This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR
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
Gaia DR3 1824461361051681152,2461126.8959,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1824461361051681152 20260327.3959 10.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:40:32.02 +18:48:58.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461126.8959,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.3959 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:15:46.78 +25:54:05.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461126.8959,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.3959 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:34:22.24 +19:01:20.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191805.00+244401.4,2461126.8959,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191805.00+244401.4 20260327.3959 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:18:06.21 +24:44:08.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3959 2461126.8959 12.99 19:31:24.82 +17:41:51.7
53.17186 -0.48849 galactic Sge Second-epoch detections are separated by 3.2" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J292.8527+17.7076 | 19:31:24.96 +17:41:44.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J292.8527+17.7076,2461126.8959,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J292.8527+17.7076 20260327.3959 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:31:24.82 +17:41:51.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3959 2461126.8959 13.04 19:27:24.33 +25:06:15.7
59.23632 3.87035 galactic Vul Second-epoch detections are separated by 3.5" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J291.8557+25.0960 | 19:27:24.33 +25:06:15.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J291.8557+25.0960,2461126.8959,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J291.8557+25.0960 20260327.3959 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:27:24.33 +25:06:15.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J192813.01+255921.8,2461126.8959,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J192813.01+255921.8 20260327.3959 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:28:12.35 +25:59:09.4 ;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_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3959 2461126.8959 12.84 19:28:10.54 +23:26:27.4
57.85269 2.92691 galactic Vul Second-epoch detections are separated by 0.6" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2019649242190968320 | 19:28:10.61 +23:26:19.9 (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 2019649242190968320,2461126.8959,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2019649242190968320 20260327.3959 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:28:10.54 +23:26:27.4 ;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_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3959 2461126.8959 12.37 19:42:28.53 +24:15:43.0
60.15987 0.46802 galactic Vul Second-epoch detections are separated by 4.1" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J295.6259+24.2559 | 19:42:27.97 +24:15:37.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J295.6259+24.2559,2461126.8959,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J295.6259+24.2559 20260327.3959 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:42:28.53 +24:15:43.0 ;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_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1925203+261234,2461126.8959,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1925203+261234 20260327.3959 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:25:20.13 +26:12:36.0 ;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_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2024007293942889216,2461126.8959,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2024007293942889216 20260327.3959 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:22:17.41 +26:05:10.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_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
ASAS J190721+2339.7,2461126.8959,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J190721+2339.7 20260327.3959 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:07:20.93 +23:39:42.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4517811541041758464,2461126.8959,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4517811541041758464 20260327.3959 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:01:38.46 +19:21:28.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3959 2461126.8959 12.54 18:54:39.86 +19:48:37.1
51.04213 8.20694 galactic Her Second-epoch detections are separated by 0.4" and 3.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J283.6643+19.8182 | 18:54:39.86 +19:48:37.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 27.3959* 18 54 39.86 +19 48 37.1 12.5 U Her 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
ATO J283.6643+19.8182,2461126.8959,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J283.6643+19.8182 20260327.3959 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:54:39.86 +19:48:37.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191602.00+252323.6,2461126.8959,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J191602.00+252323.6 20260327.3959 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:16:03.07 +25:23:33.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2035700217820634880,2461126.8959,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2035700217820634880 20260327.3959 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:06:36.22 +25:05:42.0 ;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_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3959 2461126.8959 13.05 19:23:27.63 +25:36:41.7
59.26553 4.89538 galactic Vul Second-epoch detections are separated by 1.3" and 2.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 19:23:27.63 +25:36:41.7 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461126.8959,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.3959 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:23:27.63 +25:36:41.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3959 2461126.8959 13.01 19:28:26.77 +22:05:08.4
56.68937 2.22682 galactic Vul Second-epoch detections are separated by 4.0" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J292.1049+22.0919 | 19:28:26.77 +22:05:08.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J292.1049+22.0919,2461126.8959,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J292.1049+22.0919 20260327.3959 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:28:26.77 +22:05:08.4 ;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_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J192012.11+240047.9,2461126.8959,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J192012.11+240047.9 20260327.3959 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:20:12.05 +24:00:40.4 ;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_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20_00sec_-15_00C_LIGHT_0419_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20_00sec_-14_90C_LIGHT_0418_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.99380530 27.02.2026 11:50:54.778 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
