This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 03 27.4461 2461126.9461 11.84 20:10:33.36 +20:52:52.8
60.62189 -6.82658 galactic Sge Second-epoch detections are separated by 1.5" and 1.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 1828844701550089088 | 20:10:33.88 +20:52:55.4 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 1828844701550089088,2461126.9461,11.84,0.05,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
Large-amplitude variable Gaia DR2 1828844701550089088 20260327.4461 11.84CV 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-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:10:33.36 +20:52:52.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4461 2461126.9461 10.93 20:34:34.37 +26:08:11.1
68.12562 -8.43419 galactic Vul Second-epoch detections are separated by 7.3" and 1.7 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 1855876950830279424 | 20:34:34.41 +26:08:19.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1855876950830279424,2461126.9461,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1855876950830279424 20260327.4461 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:34:34.37 +26:08:11.1 ;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-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4461 2461126.9461 13.45 20:10:34.75 +23:50:51.9
63.13695 -5.23148 galactic Vul Second-epoch detections are separated by 1.3" and 1.8 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 | 20:10:34.75 +23:50:51.9 (user input) | T | P | (position from user input) SpType: K4 (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,2461126.9461,13.45,0.05,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 20260327.4461 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:10:34.75 +23:50:51.9 ;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-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4461 2461126.9461 13.30 20:00:07.15 +23:42:01.8
61.73404 -3.28435 galactic Vul Second-epoch detections are separated by 4.9" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 20:00:07.15 +23:42:01.8 (user input) | T | P | (position from user input) J-Ks=1.295+/-0.033 (Very red! L if it's a dwarf)
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,2461126.9461,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.4461 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:00:07.15 +23:42:01.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_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 J195710.98+233220.6,2461126.9461,13.26,0.05,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 J195710.98+233220.6 20260327.4461 13.26CV 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-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:57:10.62 +23:32:28.4 ;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-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_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 J200936.41+222124.2,2461126.9461,13.02,0.05,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 J200936.41+222124.2 20260327.4461 13.02CV 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-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:09:35.89 +22:21:28.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4461 2461126.9461 12.99 20:10:47.86 +22:45:11.3
62.23902 -5.86548 galactic Vul Second-epoch detections are separated by 5.5" 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 J302.6975+22.7415 | 20:10:47.86 +22:45:11.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J302.6975+22.7415,2461126.9461,12.99,0.05,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 J302.6975+22.7415 20260327.4461 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-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:10:47.86 +22:45:11.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_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,2461126.9461,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.4461 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:52:23.14 +17:47:15.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_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,2461126.9461,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.4461 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:40:40.39 +25:22:16.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_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
CzeV123,2461126.9461,12.86,0.05,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
CzeV123 20260327.4461 12.86CV 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-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:49:18.35 +20:39:37.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4461 2461126.9461 12.99 19:50:20.23 +17:50:11.0
55.51571 -4.33992 galactic Sge Second-epoch detections are separated by 3.5" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J297.5824+17.8385 | 19:50:20.23 +17:50:11.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J297.5824+17.8385,2461126.9461,12.99,0.05,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 J297.5824+17.8385 20260327.4461 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-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:50:20.23 +17:50:11.0 ;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-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4461 2461126.9461 13.19 20:16:56.52 +22:09:59.5
62.52220 -7.37549 galactic Vul Second-epoch detections are separated by 1.2" and 1.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J304.2353+22.1670 | 20:16:54.43 +22:09:54.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.728+/-0.030 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J304.2353+22.1670,2461126.9461,13.19,0.05,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 J304.2353+22.1670 20260327.4461 13.19CV 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-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:16:56.52 +22:09:59.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_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 J195213.43+182006.3,2461126.9461,12.73,0.05,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 J195213.43+182006.3 20260327.4461 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:52:14.41 +18:20:26.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4461 2461126.9461 12.74 20:28:28.81 +18:32:09.0
60.98140 -11.63980 galactic Del Second-epoch detections are separated by 1.0" and 1.8 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 | ATO J307.1190+18.5335 | 20:28:28.81 +18:32:09.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 27.4461* 20 28 28.81 +18 32 09.0 12.7 U Del 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 J307.1190+18.5335,2461126.9461,12.74,0.05,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
ATO J307.1190+18.5335 20260327.4461 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-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:28:28.81 +18:32:09.0 ;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-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_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,2461126.9461,12.41,0.05,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
target 20260327.4461 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-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:08:48.80 +21:40:25.2 ;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-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4461 2461126.9461 12.91 19:51:20.07 +19:18:25.2
56.90717 -3.79940 galactic Sge Second-epoch detections are separated by 2.9" and 1.4 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 J297.8275+19.3102 | 19:51:20.07 +19:18:25.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J297.8275+19.3102,2461126.9461,12.91,0.05,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
ATO J297.8275+19.3102 20260327.4461 12.91CV 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-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:51:20.07 +19:18:25.2 ;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-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_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 1843575374208730752,2461126.9461,12.80,0.05,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 1843575374208730752 20260327.4461 12.80CV 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-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:44:15.26 +25:13:13.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20_00sec_-15_00C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20_00sec_-15_00C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20_00sec_-15_00C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20_00sec_-15_00C_LIGHT_0044_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4461 2461126.9461 12.75 19:49:29.94 +20:21:41.5
