This analysis is done by the script util/transients/transient_factory_test31.sh /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461061.8418,12.24,0.05,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
VARIABLE_NAME 20260121.3418 12.24CV 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/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:46:40.95 +33:17:23.5 ;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_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20_00sec_-14_90C_LIGHT_0379_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20_00sec_-14_90C_LIGHT_0379_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 21.3419* 05 29 20.99 +28 06 53.4 12.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461061.8418,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260121.3418 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:29:20.99 +28:06:53.4 ;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_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20_00sec_-14_90C_LIGHT_0379_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20_00sec_-14_90C_LIGHT_0379_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 21.3418 2461061.8418 14.49 04:50:50.68 +33:57:16.5
169.16481 -6.66618 galactic Aur Second-epoch detections are separated by 4.4" 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 | Gaia DR3 161884704730002048 | 04:50:52.30 +33:57:42.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 161884704730002048,2461061.8418,14.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 161884704730002048 20260121.3418 14.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:50:50.68 +33:57:16.5 ;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_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20_00sec_-14_90C_LIGHT_0379_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20_00sec_-14_90C_LIGHT_0379_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 21.3419* 04 45 44.40 +25 04 05.8 13.3 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461061.8418,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260121.3418 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:45:44.40 +25:04:05.8 ;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_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20_00sec_-14_90C_LIGHT_0379_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20_00sec_-14_90C_LIGHT_0379_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,2461061.8418,13.40,0.05,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
VARIABLE_NAME 20260121.3418 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/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:09:16.63 +31:00:56.0 ;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_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20_00sec_-14_90C_LIGHT_0379_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20_00sec_-14_90C_LIGHT_0379_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,2461061.8418,13.53,0.05,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 20260121.3418 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:03:00.65 +32:13:54.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20_00sec_-14_90C_LIGHT_0379_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20_00sec_-14_90C_LIGHT_0379_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 21.3419* 05 05 54.70 +28 20 01.8 13.7 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461061.8418,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260121.3418 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:05:54.70 +28:20:01.8 ;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_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20_00sec_-14_90C_LIGHT_0379_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20_00sec_-14_90C_LIGHT_0379_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 21.3419* 04 49 47.01 +28 19 47.4 14.5 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461061.8418,14.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260121.3418 14.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:49:47.01 +28:19:47.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20_00sec_-14_90C_LIGHT_0380_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20_00sec_-14_90C_LIGHT_0379_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20_00sec_-14_90C_LIGHT_0380_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20_00sec_-15_00C_LIGHT_0362_fits__*pix.png resample_wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20_00sec_-14_90C_LIGHT_0379_fits__*pix.png animation_v2.gif
Processing complete!
Total number of candidates identified: 8
Processing log:
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.80049318 23.12.2025 07:12:32.611 /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
First image: 2461032.80049318 23.12.2025 07:12:32.611 /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Last image: 2461061.84219479 21.01.2026 08:12:35.630 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.59
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 37 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): 15348
Objects passed selection criteria: 15335
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 14469.8
Average stars matched: 14167.5 (97.9112 %)
Memory usage VmPeak: 117444 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Jan 14 09:05:05 CST 2026
VaST build number 1.0rc88-183-g45c3f81a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-01-14)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Jan 21 02:40:14 CST 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.80049318 23.12.2025 07:12:32.611 /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
First image: 2461032.80049318 23.12.2025 07:12:32.611 /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Last image: 2461061.84219479 21.01.2026 08:12:35.630 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 111
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.27
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 212 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): 120386
Objects passed selection criteria: 120195
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 112659
Average stars matched: 109232 (96.9583 %)
Memory usage VmPeak: 1897596 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Jan 14 09:05:05 CST 2026
