958_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288958_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (230.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288962_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288962_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288963_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288963_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (188.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288972_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288972_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (39.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288978_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288978_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288989_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 288989_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289003_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289003_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (116.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289007_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289007_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (642.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289011_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289011_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (110.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289017_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289017_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (173.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289018_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289018_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289025_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289025_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289031_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289031_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (148.8") between the two second-epoch detections
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Considering the candidate 289033_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289033_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (231.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289034_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289034_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (116.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289046_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289046_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (40.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289047_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289047_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (24.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289048_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289048_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (178.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289052_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289052_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (386.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289058_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289058_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289061_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Preparing report for the candidate 289061_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Successfully moved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.png to transient_report/289061_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_reference.png
The output file transient_report/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits_preview.png already exist
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.png to transient_report/289061_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery1.png
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.png to transient_report/289061_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289062_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289062_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (45.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289063_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289063_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (68.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289064_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289064_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (88.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289069_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289069_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (140.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289076_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289076_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (97.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289077_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289077_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (98.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289079_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289079_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (53.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289082_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289082_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289094_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289094_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289095_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Preparing report for the candidate 289095_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Successfully moved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.png to transient_report/289095_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_reference.png
The output file transient_report/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits_preview.png already exist
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.png to transient_report/289095_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery1.png
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.png to transient_report/289095_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery2.png
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Considering the candidate 289096_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289096_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (141.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289101_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289101_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (64.7") between the two second-epoch detections
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Considering the candidate 289105_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289105_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (155.0") between the two second-epoch detections
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Considering the candidate 289109_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289109_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 289125_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289125_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (78.9") between the two second-epoch detections
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Considering the candidate 289133_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289133_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 289134_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289134_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 289141_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289141_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (66.1") between the two second-epoch detections
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Considering the candidate 289142_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289142_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (189.2") between the two second-epoch detections
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Considering the candidate 289145_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289145_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (114.7") between the two second-epoch detections
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Considering the candidate 289148_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289148_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (82.7") between the two second-epoch detections
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Considering the candidate 289149_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289149_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 289155_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289155_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (161.6") between the two second-epoch detections
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Considering the candidate 289161_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289161_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289162_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289162_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (146.5") between the two second-epoch detections
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Considering the candidate 289163_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289163_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 289170_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289170_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (84.7") between the two second-epoch detections
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Considering the candidate 289171_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289171_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (124.3") between the two second-epoch detections
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Considering the candidate 289180_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289180_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (88.9") between the two second-epoch detections
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Considering the candidate 289181_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289181_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (63.5") between the two second-epoch detections
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Considering the candidate 289194_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289194_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 289202_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289202_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (55.7") between the two second-epoch detections
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Considering the candidate 289206_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289206_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (399.5") between the two second-epoch detections
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Considering the candidate 289207_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289207_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 289210_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289210_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (81.7") between the two second-epoch detections
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Considering the candidate 289216_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289216_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 289224_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289224_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 289228_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289228_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (177.9") between the two second-epoch detections
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Considering the candidate 289238_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289238_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (48.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289241_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289241_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (160.0") between the two second-epoch detections
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Considering the candidate 289242_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289242_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (97.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289243_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289243_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (62.3") between the two second-epoch detections
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Considering the candidate 289247_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289247_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (116.0") between the two second-epoch detections
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Considering the candidate 289249_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289249_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (49.9") between the two second-epoch detections
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Considering the candidate 289255_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289255_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (103.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289258_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289258_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289260_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289260_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (52.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289264_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289264_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (550.7") between the two second-epoch detections
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Considering the candidate 289271_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289271_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (111.2") between the two second-epoch detections
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Considering the candidate 289277_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289277_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (87.0") between the two second-epoch detections
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Considering the candidate 289281_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289281_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (88.0") between the two second-epoch detections
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Considering the candidate 289284_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289284_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 289285_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289285_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (75.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289288_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289288_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 289289_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289289_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 289290_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289290_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (315.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289293_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289293_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (161.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289301_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289301_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (294.7") between the two second-epoch detections