57.59883 -2.89298 galactic Vul Second-epoch detections are separated by 5.2" and 1.7 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 J297.3700+20.3609 | 19:49:29.94 +20:21:41.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J297.3700+20.3609,2461126.9461,12.75,0.05,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 J297.3700+20.3609 20260327.4461 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:49:29.94 +20:21:41.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4461 2461126.9461 13.44 20:28:51.78 +18:16:11.7
60.80834 -11.86397 galactic Del Second-epoch detections are separated by 2.2" and 1.4 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 J307.2208+18.2746 | 20:28:51.78 +18:16:11.7 (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!
TCP 2026 03 27.4461* 20 28 51.78 +18 16 11.7 13.4 U Del 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 J307.2208+18.2746,2461126.9461,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J307.2208+18.2746 20260327.4461 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:28:51.78 +18:16:11.7 ;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-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_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 1823541550814668160,2461126.9461,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1823541550814668160 20260327.4461 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:06:02.08 +20:16:22.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20_00sec_-14_90C_LIGHT_0500_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20_00sec_-15_00C_LIGHT_0499_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: 2461098.99517851 27.02.2026 11:52:53.423 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
First image: 2461098.99517851 27.02.2026 11:52:53.423 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Last image: 2461126.94634567 27.03.2026 10:42:34.266 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 107
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.96
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: 9 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): 21883
Objects passed selection criteria: 21862
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 20516.8
Average stars matched: 19895.8 (96.9732 %)
Memory usage VmPeak: 125880 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 07:27:26 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: 2461098.99517851 27.02.2026 11:52:53.423 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
First image: 2461098.99517851 27.02.2026 11:52:53.423 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Last image: 2461126.94634567 27.03.2026 10:42:34.266 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 216
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.61
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: 73 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): 195111
Objects passed selection criteria: 194634
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 3.0 2 4
Average stars detected per image: 158828
Average stars matched: 153328 (96.5374 %)
Memory usage VmPeak: 1957192 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 07:32:21 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-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits
SExtractor catalog cache: saved Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat to cache
SExtractor catalog cache: saved Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.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-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.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: 2461126.94583794
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-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits exists and is non-empty
Saving wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits to local_wcs_cache/
'wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits' -> 'local_wcs_cache/wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits'
wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits exists and is non-empty
Saving wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits to local_wcs_cache/
'wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits' -> 'local_wcs_cache/wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits'
wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits exists and is non-empty
Saving wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits to local_wcs_cache/
'wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits' -> 'local_wcs_cache/wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits'
wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits exists and is non-empty
Saving wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits to local_wcs_cache/
'wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits' -> 'local_wcs_cache/wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.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 20:18:28.950 +22:00:14.29
Second-epoch image center 20:18:33.159 +21:57:42.92
Angular distance between the image centers 0.05 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 20:18:28.950 +22:00:14.29
Second-epoch image center 20:18:33.903 +21:57:39.35
Angular distance between the image centers 0.05 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 20:18:33.159 +21:57:42.92
Second-epoch second image center 20:18:33.903 +21:57:39.35
Angular distance between the image centers 0.00304 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-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits &> /tmp/tmp.xxIUdkNSmM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits &> /tmp/tmp.H9neLAEj0A
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits &> /tmp/tmp.OD2iT0oxiQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits &> /tmp/tmp.Veh5kUaXaR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits
Calibrating the magnitude scale
Found non-empty wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
Found non-empty wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
The reference image (wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits) and catalog (wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat) found
'wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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 14549 out of 24638 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.758582
a=0.000000 b=1.000000 c=22.758582
From vast_summary.log: estimated ref. image limiting mag.: -7.96
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.80
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.80
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 97 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
2.0 pix Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
3.6 pix fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits
3.6 pix fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits
Limiting magnitude estimates:
14.8 mag. Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
14.8 mag. Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
14.3 mag. fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits
14.3 mag. fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 11.7 (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.xxIUdkNSmM (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-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits' -> 'wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WCS_IMAGE_NAME=wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WCS-calibrated image found: wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Checking if the catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits alredy exist and is non-empty...
Catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WCS catalog name: wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2463, passed=24638
Got 24638 stars (including 22152 good ones) from the SExtractor catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
util/solve_plate_with_UCAC5 got 24638 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (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 935 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: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.68"
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 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.67"
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 935 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits -region wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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.H9neLAEj0A (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-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.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-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.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-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.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-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits' -> 'wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WCS_IMAGE_NAME=wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WCS-calibrated image found: wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