VaST build number 1.0rc88-183-g45c3f81a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-01-14)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Jan 21 02:45:31 CST 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= 25
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= yes
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= 0
TELESCOP=
TELESCOP_NAME_KNOWN_TO_VaST_FOR_FOV_DETERMINATION=
UCAC5_PLATESOLVE_ITERATIONS= 2
FPACK_FULLY_CALIBRATED_IMAGE= no
#######################################
HOSTNAME= tau
USER=
HOME=
#######################################
Reference image directory is set to /mnt/usb2/NMW-TexasTech/reference_imgs
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:
Aur-05-Q1b1x1
#######################################
########### Starting Aur-05-Q1b1x1 ###########
Processing Aur-05-Q1b1x1
server tau has sufficient free disk space available: 160697 MB at /mnt/usb2/NMW-TexasTech/workdir
server tau has sufficient free disk space available: 160697 MB at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
REFERENCE_EPOCH__SECOND_IMAGE= /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.png' -> 'transient_report/Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits_preview.png'
Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits
renamed 'Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.png' -> 'transient_report/Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits_preview.png'
Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.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= 565.0960
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 645.3049
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 1266.3777
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 642.7504
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 1267.1853
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 642.2026
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 2.241
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_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits
CCD-TEMP= -14.900000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits
SET-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.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= '2026-01-21T02:11:35.4723636' / Time of observation (local)" status=0
Record 12: "DATE-OBS= '2026-01-21T08:11:35.4723636' / Time of observation (UTC)" status=0
Record 13: "MJD-OBS = 61061.3413827778 / Modified Julian Date of observation" status=0
Record 14: "DATE-AVG= '2026-01-21T08:11:45.3756391' / Averaged midpoint time (UTC)" status=0
Record 15: "MJD-AVG = 61061.3414973957 / 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 = 74.9993933067131 / [deg] RA of telescope" status=0
Record 32: "DEC = 30.0001402165207 / [deg] Declination of telescope" status=0
Record 33: "CENTALT = 34.5583333333333 / [deg] Altitude of telescope" status=0
Record 34: "CENTAZ = 285.716111111111 / [deg] Azimuth of telescope" status=0
Record 35: "AIRMASS = 1.7593621789556 / Airmass at frame center (Gueymard 1993)" status=0
Record 36: "PIERSIDE= 'East' / 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 = 'Aur-05' / Name of the object of interest" status=0
Record 46: "OBJCTRA = '05 00 00' / [H M S] RA of imaged object" status=0
Record 47: "OBJCTDEC= '+30 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_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits 9576 6388 16 bitpix
SET-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.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_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.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_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/d_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits :)
Spent 0.429988 seconds
renamed 'mdark_TTUQ1b1x1_-15C_20s_2026-01-08.png' -> 'transient_report/dark.png'
MegaDivider v7
Reading image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/d_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.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_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.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_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.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_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
CCD-TEMP= -14.900000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
SET-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.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= '2026-01-21T02:12:35.6300240' / Time of observation (local)" status=0
Record 12: "DATE-OBS= '2026-01-21T08:12:35.6300240' / Time of observation (UTC)" status=0
Record 13: "MJD-OBS = 61061.3420790508 / Modified Julian Date of observation" status=0
Record 14: "DATE-AVG= '2026-01-21T08:12:45.5348340' / Averaged midpoint time (UTC)" status=0
Record 15: "MJD-AVG = 61061.3421936803 / 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 = 74.9993933419154 / [deg] RA of telescope" status=0
Record 32: "DEC = 30.0001402021162 / [deg] Declination of telescope" status=0
Record 33: "CENTALT = 34.3577777777778 / [deg] Altitude of telescope" status=0
Record 34: "CENTAZ = 285.816388888889 / [deg] Azimuth of telescope" status=0
Record 35: "AIRMASS = 1.76830602300578 / Airmass at frame center (Gueymard 1993)" status=0
Record 36: "PIERSIDE= 'East' / 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 = 'Aur-05' / Name of the object of interest" status=0
Record 46: "OBJCTRA = '05 00 00' / [H M S] RA of imaged object" status=0
Record 47: "OBJCTDEC= '+30 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_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits 9576 6388 16 bitpix
SET-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.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_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.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_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/d_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits :)
Spent 0.424512 seconds
renamed 'mdark_TTUQ1b1x1_-15C_20s_2026-01-08.png' -> 'transient_report/dark.png'
MegaDivider v7