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Considering the candidate 289310_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289310_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (50.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289316_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289316_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (41.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289324_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289324_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (55.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289327_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289327_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (175.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289329_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289329_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289337_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289337_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289338_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289338_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
**** FOUND 06:28:11.44 +01:54:27.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 289344_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289344_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (55.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289345_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289345_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (153.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289359_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289359_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289363_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289363_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (60.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289365_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289365_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (467.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289372_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289372_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289373_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289373_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (26.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289374_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289374_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (60.5") between the two second-epoch detections
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Considering the candidate 289385_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289385_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (37.8") between the two second-epoch detections
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Considering the candidate 289393_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289393_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (172.6") between the two second-epoch detections
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Considering the candidate 289396_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289396_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (126.8") between the two second-epoch detections
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Considering the candidate 289402_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289402_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (35.9") between the two second-epoch detections
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Considering the candidate 289410_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289410_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 289416_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289416_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 289418_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289418_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (86.5") between the two second-epoch detections
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Considering the candidate 289424_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289424_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (81.5") between the two second-epoch detections
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Considering the candidate 289429_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289429_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 289446_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289446_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 289453_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289453_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (60.1") between the two second-epoch detections
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Considering the candidate 289454_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Preparing report for the candidate 289454_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Successfully moved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.png to transient_report/289454_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_reference.png
The output file transient_report/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits_preview.png already exist
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.png to transient_report/289454_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery1.png
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.png to transient_report/289454_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery2.png
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Considering the candidate 289458_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289458_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (67.9") between the two second-epoch detections
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Considering the candidate 289462_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289462_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (68.5") between the two second-epoch detections
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Considering the candidate 289473_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289473_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
**** FOUND 06:44:24.75 -00:04:49.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)
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Considering the candidate 289474_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Preparing report for the candidate 289474_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Successfully moved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.png to transient_report/289474_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_reference.png
The output file transient_report/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits_preview.png already exist
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.png to transient_report/289474_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery1.png
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.png to transient_report/289474_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery2.png
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Considering the candidate 289475_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289475_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 289495_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289495_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 289505_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289505_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 289506_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289506_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (133.1") between the two second-epoch detections
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Considering the candidate 289510_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289510_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 289516_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289516_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
**** FOUND 06:40:25.70 -01:49:10.1 in Gaia DR2 single (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99, VIZIER_COMMAND=#lib/vizquery -site=vizier.cds.unistra.fr -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..13.99 -c=06:40:25.70 -01:49:10.1 -c.rs=14.50 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)VIZIER_GAIADR2_OUTPUT=# 2.050 3106835447643595264 100.10754055648 -01.81981189803 13.5127 12.5464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.050#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 289519_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Preparing report for the candidate 289519_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Successfully moved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.png to transient_report/289519_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_reference.png
The output file transient_report/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits_preview.png already exist
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.png to transient_report/289519_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery1.png
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.png to transient_report/289519_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery2.png
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Considering the candidate 289527_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Preparing report for the candidate 289527_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Successfully moved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.png to transient_report/289527_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_reference.png
The output file transient_report/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits_preview.png already exist
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.png to transient_report/289527_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery1.png
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.png to transient_report/289527_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery2.png
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Considering the candidate 289528_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289528_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 289530_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289530_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (314.1") between the two second-epoch detections
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Considering the candidate 289534_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289534_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (129.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289538_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Preparing report for the candidate 289538_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Successfully moved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.png to transient_report/289538_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_reference.png
The output file transient_report/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits_preview.png already exist
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.png to transient_report/289538_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery1.png
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.png to transient_report/289538_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery2.png
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Considering the candidate 289540_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289540_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (74.5") between the two second-epoch detections
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Considering the candidate 289549_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289549_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
**** FOUND 06:28:13.43 +01:52:59.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 289550_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Preparing report for the candidate 289550_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Successfully moved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.png to transient_report/289550_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_reference.png
The output file transient_report/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits_preview.png already exist
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.png to transient_report/289550_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery1.png
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.png to transient_report/289550_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery2.png
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Considering the candidate 289551_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289551_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 289553_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289553_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
**** FOUND 06:44:57.48 -02:51:43.7 in Gaia DR2 single (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09, VIZIER_COMMAND=#lib/vizquery -site=vizier.cds.unistra.fr -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..14.09 -c=06:44:57.48 -02:51:43.7 -c.rs=14.50 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)VIZIER_GAIADR2_OUTPUT=# 1.260 3105761838958624896 101.23984910248 -02.86210694641 14.0439 13.5422 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.260#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289559_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Preparing report for the candidate 289559_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Successfully moved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.png to transient_report/289559_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_reference.png
The output file transient_report/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits_preview.png already exist
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.png to transient_report/289559_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery1.png
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.png to transient_report/289559_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery2.png
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Considering the candidate 289561_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289561_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 289564_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289564_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (128.1") between the two second-epoch detections
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Considering the candidate 289578_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289578_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (59.3") between the two second-epoch detections
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Considering the candidate 289580_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289580_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 289582_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Preparing report for the candidate 289582_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Successfully moved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.png to transient_report/289582_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_reference.png