Checking if the catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat corresponding to the image wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits alredy exist and is non-empty...
Catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat corresponding to the image wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WCS catalog name: wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2477, passed=24779
Got 24779 stars (including 22281 good ones) from the SExtractor catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat
util/solve_plate_with_UCAC5 got 24779 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (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 937 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: 0.67"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.70"
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 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.70"
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 936 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits -region wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.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.OD2iT0oxiQ (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-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.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-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits
WCS_IMAGE_NAME=wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits
WCS-calibrated image found: wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits
Checking if the catalog wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits.cat corresponding to the image wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits.cat corresponding to the image wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.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-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits
WCS catalog name: wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1374, passed=21719
Got 21719 stars (including 20339 good ones) from the SExtractor catalog wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits.cat
util/solve_plate_with_UCAC5 got 21719 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 938 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: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.68"
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 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.68"
Estimated accuracy of the plate solution: 0.79"
Excluding outliers - 932 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits -region wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.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.Veh5kUaXaR (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-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.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-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits
WCS_IMAGE_NAME=wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits
WCS-calibrated image found: wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits
Checking if the catalog wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits.cat corresponding to the image wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits.cat corresponding to the image wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.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-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits
WCS catalog name: wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1498, passed=22170
Got 22170 stars (including 20661 good ones) from the SExtractor catalog wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits.cat
util/solve_plate_with_UCAC5 got 22170 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 935 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: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.69"
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 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.69"
Estimated accuracy of the plate solution: 0.82"
Excluding outliers - 929 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits -region wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.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-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits'
Saving fully-calibrated image wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits'
Saving fully-calibrated image wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits'
Saving fully-calibrated image wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits'
Preparing the HTML report for the field Vul-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31632.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31664.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31690.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31716.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31731.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31736.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31747.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31758.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31760.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31773.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31778.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31779.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31788.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31790.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31791.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31794.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31795.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31799.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31801.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31813.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31819.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31824.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31847.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31853.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31856.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31867.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31880.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out22029.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31793.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 18s
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: 2s
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Considering the candidate 31403_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31403_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:26:35.72 +19:05:37.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31526_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31526_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 19:52:33.54 +19:06:26.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31563_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31563_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:26:15.38 +20:27:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31611_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31611_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:09:02.12 +21:39:43.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31622_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31622_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:08:52.58 +21:23:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31627_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31627_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 19:57:59.17 +18:05:47.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31632_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31632_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:12:29.57 +22:49:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)GAIADR2_OUTPUT=# 2.642 1830435248201667584 303.12276906161 +22.82272133310 11.4052 10.6797 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.642#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31635_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31635_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:10:17.91 +20:24:04.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31646_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31646_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:07:12.62 +18:12:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31648_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31648_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 19:54:24.91 +21:34:49.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31655_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31655_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:30:44.49 +21:26:48.