Reading image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/d_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.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_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.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_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.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_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits
SECOND_EPOCH__SECOND_IMAGE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.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 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.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: 2461061.84149852
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits exists and is non-empty
Saving wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits to local_wcs_cache/
'wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits' -> 'local_wcs_cache/wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits'
wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits exists and is non-empty
Saving wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits to local_wcs_cache/
'wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits' -> 'local_wcs_cache/wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits'
wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits exists and is non-empty
Saving wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits to local_wcs_cache/
'wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits' -> 'local_wcs_cache/wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits'
wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits exists and is non-empty
Saving wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits to local_wcs_cache/
'wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits' -> 'local_wcs_cache/wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:00:01.017 +29:59:40.48
Second-epoch image center 04:59:59.628 +30:00:21.14
Angular distance between the image centers 0.01 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 05:00:01.017 +29:59:40.48
Second-epoch image center 04:59:57.110 +29:59:43.71
Angular distance between the image centers 0.01 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 04:59:59.628 +30:00:21.14
Second-epoch second image center 04:59:57.110 +29:59:43.71
Angular distance between the image centers 0.01381 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/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits &> /tmp/tmp.asGDzg0m9O
Parallel run for /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits &> /tmp/tmp.TmZL3vQSDn
Parallel run for /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits &> /tmp/tmp.bIRyAC6tE0
Parallel run for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits &> /tmp/tmp.UrgzS5rRcr
Parallel run for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat
Found non-empty wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat
The reference image (wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits) and catalog (wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat) found
'wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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 6742 out of 16295 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.979657
a=0.000000 b=1.000000 c=22.979657
From vast_summary.log: estimated ref. image limiting mag.: -7.59
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.39
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.39
____ 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 4 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
1.9 pix Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
2.1 pix fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits
2.2 pix fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
Limiting magnitude estimates:
15.4 mag. Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
15.4 mag. Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
15.0 mag. fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits
15.0 mag. fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.asGDzg0m9O (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_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
verification OK: /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits has a WCS header - will blindly trust it is good...
'/mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits' -> 'wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits'
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS_IMAGE_NAME=wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS-calibrated image found: wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Checking if the catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat corresponding to the image wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits alredy exist and is non-empty...
Catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat corresponding to the image wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS catalog name: wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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=1498, passed=16295
Got 16295 stars (including 14768 good ones) from the SExtractor catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat
util/solve_plate_with_UCAC5 got 16295 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 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 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
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 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits -region wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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.TmZL3vQSDn (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_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
verification OK: /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits has a WCS header - will blindly trust it is good...
'/mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits' -> 'wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits'
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS_IMAGE_NAME=wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS-calibrated image found: wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Checking if the catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat corresponding to the image wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits alredy exist and is non-empty...
Catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat corresponding to the image wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS catalog name: wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.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=1486, passed=16349
Got 16349 stars (including 14839 good ones) from the SExtractor catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat
util/solve_plate_with_UCAC5 got 16349 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 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 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
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 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits -region wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.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.bIRyAC6tE0 (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_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits
FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits
verification OK: /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits
Checking if the catalog wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits.cat corresponding to the image wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits.cat corresponding to the image wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits
WCS catalog name: wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.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=1043, passed=12787
Got 12787 stars (including 11726 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits.cat
util/solve_plate_with_UCAC5 got 12787 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
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 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits -region wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.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.UrgzS5rRcr (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_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
verification OK: /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
Checking if the catalog wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits.cat corresponding to the image wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits.cat corresponding to the image wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
WCS catalog name: wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.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=1012, passed=12842
Got 12842 stars (including 11807 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits.cat
util/solve_plate_with_UCAC5 got 12842 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 952 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: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
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 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits -region wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.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_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits' -> '/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits'
Saving fully-calibrated image wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits' -> '/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits'
Preparing the HTML report for the field Aur-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out21134.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21143.dat to exclusion_list_local.txt
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21125_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
The candidate 21125_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380 did not pass the final checks
**** FOUND 05:36:07.69 +34:09:24.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21133_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
The candidate 21133_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380 did not pass the final checks
**** FOUND 05:33:36.85 +33:40:02.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21134_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
Preparing report for the candidate 21134_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
Successfully moved Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.png to transient_report/21134_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380_reference.png
Successfully moved Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.png to transient_report/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits_preview.png
Successfully moved fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.png to transient_report/21134_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380_discovery1.png
Successfully moved fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.png to transient_report/21134_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380_discovery2.png
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21143_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
Preparing report for the candidate 21143_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
Successfully moved Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.png to transient_report/21143_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380_reference.png
The output file transient_report/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits_preview.png already exist
Successfully moved fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.png to transient_report/21143_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380_discovery1.png
Successfully moved fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.png to transient_report/21143_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380_discovery2.png
Prepared the HTML report for the field Aur-05-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 ####
04:46:40.95 +33:17:23.5
05:29:20.99 +28:06:53.4
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 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Creating symlink local_wcs_cache/wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Creating symlink local_wcs_cache/exclusion_list_bbsc.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_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits exists and is non-empty
wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits exists and is non-empty
wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits exists and is non-empty
wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:00:01.017 +29:59:40.48
Second-epoch image center 04:59:59.628 +30:00:21.14
Angular distance between the image centers 0.01 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 05:00:01.017 +29:59:40.48
Second-epoch image center 04:59:57.110 +29:59:43.71
Angular distance between the image centers 0.01 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 04:59:59.628 +30:00:21.14
Second-epoch second image center 04:59:57.110 +29:59:43.71
Angular distance between the image centers 0.01381 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/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits &> /tmp/tmp.5ywmuhcsf2
Parallel run for /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits &> /tmp/tmp.wE01SP3LiH
Parallel run for /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits &> /tmp/tmp.mctTApDHNs
Parallel run for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits &> /tmp/tmp.Vcu97GPJJG
Parallel run for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat
Found non-empty wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat
The reference image (wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits) and catalog (wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat) found
'wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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 6875 out of 129003 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.825003
a=0.000000 b=1.000000 c=22.825003
From vast_summary.log: estimated ref. image limiting mag.: -7.27
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.56
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.56
____ 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 53 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.8 pix Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
1.9 pix Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
2.1 pix fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits
2.1 pix fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
Limiting magnitude estimates:
15.6 mag. Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
15.5 mag. Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
15.2 mag. fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits
15.2 mag. fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 14.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.5ywmuhcsf2 (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_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
verification OK: /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits has a WCS header - will blindly trust it is good...
'/mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits' -> 'wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits'
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS_IMAGE_NAME=wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS-calibrated image found: wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Checking if the catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat corresponding to the image wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits alredy exist and is non-empty...
Catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat corresponding to the image wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS catalog name: wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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=36, blended=14027, passed=128967
Got 128967 stars (including 114720 good ones) from the SExtractor catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat
util/solve_plate_with_UCAC5 got 128967 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 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 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits -region wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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.wE01SP3LiH (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_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
verification OK: /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits has a WCS header - will blindly trust it is good...
'/mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits' -> 'wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits'
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS_IMAGE_NAME=wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS-calibrated image found: wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Checking if the catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat corresponding to the image wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits alredy exist and is non-empty...
Catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat corresponding to the image wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS catalog name: wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.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=35, blended=13827, passed=129020
Got 129020 stars (including 114972 good ones) from the SExtractor catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat
util/solve_plate_with_UCAC5 got 129020 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 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 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
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 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits -region wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.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.mctTApDHNs (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_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits
FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits
verification OK: /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits
Checking if the catalog wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits.cat corresponding to the image wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits.cat corresponding to the image wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits
WCS catalog name: wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.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=14, blended=9548, passed=98647
Got 98647 stars (including 88952 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits.cat
util/solve_plate_with_UCAC5 got 98647 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
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 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits -region wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.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.Vcu97GPJJG (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_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
verification OK: /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
Checking if the catalog wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits.cat corresponding to the image wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits.cat corresponding to the image wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
WCS catalog name: wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.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=13, blended=9451, passed=97320
Got 97320 stars (including 87714 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits.cat
util/solve_plate_with_UCAC5 got 97320 stars from the SExtractor catalog
/mnt/usb2/NMW-TexasTech/workdir/vast_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
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 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits -region wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.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_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.fits
Saving fully-calibrated image wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-21_CI_Aur-05-Q1b1x1_023159_TTUQ1b1x1_3397_mhcGrj92/wcs_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.fits
Preparing the HTML report for the field Aur-05-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out151300.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151317.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151319.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151322.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151332.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151338.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151341.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151350.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151351.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151353.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151389.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151415.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151437.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151438.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151465.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151466.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151468.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151474.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151481.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151527.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151547.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out151289.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151405.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151412.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151430.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151439.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151562.dat to exclusion_list_local.txt
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Considering the candidate 151289_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
Preparing report for the candidate 151289_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
Successfully moved Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.png to transient_report/151289_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380_reference.png
The output file transient_report/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits_preview.png already exist
Successfully moved fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.png to transient_report/151289_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380_discovery1.png
Successfully moved fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.png to transient_report/151289_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380_discovery2.png
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Considering the candidate 151295_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
The candidate 151295_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380 did not pass the final checks
**** FOUND 04:58:10.36 +28:15:16.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151298_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
The candidate 151298_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380 did not pass the final checks
**** FOUND 04:41:09.78 +28:51:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151300_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
The candidate 151300_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380 did not pass the final checks
**** FOUND 05:07:59.00 +29:14:27.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151310_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
The candidate 151310_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380 did not pass the final checks
**** FOUND 05:01:28.61 +31:02:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151313_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
The candidate 151313_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380 did not pass the final checks
**** FOUND 05:28:08.32 +32:58:53.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151315_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
The candidate 151315_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380 did not pass the final checks
**** FOUND 05:16:24.92 +33:19:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151317_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
The candidate 151317_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380 did not pass the final checks
**** FOUND 05:23:05.41 +33:46:35.6 in Gaia DR2 blend (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.82, 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..14.80 -c=05:23:05.41 +33:46:35.6 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)
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Considering the candidate 151338_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
The candidate 151338_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380 did not pass the final checks
**** FOUND 04:28:07.27 +31:57:42.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151346_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
The candidate 151346_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380 did not pass the final checks
**** FOUND 04:39:21.17 +27:59:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151348_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
The candidate 151348_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380 did not pass the final checks
**** FOUND 05:28:56.43 +34:52:19.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151349_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
The candidate 151349_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380 did not pass the final checks
**** FOUND 05:29:32.44 +33:28:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151350_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
The candidate 151350_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380 did not pass the final checks
**** FOUND 04:35:37.54 +26:55:58.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151353_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
The candidate 151353_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380 did not pass the final checks
**** FOUND 04:46:40.94 +33:17:23.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 151373_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
The candidate 151373_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380 did not pass the final checks