The output file transient_report/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits_preview.png already exist
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.png to transient_report/289582_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery1.png
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.png to transient_report/289582_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery2.png
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Considering the candidate 289585_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289585_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (99.9") between the two second-epoch detections
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Considering the candidate 289587_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289587_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 289590_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289590_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 289592_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289592_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (23.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289597_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Preparing report for the candidate 289597_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Successfully moved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.png to transient_report/289597_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_reference.png
The output file transient_report/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits_preview.png already exist
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.png to transient_report/289597_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery1.png
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.png to transient_report/289597_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289620_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289620_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (115.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289631_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Preparing report for the candidate 289631_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Successfully moved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.png to transient_report/289631_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_reference.png
The output file transient_report/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits_preview.png already exist
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.png to transient_report/289631_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery1.png
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.png to transient_report/289631_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery2.png
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Considering the candidate 289653_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289653_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (186.5") between the two second-epoch detections
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Considering the candidate 289655_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289655_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
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Considering the candidate 289663_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289663_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 289665_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289665_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289676_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289676_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 289683_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289683_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (134.8") between the two second-epoch detections
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Considering the candidate 289690_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289690_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 289693_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289693_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (61.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289718_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289718_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (66.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289722_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289722_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289724_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Preparing report for the candidate 289724_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Successfully moved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.png to transient_report/289724_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_reference.png
The output file transient_report/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits_preview.png already exist
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.png to transient_report/289724_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery1.png
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.png to transient_report/289724_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289727_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289727_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (93.2") between the two second-epoch detections
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Considering the candidate 289733_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289733_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289761_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289761_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (28.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289764_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289764_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (67.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289768_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Preparing report for the candidate 289768_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Successfully moved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.png to transient_report/289768_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_reference.png
The output file transient_report/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits_preview.png already exist
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.png to transient_report/289768_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery1.png
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.png to transient_report/289768_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289775_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289775_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 289779_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289779_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
**** FOUND 06:51:34.37 -02:33:18.9 in Gaia DR2 single (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33, VIZIER_COMMAND=#lib/vizquery -site=vizier.cds.unistra.fr -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..14.33 -c=06:51:34.37 -02:33:18.9 -c.rs=14.50 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)VIZIER_GAIADR2_OUTPUT=# 4.523 3106011535478207360 102.89197053929 -02.55502747934 14.0434 13.2003 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.523#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289781_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Preparing report for the candidate 289781_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Successfully moved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.png to transient_report/289781_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_reference.png
The output file transient_report/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits_preview.png already exist
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.png to transient_report/289781_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery1.png
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.png to transient_report/289781_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery2.png
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Considering the candidate 289788_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289788_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (71.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289792_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289792_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (65.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289829_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Preparing report for the candidate 289829_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Successfully moved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.png to transient_report/289829_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_reference.png
The output file transient_report/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits_preview.png already exist
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.png to transient_report/289829_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery1.png
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.png to transient_report/289829_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289841_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289841_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289871_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289871_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
**** FOUND 06:51:10.08 -02:47:58.5 in Gaia DR2 single (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49, VIZIER_COMMAND=#lib/vizquery -site=vizier.cds.unistra.fr -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..14.49 -c=06:51:10.08 -02:47:58.5 -c.rs=14.50 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)VIZIER_GAIADR2_OUTPUT=# 2.436 3105909590133909760 102.79168393796 -02.80018181706 14.4805 14.0038 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.436#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289877_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Preparing report for the candidate 289877_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Successfully moved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.png to transient_report/289877_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_reference.png
The output file transient_report/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits_preview.png already exist
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.png to transient_report/289877_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery1.png
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.png to transient_report/289877_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery2.png
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Considering the candidate 289895_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289895_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289896_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289896_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289904_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Preparing report for the candidate 289904_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
Successfully moved Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.png to transient_report/289904_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_reference.png
The output file transient_report/Mon-02-Q1b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits_preview.png already exist
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-36-35_20.00sec_-14.90C_LIGHT_0049.png to transient_report/289904_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery1.png
Successfully moved fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050.png to transient_report/289904_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050_discovery2.png
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Considering the candidate 289929_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289929_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 289930_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289930_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 289936_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289936_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (90.2") between the two second-epoch detections
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Considering the candidate 289937_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289937_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 289944_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289944_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 289955_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289955_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 289962_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289962_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (105.5") between the two second-epoch detections
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Considering the candidate 289971_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289971_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (70.9") between the two second-epoch detections
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Considering the candidate 289980_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289980_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 289982_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 289982_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 290000_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 290000_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (55.2") between the two second-epoch detections
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Considering the candidate 290001_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 290001_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 290011_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 290011_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 290026_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 290026_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 290036_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 290036_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 290043_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 290043_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (94.2") between the two second-epoch detections
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Considering the candidate 228912_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 228912_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 199360_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 199360_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks
Rejecting candidate due to large distance (143.8") between the two second-epoch detections
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Considering the candidate 158645_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 158645_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 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 129229_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050
The candidate 129229_fd_Mon-02-Q1b1x1_2026-01-08_20-37-17_20.00sec_-14.90C_LIGHT_0050 did not pass the final checks