First image: 2461098.99380530 27.02.2026 11:50:54.778 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Last image: 2461126.89620537 27.03.2026 09:30:22.144 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 28
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.87
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 17517
Objects passed selection criteria: 17476
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 14640.2
Average stars matched: 14271.5 (97.4813 %)
Memory usage VmPeak: 124060 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 27 05:34:41 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.99380530 27.02.2026 11:50:54.778 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
First image: 2461098.99380530 27.02.2026 11:50:54.778 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Last image: 2461126.89620537 27.03.2026 09:30:22.144 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 242
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.54
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 47 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 171906
Objects passed selection criteria: 171474
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 124185
Average stars matched: 118069 (95.0751 %)
Memory usage VmPeak: 2400980 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 27 05:40:17 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits
SExtractor catalog cache: saved Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat to cache
SExtractor catalog cache: saved Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.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: 2461126.89567703
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits exists and is non-empty
Saving wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits to local_wcs_cache/
'wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits' -> 'local_wcs_cache/wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits'
wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits exists and is non-empty
Saving wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits to local_wcs_cache/
'wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits' -> 'local_wcs_cache/wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits'
wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits exists and is non-empty
Saving wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits to local_wcs_cache/
'wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits' -> 'local_wcs_cache/wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits'
wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits exists and is non-empty
Saving wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits to local_wcs_cache/
'wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits' -> 'local_wcs_cache/wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.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 19:23:05.554 +21:59:47.51
Second-epoch image center 19:22:44.171 +22:00:37.54
Angular distance between the image centers 0.08 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 19:23:05.554 +21:59:47.51
Second-epoch image center 19:22:42.968 +22:00:43.54
Angular distance between the image centers 0.09 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 19:22:44.171 +22:00:37.54
Second-epoch second image center 19:22:42.968 +22:00:43.54
Angular distance between the image centers 0.00494 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits &> /tmp/tmp.6D8c0Oce4Y
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits &> /tmp/tmp.Lq9nawGArF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits &> /tmp/tmp.s6NhHz0awR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits &> /tmp/tmp.nQUb6BuaVD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits
Calibrating the magnitude scale
Found non-empty wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.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_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits and wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.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_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits and wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
Found non-empty wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits and wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
The reference image (wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits) and catalog (wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat) found
'wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.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 14431 out of 24236 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.881026
a=0.000000 b=1.000000 c=22.881026
From vast_summary.log: estimated ref. image limiting mag.: -7.87
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.01
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.01
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 21 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
2.2 pix Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
4.5 pix fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits
3.9 pix fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits
Limiting magnitude estimates:
15.0 mag. Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
15.0 mag. Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
14.0 mag. fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits
14.1 mag. fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 11.5 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.6D8c0Oce4Y (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits' -> 'wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WCS_IMAGE_NAME=wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WCS-calibrated image found: wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Checking if the catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits alredy exist and is non-empty...
Catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WCS catalog name: wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
SExtractor catalog parsing summary: zero_flux=4, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2379, passed=24232
Got 24232 stars (including 21810 good ones) from the SExtractor catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
util/solve_plate_with_UCAC5 got 24232 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 963 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: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.44"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits -region wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.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.Lq9nawGArF (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits' -> 'wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WCS_IMAGE_NAME=wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WCS-calibrated image found: wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
Checking if the catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits alredy exist and is non-empty...
Catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WCS catalog name: wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2427, passed=23940
Got 23940 stars (including 21482 good ones) from the SExtractor catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat
util/solve_plate_with_UCAC5 got 23940 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.48"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits -region wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.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.s6NhHz0awR (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits
WCS_IMAGE_NAME=wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits
WCS-calibrated image found: wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits
Checking if the catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits
WCS catalog name: wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=526, passed=12038
Got 12038 stars (including 11508 good ones) from the SExtractor catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits.cat
util/solve_plate_with_UCAC5 got 12038 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010421 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.80"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.83"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.84"
Estimated accuracy of the plate solution: 0.98"
Excluding outliers - 946 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits -region wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.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.nQUb6BuaVD (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits
WCS_IMAGE_NAME=wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits
WCS-calibrated image found: wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits
Checking if the catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits
WCS catalog name: wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=633, passed=13868
Got 13868 stars (including 13229 good ones) from the SExtractor catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits.cat
util/solve_plate_with_UCAC5 got 13868 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010421 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.77"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.80"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.80"
Estimated accuracy of the plate solution: 0.93"
Excluding outliers - 949 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits -region wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.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_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits'
Saving fully-calibrated image wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits'
Saving fully-calibrated image wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits'
Saving fully-calibrated image wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits'
Preparing the HTML report for the field Vul-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out30022.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02831_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 02831_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:40:05.78 +18:00:53.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13660_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 13660_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 18:54:45.32 +22:38:44.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16718_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 16718_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:28:42.18 +24:39:50.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10521_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 10521_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:16:13.19 +21:23:26.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21588_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 21588_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:02:34.32 +25:50:25.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30022_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
Preparing report for the candidate 30022_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07054_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 07054_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:18:48.48 +19:36:39.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17777_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 17777_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:25:25.50 +24:54:30.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08304_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 08304_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:15:02.85 +20:12:13.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10986_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 10986_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:12:36.94 +21:33:19.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10277_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 10277_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:15:17.63 +21:14:02.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07921_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 07921_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:26:13.41 +20:05:55.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13852_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 13852_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:17:43.83 +23:01:34.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07459_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 07459_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:26:28.77 +19:53:30.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17372_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 17372_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:28:57.19 +24:46:08.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07274_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 07274_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:25:28.93 +19:47:57.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07144_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 07144_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:34:35.00 +19:46:28.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16641_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 16641_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:06:38.69 +24:15:04.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20229_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 20229_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:22:51.08 +26:15:45.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04054_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 04054_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 18:56:06.29 +18:06:18.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22452_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 22452_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:43:43.02 +25:46:20.8 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Vul-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
19:40:32.02 +18:48:58.0
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits
SExtractor catalog cache: saved Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat to cache
SExtractor catalog cache: saved Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Creating symlink local_wcs_cache/wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
Creating symlink local_wcs_cache/wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits
Creating symlink local_wcs_cache/wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits exists and is non-empty
wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits exists and is non-empty
wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits exists and is non-empty
wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.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 19:23:05.554 +21:59:47.51
Second-epoch image center 19:22:44.171 +22:00:37.54
Angular distance between the image centers 0.08 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 19:23:05.554 +21:59:47.51
Second-epoch image center 19:22:42.968 +22:00:43.54
Angular distance between the image centers 0.09 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 19:22:44.171 +22:00:37.54
Second-epoch second image center 19:22:42.968 +22:00:43.54
Angular distance between the image centers 0.00494 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits &> /tmp/tmp.8ytlPXayWF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits &> /tmp/tmp.Q2CRRG8ODs
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits &> /tmp/tmp.tvstWYxLWj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits &> /tmp/tmp.NUM8cwrGZD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits
Calibrating the magnitude scale
Found non-empty wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.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_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits and wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.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_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits and wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
Found non-empty wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits and wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
The reference image (wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits) and catalog (wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat) found
'wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.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 15518 out of 221580 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.709941
a=0.000000 b=1.000000 c=22.709941
From vast_summary.log: estimated ref. image limiting mag.: -7.54
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.17
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.17
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 146 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
1.9 pix Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
4.7 pix fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits
4.0 pix fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits
Limiting magnitude estimates:
15.2 mag. Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
15.2 mag. Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
14.0 mag. fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits
14.2 mag. fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 13.2 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.8ytlPXayWF (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits' -> 'wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WCS_IMAGE_NAME=wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WCS-calibrated image found: wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Checking if the catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits alredy exist and is non-empty...
Catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WCS catalog name: wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=40, blended=30047, passed=221539
Got 221539 stars (including 191094 good ones) from the SExtractor catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
util/solve_plate_with_UCAC5 got 221539 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 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: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.46"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits -region wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.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.Q2CRRG8ODs (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits' -> 'wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WCS_IMAGE_NAME=wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WCS-calibrated image found: wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
Checking if the catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits alredy exist and is non-empty...
Catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WCS catalog name: wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=41, blended=30936, passed=228140
Got 228140 stars (including 196813 good ones) from the SExtractor catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat
util/solve_plate_with_UCAC5 got 228140 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.52"
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits -region wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.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.tvstWYxLWj (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits
WCS_IMAGE_NAME=wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits
WCS-calibrated image found: wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits
Checking if the catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits
WCS catalog name: wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=6866, passed=61680
Got 61680 stars (including 54779 good ones) from the SExtractor catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits.cat
util/solve_plate_with_UCAC5 got 61680 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010421 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.81"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.80"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.80"
Estimated accuracy of the plate solution: 0.90"
Excluding outliers - 949 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits -region wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.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.NUM8cwrGZD (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits
WCS_IMAGE_NAME=wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits
WCS-calibrated image found: wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits
Checking if the catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits
WCS catalog name: wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=7290, passed=75377
Got 75377 stars (including 68013 good ones) from the SExtractor catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits.cat
util/solve_plate_with_UCAC5 got 75377 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010421 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.73"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.72"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.72"
Estimated accuracy of the plate solution: 0.81"
Excluding outliers - 949 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits -region wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.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_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Saving fully-calibrated image wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
Saving fully-calibrated image wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-29-36_20.00sec_-14.90C_LIGHT_0418.fits
Saving fully-calibrated image wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_053144_TTUQ2b1x1_6371_anhqHdGR/wcs_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419.fits
Preparing the HTML report for the field Vul-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out233701.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254441.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254442.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254450.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254452.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254457.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254460.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254462.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254464.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254465.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254475.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254477.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254480.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254507.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254511.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254532.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254534.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254537.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out107429.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out143553.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out147973.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174599.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177075.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out187956.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191839.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195630.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254471.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254484.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254499.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254508.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254512.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254513.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254524.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254543.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59170.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70828.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 29s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 9s
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Considering the candidate 254441_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 254441_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:22:42.93 +17:55:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 1.102 4515012145751222912 290.67872017349 +17.91915712953 12.1527 10.7477 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.102#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254442_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 254442_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:29:46.90 +18:42:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 1.734 4323347512179033856 292.44493711652 +18.71497855016 12.4052 11.1884 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.734#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254445_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 254445_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:18:31.75 +26:00:37.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254450_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 254450_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 18:58:40.05 +23:37:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 0.971 4533139592111321472 284.66668669679 +23.61981847950 13.1176 12.2570 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.971#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254452_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 254452_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:34:30.02 +20:42:49.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)
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Considering the candidate 254457_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 254457_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:05:24.16 +22:08:32.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 0.818 4520690092520920576 286.35044966533 +22.14255048581 12.5529 11.5056 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.818#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254460_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 254460_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:34:39.29 +18:44:43.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 5.386 1825164292552968192 293.66273254054 +18.74435127314 13.1831 12.7805 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.386#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254462_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 254462_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:01:24.80 +24:56:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 1.298 4533879288556062080 285.35304220956 +24.94832912580 12.7622 11.9030 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.298#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254464_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 254464_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:39:53.04 +21:38:16.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)
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Considering the candidate 254465_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 254465_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:22:11.04 +18:02:01.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)
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Considering the candidate 254471_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
Preparing report for the candidate 254471_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
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Considering the candidate 254474_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 254474_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:38:47.19 +18:19:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254475_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 254475_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:23:57.13 +24:56:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 2.237 2023121671692621312 290.98735895758 +24.93425195126 13.2583 12.3647 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.237#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254477_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 254477_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:03:04.00 +25:07:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 1.190 4533898804888214144 285.76699238609 +25.13232270216 12.8465 12.0381 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.190#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254480_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 254480_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:34:31.15 +18:54:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 1.574 1825181231905162240 293.62992645603 +18.91477923198 12.7489 12.0999 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.574#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254484_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
Preparing report for the candidate 254484_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
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Considering the candidate 254499_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
Preparing report for the candidate 254499_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
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Considering the candidate 254507_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 254507_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 18:54:23.30 +22:15:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 1.707 4531440017704136960 283.59666242020 +22.26207604695 11.9553 10.7163 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.707#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254508_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