**** FOUND 05:29:20.97 +28:06:53.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 151389_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
The candidate 151389_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380 did not pass the final checks
**** FOUND 05:05:45.96 +26:25:47.0 in Gaia DR2 single (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78, 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..13.78 -c=05:05:45.96 +26:25:47.0 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)VIZIER_GAIADR2_OUTPUT=# 0.515 3420381254386240896 076.44134569079 +26.42968567991 12.4233 11.5339 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.515#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151405_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
Preparing report for the candidate 151405_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
Successfully moved Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.png to transient_report/151405_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380_reference.png
The output file transient_report/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits_preview.png already exist
Successfully moved fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.png to transient_report/151405_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380_discovery1.png
Successfully moved fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.png to transient_report/151405_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380_discovery2.png
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Considering the candidate 151412_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
Preparing report for the candidate 151412_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
Successfully moved Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.png to transient_report/151412_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380_reference.png
The output file transient_report/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits_preview.png already exist
Successfully moved fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.png to transient_report/151412_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380_discovery1.png
Successfully moved fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.png to transient_report/151412_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380_discovery2.png
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Considering the candidate 151415_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
The candidate 151415_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380 did not pass the final checks
**** FOUND 04:29:38.24 +25:25:13.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151430_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
Preparing report for the candidate 151430_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
Successfully moved Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.png to transient_report/151430_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380_reference.png
The output file transient_report/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits_preview.png already exist
Successfully moved fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.png to transient_report/151430_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380_discovery1.png
Successfully moved fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.png to transient_report/151430_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380_discovery2.png
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Considering the candidate 151432_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
The candidate 151432_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380 did not pass the final checks
**** FOUND 05:28:52.21 +34:52:16.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151433_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
The candidate 151433_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380 did not pass the final checks
**** FOUND 05:19:27.51 +34:00:23.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 151437_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
The candidate 151437_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380 did not pass the final checks
**** FOUND 05:23:36.20 +29:35:08.5 in Gaia DR2 single (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71, 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..14.71 -c=05:23:36.20 +29:35:08.5 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)VIZIER_GAIADR2_OUTPUT=# 1.084 3446527915775596416 080.90068800556 +29.58596760080 13.9082 13.2907 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.084#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151439_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
Preparing report for the candidate 151439_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
Successfully moved Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.png to transient_report/151439_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380_reference.png
The output file transient_report/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits_preview.png already exist
Successfully moved fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.png to transient_report/151439_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380_discovery1.png
Successfully moved fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.png to transient_report/151439_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380_discovery2.png
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Considering the candidate 151442_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
The candidate 151442_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380 did not pass the final checks
**** FOUND 05:29:20.85 +33:12:11.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151454_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
The candidate 151454_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380 did not pass the final checks
**** FOUND 05:34:41.85 +31:29:54.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151455_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
The candidate 151455_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380 did not pass the final checks
**** FOUND 04:26:35.90 +31:24:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151460_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
The candidate 151460_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380 did not pass the final checks
**** FOUND 04:43:52.81 +26:43:11.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151465_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
The candidate 151465_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380 did not pass the final checks
**** FOUND 05:17:16.73 +32:46:23.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151509_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
The candidate 151509_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380 did not pass the final checks
**** FOUND 04:38:29.38 +31:30:17.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151523_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
The candidate 151523_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380 did not pass the final checks
**** FOUND 04:35:26.98 +31:27:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151527_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
The candidate 151527_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380 did not pass the final checks
**** FOUND 05:34:20.44 +32:24:26.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151542_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
The candidate 151542_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380 did not pass the final checks
**** FOUND 05:02:21.19 +28:21:02.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151547_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
The candidate 151547_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380 did not pass the final checks
**** FOUND 05:18:35.29 +31:00:22.4 in Gaia DR2 single (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37, 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..15.37 -c=05:18:35.29 +31:00:22.4 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)VIZIER_GAIADR2_OUTPUT=# 0.843 180295412760891904 079.64719671430 +31.00641517348 14.4176 13.8606 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.843#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 151562_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
Preparing report for the candidate 151562_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
Successfully moved Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.png to transient_report/151562_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380_reference.png
The output file transient_report/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits_preview.png already exist
Successfully moved fd_Aur-05-Q1b1x1_2026-01-21_02-11-35_20.00sec_-14.90C_LIGHT_0379.png to transient_report/151562_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380_discovery1.png
Successfully moved fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380.png to transient_report/151562_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380_discovery2.png
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Considering the candidate 139636_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380
The candidate 139636_fd_Aur-05-Q1b1x1_2026-01-21_02-12-35_20.00sec_-14.90C_LIGHT_0380 did not pass the final checks