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31660_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31660_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:04:59.86 +20:13:28.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31662_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31662_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:09:13.55 +22:58:46.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31664_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31664_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:09:02.28 +18:05:20.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.77, MAG_FAINT_SEARCH_LIMIT=12.75)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31669_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31669_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:23:14.26 +20:58:33.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31674_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31674_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:25:11.48 +22:31:55.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31677_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31677_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 19:51:24.48 +20:26:16.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31682_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31682_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:09:50.64 +20:58:20.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31688_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31688_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:06:51.93 +20:48:16.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31689_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31689_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:25:20.82 +20:56:01.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31690_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31690_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:19:39.96 +17:42:51.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31693_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31693_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 19:52:14.83 +19:43:12.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31694_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31694_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:11:06.85 +18:29:42.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31696_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31696_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:10:28.63 +22:26:02.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31706_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31706_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:10:06.05 +20:46:47.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31708_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31708_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:13:44.91 +22:17:59.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31709_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31709_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:13:31.51 +21:32:49.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31714_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31714_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:19:11.75 +21:31:52.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31716_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31716_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 19:56:05.64 +18:16:49.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31717_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31717_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:21:18.34 +20:44:30.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31718_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31718_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:03:14.75 +17:48:50.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31720_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31720_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:22:19.30 +22:01:07.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31723_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31723_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:10:46.18 +19:28:52.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31726_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31726_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:11:18.46 +20:53:49.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31727_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31727_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:17:45.15 +21:33:49.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31731_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31731_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:16:58.27 +19:00:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.81, MAG_FAINT_SEARCH_LIMIT=12.79)GAIADR2_OUTPUT=# 3.009 1810371085134638208 304.24362795134 +19.01324287248 11.8914 11.4940 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.009#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31732_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31732_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:07:57.31 +22:22:49.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31735_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31735_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:09:30.30 +20:43:10.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31736_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31736_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:27:55.77 +19:05:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 2.016 1815817138013757568 306.98286483708 +19.09832374264 11.3389 10.3700 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.016#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31738_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31738_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:18:32.72 +20:53:30.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31739_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31739_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:11:31.85 +23:09:16.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31741_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31741_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:20:49.47 +21:10:35.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31743_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31743_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:13:29.65 +21:10:53.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31746_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31746_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:11:27.90 +22:08:22.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31747_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31747_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:10:19.45 +20:02:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 1.625 1822744988997570944 302.58057353101 +20.04434242649 11.7580 11.3123 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.625#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31748_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31748_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:05:41.02 +20:37:47.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31752_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31752_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:24:09.71 +22:27:57.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31753_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31753_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:07:09.48 +23:13:14.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31754_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31754_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:04:04.95 +21:14:04.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31758_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31758_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:18:41.25 +21:30:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.86, MAG_FAINT_SEARCH_LIMIT=12.84)GAIADR2_OUTPUT=# 0.817 1829120026129717888 304.67210583625 +21.50051799890 11.7194 10.9510 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.817#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31760_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31760_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:20:18.64 +20:45:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 4.111 1828650049318861312 305.07658290224 +20.75580678780 11.7240 11.0524 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.111#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31762_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31762_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:15:31.04 +22:07:04.