Preparing report for the candidate 254508_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
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Considering the candidate 254511_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 254511_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:01:15.20 +17:51:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 0.824 4514279974085073920 285.31341161174 +17.86025590869 12.3656 11.5305 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.824#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254512_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
Preparing report for the candidate 254512_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
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Considering the candidate 254513_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
Preparing report for the candidate 254513_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
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Considering the candidate 254524_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
Preparing report for the candidate 254524_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
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Considering the candidate 254532_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 254532_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:11:27.85 +18:49:33.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)
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Considering the candidate 254534_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 254534_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:45:16.28 +25:21:37.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)
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Considering the candidate 254536_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 254536_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 254537_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 254537_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:03:49.02 +21:09:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 3.843 4519774993927573376 285.95492181090 +21.16397548548 12.4124 11.4626 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.843#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254543_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
Preparing report for the candidate 254543_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
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Considering the candidate 254957_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 254957_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 18:54:38.45 +22:40:12.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255144_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 255144_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 255166_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 255166_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 255190_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 255190_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:25:26.96 +20:15:13.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 255203_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 255203_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:36:25.46 +23:56:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255303_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 255303_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 255399_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 255399_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 255403_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 255403_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:34:29.91 +19:47:38.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 255404_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 255404_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 255494_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 255494_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:36:27.68 +21:59:04.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255526_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 255526_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 255537_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 255537_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 255562_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 255562_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 255567_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 255567_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 255592_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 255592_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 255598_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 255598_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 255602_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 255602_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 255611_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 255611_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:41:27.81 +21:04:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255614_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 255614_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:24:20.63 +20:00:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255620_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 255620_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 255622_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 255622_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 255627_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 255627_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 255635_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 255635_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 255636_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 255636_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 255638_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 255638_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 255639_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 255639_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 255641_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 255641_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 255645_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 255645_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 255651_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 255651_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 255652_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 255652_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 255654_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 255654_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 255656_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 255656_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 129581_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 129581_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 18:54:45.27 +22:38:45.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 28662_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 28662_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:40:05.77 +18:00:53.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 209821_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 209821_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:22:51.06 +26:15:46.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 65594_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 65594_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:34:34.97 +19:46:28.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 165993_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 165993_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:28:42.16 +24:39:50.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 68296_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 68296_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:26:28.75 +19:53:31.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 129900_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 129900_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:17:43.81 +23:01:34.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 98492_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 98492_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:16:13.20 +21:23:28.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 140690_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 140690_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:39:20.43 +23:44:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 110128_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 110128_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 18:58:11.50 +21:52:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174599_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
Preparing report for the candidate 174599_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
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Considering the candidate 177075_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
Preparing report for the candidate 177075_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
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Considering the candidate 143553_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
Preparing report for the candidate 143553_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
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Considering the candidate 188880_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 188880_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:00:59.61 +25:17:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154477_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 154477_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:30:07.97 +24:22:54.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 161366_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 161366_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 52335_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 52335_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:27:53.60 +19:17:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59170_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
Preparing report for the candidate 59170_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
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Considering the candidate 177832_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 177832_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:02:34.34 +25:50:25.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30752_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 30752_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:05:00.99 +18:02:40.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70828_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
Preparing report for the candidate 70828_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
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Considering the candidate 191839_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
Preparing report for the candidate 191839_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
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Considering the candidate 71341_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 71341_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:43:04.76 +20:14:33.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234683_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 234683_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:49:47.11 +25:35:12.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234148_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 234148_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 18:55:16.91 +24:49:57.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195630_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
