This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461126.9414,13.51,0.05,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 20260327.4414 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:23:37.95 +25:23:34.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20_00sec_-15_00C_LIGHT_0492_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20_00sec_-14_90C_LIGHT_0491_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20_00sec_-15_00C_LIGHT_0492_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20_00sec_-14_90C_LIGHT_0491_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 1824066979978503808,2461126.9414,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1824066979978503808 20260327.4414 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:41:21.56 +17:44:08.3 ;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-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20_00sec_-15_00C_LIGHT_0492_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20_00sec_-14_90C_LIGHT_0491_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20_00sec_-15_00C_LIGHT_0492_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J192322.76+234858.0,2461126.9414,13.30,0.05,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
ZTF J192322.76+234858.0 20260327.4414 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-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:23:23.41 +23:49:16.6 ;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-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20_00sec_-15_00C_LIGHT_0492_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20_00sec_-14_90C_LIGHT_0491_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20_00sec_-15_00C_LIGHT_0492_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20_00sec_-14_90C_LIGHT_0491_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 J193644.71+260041.5,2461126.9414,13.07,0.05,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 J193644.71+260041.5 20260327.4414 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:36:44.76 +26:00:47.8 ;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-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20_00sec_-15_00C_LIGHT_0492_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20_00sec_-14_90C_LIGHT_0491_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20_00sec_-15_00C_LIGHT_0492_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4414 2461126.9414 13.31 19:31:31.04 +20:15:04.1
55.42172 0.71942 galactic Vul Second-epoch detections are separated by 1.9" 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 J292.8769+20.2505 | 19:31:30.45 +20:15:01.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J292.8769+20.2505,2461126.9414,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J292.8769+20.2505 20260327.4414 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:31:31.04 +20:15:04.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20_00sec_-15_00C_LIGHT_0492_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20_00sec_-14_90C_LIGHT_0491_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20_00sec_-15_00C_LIGHT_0492_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 27.4414* 18 54 15.33 +19 33 19.8 12.7 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J185415.41+193325.3,2461126.9414,12.66,0.05,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 J185415.41+193325.3 20260327.4414 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:54:15.33 +19:33:19.8 ;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-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20_00sec_-15_00C_LIGHT_0492_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20_00sec_-14_90C_LIGHT_0491_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20_00sec_-15_00C_LIGHT_0492_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1935282+184844,2461126.9414,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1935282+184844 20260327.4414 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:35:27.15 +18:48:38.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20_00sec_-15_00C_LIGHT_0492_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20_00sec_-14_90C_LIGHT_0491_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20_00sec_-15_00C_LIGHT_0492_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4414 2461126.9414 13.41 19:04:04.85 +23:45:17.4
55.59101 7.97652 galactic Vul Second-epoch detections are separated by 3.5" and 1.0 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 J286.0229+23.7589 | 19:04:04.85 +23:45:17.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J286.0229+23.7589,2461126.9414,13.41,0.05,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
ATO J286.0229+23.7589 20260327.4414 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:04:04.85 +23:45:17.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20_00sec_-15_00C_LIGHT_0492_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20_00sec_-14_90C_LIGHT_0491_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20_00sec_-15_00C_LIGHT_0492_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4414 2461126.9414 13.20 19:18:14.54 +25:01:49.1
58.19992 5.67160 galactic Vul Second-epoch detections are separated by 1.0" 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 J289.5665+25.0255 | 19:18:14.54 +25:01:49.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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 J289.5665+25.0255,2461126.9414,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J289.5665+25.0255 20260327.4414 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:18:14.54 +25:01:49.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20_00sec_-15_00C_LIGHT_0492_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20_00sec_-14_90C_LIGHT_0491_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20_00sec_-15_00C_LIGHT_0492_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.4414 2461126.9414 13.44 19:25:03.71 +24:52:50.1
58.78753 4.23324 galactic Vul Second-epoch detections are separated by 0.9" 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 J291.2595+24.8779 | 19:25:03.71 +24:52:50.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J291.2595+24.8779,2461126.9414,13.44,0.05,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 J291.2595+24.8779 20260327.4414 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-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:25:03.71 +24:52:50.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20_00sec_-15_00C_LIGHT_0492_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20_00sec_-14_90C_LIGHT_0491_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20_00sec_-15_00C_LIGHT_0492_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.99380530 27.02.2026 11:50:54.778 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
First image: 2461098.99380530 27.02.2026 11:50:54.778 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Last image: 2461126.94162515 27.03.2026 10:35:46.413 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 44
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.87
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 6 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): 18650
Objects passed selection criteria: 18637
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 17446.8
Average stars matched: 16944.8 (97.1227 %)
Memory usage VmPeak: 124060 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 27 07:23:57 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.99380530 27.02.2026 11:50:54.778 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
First image: 2461098.99380530 27.02.2026 11:50:54.778 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Last image: 2461126.94162515 27.03.2026 10:35:46.413 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 203