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31764_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31764_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:06:13.22 +19:53:46.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31767_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31767_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:13:14.72 +21:37:49.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31768_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31768_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:10:58.79 +20:05:05.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31769_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31769_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:33:35.83 +23:03:36.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31772_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31772_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:06:07.05 +20:09:07.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31773_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31773_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:07:47.34 +21:09:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 1.320 1829659336594095360 301.94740777762 +21.16588626676 11.8276 11.4481 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.320#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31776_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31776_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:15:04.48 +21:04:48.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31777_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31777_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:17:20.57 +23:33:44.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31778_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31778_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:29:24.53 +23:59:35.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 5.889 1831370314107356928 307.35231647897 +23.99153395711 11.9677 11.3791 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.889#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31779_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31779_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 19:58:42.61 +19:20:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.86, MAG_FAINT_SEARCH_LIMIT=12.84)GAIADR2_OUTPUT=# 1.559 1823060926801058432 299.67797759524 +19.33972595131 11.4432 10.4634 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.559#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31782_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31782_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:15:58.77 +20:05:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31785_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31785_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:02:04.57 +21:12:21.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31787_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31787_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:16:12.34 +21:17:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31788_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31788_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:11:40.83 +21:35:39.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 0.393 1829746232365693440 302.92017933239 +21.59420877251 11.4885 10.6320 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.393#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31790_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31790_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:10:00.80 +22:10:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.86, MAG_FAINT_SEARCH_LIMIT=12.84)GAIADR2_OUTPUT=# 1.460 1829824778730737664 302.50375395577 +22.16897430403 11.7151 10.9495 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.460#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31791_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31791_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:15:36.89 +21:09:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 1.010 1828900398681384960 303.90357198290 +21.15197215335 11.7998 11.3203 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.010#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31792_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31792_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:14:14.15 +21:15:41.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31793_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
Preparing report for the candidate 31793_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31794_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31794_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:14:41.00 +21:39:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 1.310 1829009215976076544 303.67121106838 +21.66123772804 11.7984 11.3169 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.310#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31795_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31795_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:03:35.45 +21:00:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 0.850 1823825327898033920 300.89752204358 +21.00704850853 11.6911 10.9571 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.850#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31797_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31797_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:07:16.25 +19:30:05.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31799_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31799_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:21:17.84 +20:40:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 4.401 1817010211213732224 305.32302748736 +20.66867998861 11.5336 10.8102 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.401#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31801_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31801_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:11:19.56 +22:20:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.86, MAG_FAINT_SEARCH_LIMIT=12.84)GAIADR2_OUTPUT=# 0.769 1829856286604659200 302.83162947263 +22.33862124533 11.6335 10.8519 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.769#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31803_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31803_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:06:32.83 +20:43:31.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31805_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31805_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:19:34.16 +22:45:42.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31809_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31809_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:04:38.24 +21:26:28.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31810_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31810_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:16:52.37 +21:56:25.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31811_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31811_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:08:46.53 +21:11:00.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31813_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31813_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:18:02.20 +23:41:02.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 1.526 1830411780496092416 304.50958605644 +23.68376510988 11.7705 11.3054 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.526#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31814_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31814_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:08:29.11 +21:50:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31818_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31818_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:12:19.79 +20:59:25.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31819_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31819_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:12:31.28 +21:47:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 0.867 1829756677726388480 303.13059195881 +21.79412136625 11.8745 11.6958 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.867#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31821_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31821_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:16:06.61 +23:39:57.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31824_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31824_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:23:38.32 +23:04:00.