Preparing report for the candidate 195630_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
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Considering the candidate 187956_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
Preparing report for the candidate 187956_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
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Considering the candidate 233701_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 233701_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:16:48.47 +25:07:40.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 2.993 2023881365495206016 289.20253076797 +25.12862237348 13.7964 12.9023 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.993#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 121912_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 121912_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:45:37.51 +22:51:12.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198637_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 198637_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 64045_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 64045_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 107429_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
Preparing report for the candidate 107429_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
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Considering the candidate 147973_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
Preparing report for the candidate 147973_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
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Considering the candidate 161378_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 161378_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 120276_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 120276_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:43:34.04 +22:44:55.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90290_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 90290_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:26:58.97 +21:06:22.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 67609_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 67609_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:24:44.50 +19:56:23.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 105210_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 105210_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:17:31.98 +21:48:54.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 117889_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 117889_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:17:40.02 +22:26:28.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 75358_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 75358_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:23:12.19 +20:16:43.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 74738_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 74738_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:27:54.05 +20:14:51.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 112215_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 112215_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:20:54.39 +22:11:57.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 104274_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 104274_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:33:25.55 +21:50:20.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 141015_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 141015_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:11:10.45 +23:28:48.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 62768_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 62768_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:18:48.46 +19:36:39.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 74206_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 74206_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:26:30.60 +20:15:32.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 49066_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 49066_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:16:48.62 +18:58:33.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 74955_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 74955_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:25:22.42 +20:16:18.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 121209_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 121209_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:19:31.99 +22:34:15.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 74870_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 74870_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:23:46.97 +20:15:53.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52153_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 52153_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:20:59.96 +19:08:47.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 74394_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 74394_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:29:20.91 +20:16:48.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 71299_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 71299_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:26:13.39 +20:05:55.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 66017_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 66017_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:25:28.91 +19:47:57.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 94839_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 94839_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:15:17.63 +21:14:04.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 118172_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 118172_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:36:08.35 +22:35:10.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 33657_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 33657_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:27:26.57 +18:17:46.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 75620_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 75620_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:15:02.82 +20:12:14.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 101612_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 101612_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:12:36.92 +21:33:19.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 170317_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 170317_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:25:25.47 +24:54:31.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 83562_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 83562_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:38:17.78 +20:47:00.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166026_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 166026_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:28:57.22 +24:46:09.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 106317_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 106317_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:08:03.71 +21:42:00.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 47866_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 47866_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:35:07.59 +19:00:18.8 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 156680_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 156680_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:08:37.84 +24:10:45.9 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77766_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 77766_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:40:28.37 +20:28:37.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 86882_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 86882_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 18:58:41.40 +20:37:24.1 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 98333_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 98333_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:03:42.54 +21:16:07.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46953_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 46953_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:37:23.45 +18:58:36.7 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41097_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 41097_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:15:33.45 +18:31:01.6 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168768_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 168768_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:08:02.06 +24:43:35.1 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 91040_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 91040_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:01:22.56 +20:49:58.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116362_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 116362_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:41:14.59 +22:27:11.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 123511_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 123511_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:42:48.52 +22:51:06.5 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117927_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 117927_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:01:49.51 +22:15:53.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159112_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 159112_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:06:38.66 +24:15:05.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195167_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 195167_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:01:35.02 +25:01:33.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55929_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 55929_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:04:52.71 +19:08:41.7 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60420_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 60420_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:01:05.55 +19:18:35.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70643_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 70643_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 18:58:45.09 +19:47:41.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34054_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 34054_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 18:56:03.74 +17:59:43.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193572_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 193572_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:47:48.79 +25:23:03.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67608_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 67608_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:02:52.80 +19:39:42.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131782_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 131782_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 18:59:58.39 +22:48:53.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 184740_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 184740_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks
**** FOUND 19:43:43.00 +25:46:21.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37832_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419
The candidate 37832_fd_Vul-01-Q2b1x1_2026-03-27_04-30-22_20.00sec_-15.00C_LIGHT_0419 did not pass the final checks