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.90, MAG_FAINT_SEARCH_LIMIT=12.88)GAIADR2_OUTPUT=# 0.889 1831021768926220800 305.90978652518 +23.06658475082 11.7760 11.3759 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.889#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31825_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31825_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 19:55:28.15 +18:58:37.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31833_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31833_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:07:36.86 +22:56:01.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31847_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31847_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:07:22.97 +21:16:23.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 2.221 1829675550073499776 301.84600713098 +21.27253268762 11.6403 10.8567 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.221#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31853_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31853_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:09:23.92 +22:58:48.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 1.141 1830123880256584576 302.34973383171 +22.97971681047 11.7746 11.2854 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.141#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31856_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31856_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:11:03.49 +22:25:46.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.92, MAG_FAINT_SEARCH_LIMIT=12.90)GAIADR2_OUTPUT=# 2.419 1830045471330386816 302.76525045937 +22.42940665788 11.6748 10.8176 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.419#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31867_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31867_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:07:29.40 +22:34:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 0.818 1830098110451529472 301.87230741173 +22.56946957927 11.9025 11.6698 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31869_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31869_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:02:28.71 +21:43:35.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31870_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31870_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 19:55:46.18 +21:07:26.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31880_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 31880_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:06:20.50 +22:52:28.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.92, MAG_FAINT_SEARCH_LIMIT=12.90)GAIADR2_OUTPUT=# 1.344 1833112004948972288 301.58558453924 +22.87435469296 11.7423 11.2755 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.344#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17681_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 17681_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 19:56:28.96 +23:54:46.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22029_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
Preparing report for the candidate 22029_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 21s
Prepared the HTML report for the field Vul-02-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 ####
20:34:34.37 +26:08:11.1
20:10:33.36 +20:52:52.8
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-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits
SExtractor catalog cache: saved Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat to cache
SExtractor catalog cache: saved Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.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-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Creating symlink local_wcs_cache/wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
Creating symlink local_wcs_cache/wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits
Creating symlink local_wcs_cache/wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.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-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits exists and is non-empty
wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits exists and is non-empty
wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits exists and is non-empty
wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.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 20:18:28.950 +22:00:14.29
Second-epoch image center 20:18:33.159 +21:57:42.92
Angular distance between the image centers 0.05 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 20:18:28.950 +22:00:14.29
Second-epoch image center 20:18:33.903 +21:57:39.35
Angular distance between the image centers 0.05 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 20:18:33.159 +21:57:42.92
Second-epoch second image center 20:18:33.903 +21:57:39.35
Angular distance between the image centers 0.00304 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-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits &> /tmp/tmp.EH6r09kOFA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits &> /tmp/tmp.StXAPZuFW8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits &> /tmp/tmp.ExIeGtiwoQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits &> /tmp/tmp.3FuYdoYldy
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits
Calibrating the magnitude scale
Found non-empty wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
Found non-empty wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
The reference image (wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits) and catalog (wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat) found
'wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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 17496 out of 232861 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.547121
a=0.000000 b=1.000000 c=22.547121
From vast_summary.log: estimated ref. image limiting mag.: -7.61
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.94
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.94
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 112 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.8 pix Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
1.9 pix Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
3.8 pix fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits
3.7 pix fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits
Limiting magnitude estimates:
14.9 mag. Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
14.9 mag. Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
14.3 mag. fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits
14.3 mag. fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 13.5 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.EH6r09kOFA (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-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits' -> 'wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WCS_IMAGE_NAME=wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WCS-calibrated image found: wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Checking if the catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits alredy exist and is non-empty...
Catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WCS catalog name: wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=34, blended=33174, passed=232827
Got 232827 stars (including 199306 good ones) from the SExtractor catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
util/solve_plate_with_UCAC5 got 232827 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (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 943 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: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.69"
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 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.69"
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 941 stars left (next iteration limit 1035)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits -region wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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.StXAPZuFW8 (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-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.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-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.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-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.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-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits' -> 'wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WCS_IMAGE_NAME=wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WCS-calibrated image found: wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
Checking if the catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat corresponding to the image wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits alredy exist and is non-empty...
Catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat corresponding to the image wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WCS catalog name: wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=51, blended=32901, passed=232172
Got 232172 stars (including 198927 good ones) from the SExtractor catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat
util/solve_plate_with_UCAC5 got 232172 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (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 945 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: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.70"
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 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.70"
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits -region wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.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.ExIeGtiwoQ (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-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.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-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits
WCS_IMAGE_NAME=wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits
WCS-calibrated image found: wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits
Checking if the catalog wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits.cat corresponding to the image wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits.cat corresponding to the image wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.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-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits
WCS catalog name: wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=16999, passed=113705
Got 113705 stars (including 96620 good ones) from the SExtractor catalog wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits.cat
util/solve_plate_with_UCAC5 got 113705 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 941 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: 0.74"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.68"
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 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.68"
Estimated accuracy of the plate solution: 0.80"
Excluding outliers - 935 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits -region wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.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.3FuYdoYldy (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-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.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-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits
WCS_IMAGE_NAME=wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits
WCS-calibrated image found: wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits
Checking if the catalog wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits.cat corresponding to the image wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits.cat corresponding to the image wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.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-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits
WCS catalog name: wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=18059, passed=119782
Got 119782 stars (including 101631 good ones) from the SExtractor catalog wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits.cat
util/solve_plate_with_UCAC5 got 119782 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 937 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: 0.75"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.70"
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 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.70"
Estimated accuracy of the plate solution: 0.83"
Excluding outliers - 931 stars left (next iteration limit 1024)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits -region wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.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-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Saving fully-calibrated image wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.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-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
Saving fully-calibrated image wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.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-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-41-50_20.00sec_-15.00C_LIGHT_0499.fits
Saving fully-calibrated image wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.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-02-Q2b1x1_072339_TTUQ2b1x1_8108_9yWnCi2h/wcs_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500.fits
Preparing the HTML report for the field Vul-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out262692.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262694.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262698.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262710.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262713.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262729.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262744.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262758.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262760.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262768.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262793.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262795.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262812.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out263862.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out264332.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57832.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out262735.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out121456.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132011.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out245147.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out262726.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out262730.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out262754.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out262755.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out262761.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out262788.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out262792.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out262797.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30784.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31883.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38298.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65884.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out85674.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94287.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 28s
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 262692_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 262692_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:26:16.31 +21:14:24.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)
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Considering the candidate 262694_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 262694_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:27:08.40 +23:32:32.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)
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Considering the candidate 262698_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 262698_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:10:46.11 +25:17:16.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)
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Considering the candidate 262710_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 262710_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:16:20.10 +25:33:00.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)
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Considering the candidate 262713_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 262713_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 19:52:32.78 +26:04:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 1.595 2027043904523298816 298.13631729628 +26.07329355528 13.1555 12.3925 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.595#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 262726_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
Preparing report for the candidate 262726_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
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Considering the candidate 262729_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 262729_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:14:39.07 +19:22:05.9 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 262730_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
Preparing report for the candidate 262730_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
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Considering the candidate 262735_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 262735_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:39:57.01 +25:29:33.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)
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Considering the candidate 262744_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 262744_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:00:54.69 +21:21:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 3.840 1823816978488711296 300.22851515054 +21.35572651239 13.0467 12.2743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.840#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 262752_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 262752_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 262754_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
Preparing report for the candidate 262754_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
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Considering the candidate 262755_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
Preparing report for the candidate 262755_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
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Considering the candidate 262758_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 262758_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 19:53:23.21 +25:57:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 1.098 2026852280259003136 298.34702013973 +25.96612000525 13.1558 12.6306 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.098#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 262760_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 262760_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:44:54.74 +24:50:33.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 3.357 1843339906920424576 311.22858046688 +24.84190617921 12.9268 12.1345 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.357#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 262761_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
Preparing report for the candidate 262761_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
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Considering the candidate 262768_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 262768_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 19:58:41.63 +25:45:51.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)
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Considering the candidate 262773_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 262773_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:05:09.66 +20:31:37.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262775_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 262775_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 262778_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 262778_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 19:59:34.20 +23:17:13.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262785_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 262785_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 262788_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
Preparing report for the candidate 262788_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
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Considering the candidate 262791_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 262791_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:34:44.07 +25:27:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262792_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
Preparing report for the candidate 262792_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
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Considering the candidate 262793_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 262793_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:15:54.50 +19:18:41.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 4.262 1816434097178646272 303.97641823925 +19.31055160640 13.0769 12.3195 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.262#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 262795_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 262795_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:21:32.92 +25:57:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 4.257 1832775283820666112 305.38651526323 +25.96419408149 13.4238 12.9158 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.257#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 262796_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 262796_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 262797_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
Preparing report for the candidate 262797_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
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Considering the candidate 262805_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 262805_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 262812_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 262812_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 19:48:59.48 +23:38:17.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)
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Considering the candidate 262823_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 262823_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 263162_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 263162_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 263310_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 263310_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 263491_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 263491_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:21:47.54 +23:37:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263494_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 263494_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 263558_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 263558_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 263662_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 263662_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 263748_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 263748_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 263755_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 263755_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 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 263795_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 263795_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 263862_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 263862_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:17:42.45 +20:24:12.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)
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Considering the candidate 263893_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 263893_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 263955_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 263955_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 263977_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 263977_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 263988_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 263988_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 264064_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 264064_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 264072_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 264072_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 264099_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 264099_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 264136_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 264136_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 264143_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 264143_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 264168_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 264168_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 264174_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 264174_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 264257_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 264257_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:27:00.40 +22:20:56.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264271_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 264271_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 264276_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 264276_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 264322_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 264322_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 264332_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 264332_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:32:42.38 +21:20:49.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)
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Considering the candidate 264343_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 264343_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 264361_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 264361_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 264382_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 264382_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 264394_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 264394_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 264403_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 264403_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 264442_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 264442_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 264446_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 264446_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:36:21.77 +23:51:53.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264454_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 264454_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 264456_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 264456_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 264462_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 264462_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 264463_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 264463_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 264469_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 264469_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 264472_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 264472_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 264476_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 264476_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 188890_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 188890_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:43:29.83 +25:08:51.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30784_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
Preparing report for the candidate 30784_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
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Considering the candidate 40773_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 40773_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 19:50:23.79 +18:15:30.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 134142_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 134142_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:06:18.69 +22:08:28.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 40099_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 40099_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 19:51:28.83 +18:15:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 132011_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
Preparing report for the candidate 132011_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
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Considering the candidate 41910_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
Preparing report for the candidate 41910_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
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Considering the candidate 53589_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 53589_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:20:03.56 +19:07:57.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57832_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 57832_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:24:58.39 +19:20:11.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)
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Considering the candidate 112495_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 112495_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 38298_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
Preparing report for the candidate 38298_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
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Considering the candidate 166677_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 166677_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:42:22.16 +23:43:46.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 121456_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
Preparing report for the candidate 121456_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
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Considering the candidate 65884_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
Preparing report for the candidate 65884_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
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Considering the candidate 176744_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 176744_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 19:56:28.96 +23:54:46.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245283_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 245283_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:01:59.00 +19:58:14.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 122555_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 122555_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 245147_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
Preparing report for the candidate 245147_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
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Considering the candidate 245030_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 245030_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 19:51:20.43 +17:55:55.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 87318_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 87318_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:26:15.34 +20:27:02.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 60371_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 60371_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 19:52:33.33 +19:06:25.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35196_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 35196_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 19:52:12.11 +18:03:13.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149736_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 149736_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:11:00.00 +22:51:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 94287_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
Preparing report for the candidate 94287_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
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Considering the candidate 34531_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 34531_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:07:12.63 +18:12:28.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168079_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 168079_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:15:30.46 +23:30:32.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 201455_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 201455_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:22:03.60 +24:26:46.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 182867_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 182867_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:16:47.34 +24:40:15.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 31883_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
Preparing report for the candidate 31883_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
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Considering the candidate 171440_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 171440_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:06:53.72 +23:36:53.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 81811_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 81811_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:05:09.85 +19:59:33.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 229413_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 229413_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:15:16.09 +25:35:31.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 161057_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 161057_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 19:59:10.71 +23:06:05.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 192719_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 192719_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:01:44.94 +24:48:02.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 188455_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 188455_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 20:02:01.96 +24:56:18.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 154097_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 154097_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 19:51:04.34 +22:36:37.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 74911_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 74911_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 19:58:46.13 +19:29:37.1 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 85674_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
Preparing report for the candidate 85674_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
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Considering the candidate 182870_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 182870_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 19:53:27.96 +24:04:49.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 197384_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 197384_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks
**** FOUND 19:54:31.39 +24:19:10.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 231923_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500
The candidate 231923_fd_Vul-02-Q2b1x1_2026-03-27_05-42-34_20.00sec_-14.90C_LIGHT_0500 did not pass the final checks