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.54
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 85 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): 174355
Objects passed selection criteria: 174004
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 148596
Average stars matched: 142167 (95.673 %)
Memory usage VmPeak: 1944784 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 07:27:44 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits
SExtractor catalog cache: saved Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat to cache
SExtractor catalog cache: saved Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.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: 2461126.94111470
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits exists and is non-empty
Saving wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits to local_wcs_cache/
'wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits' -> 'local_wcs_cache/wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits'
wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits exists and is non-empty
Saving wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits to local_wcs_cache/
'wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits' -> 'local_wcs_cache/wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits'
wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits exists and is non-empty
Saving wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits to local_wcs_cache/
'wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits' -> 'local_wcs_cache/wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits'
wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits exists and is non-empty
Saving wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits to local_wcs_cache/
'wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits' -> 'local_wcs_cache/wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:23:05.554 +21:59:47.51
Second-epoch image center 19:23:04.219 +21:58:21.78
Angular distance between the image centers 0.02 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:23:05.554 +21:59:47.51
Second-epoch image center 19:23:04.737 +21:58:14.01
Angular distance between the image centers 0.03 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 19:23:04.219 +21:58:21.78
Second-epoch second image center 19:23:04.737 +21:58:14.01
Angular distance between the image centers 0.00294 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits &> /tmp/tmp.tvsjcXRvzn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits &> /tmp/tmp.l0k5sYLSNZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits &> /tmp/tmp.20U7N6Sg2r
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits &> /tmp/tmp.yuBhW734RX
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits
Calibrating the magnitude scale
Found non-empty wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits and wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits and wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
Found non-empty wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits and wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
The reference image (wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits) and catalog (wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat) found
'wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 14431 out of 24236 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.881026
a=0.000000 b=1.000000 c=22.881026
From vast_summary.log: estimated ref. image limiting mag.: -7.87
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.01
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.01
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 39 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
2.2 pix Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
3.2 pix fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits
3.0 pix fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits
Limiting magnitude estimates:
15.0 mag. Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
15.0 mag. Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
14.5 mag. fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits
14.7 mag. fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.9 (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.tvsjcXRvzn (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits' -> 'wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WCS_IMAGE_NAME=wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WCS-calibrated image found: wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Checking if the catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits alredy exist and is non-empty...
Catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WCS catalog name: wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
SExtractor catalog parsing summary: zero_flux=4, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2379, passed=24232
Got 24232 stars (including 21810 good ones) from the SExtractor catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
util/solve_plate_with_UCAC5 got 24232 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.44"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits -region wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.l0k5sYLSNZ (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits' -> 'wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WCS_IMAGE_NAME=wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WCS-calibrated image found: wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
Checking if the catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits alredy exist and is non-empty...
Catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WCS catalog name: wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2427, passed=23940
Got 23940 stars (including 21482 good ones) from the SExtractor catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat
util/solve_plate_with_UCAC5 got 23940 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.48"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits -region wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.20U7N6Sg2r (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits
WCS_IMAGE_NAME=wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits
WCS-calibrated image found: wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits
Checking if the catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits
WCS catalog name: wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1347, passed=19861
Got 19861 stars (including 18491 good ones) from the SExtractor catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits.cat
util/solve_plate_with_UCAC5 got 19861 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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 957 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: 0.71"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.76"
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 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.76"
Estimated accuracy of the plate solution: 0.90"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits -region wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.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.yuBhW734RX (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits
WCS_IMAGE_NAME=wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits
WCS-calibrated image found: wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits
Checking if the catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits
WCS catalog name: wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1558, passed=21660
Got 21660 stars (including 20082 good ones) from the SExtractor catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits.cat
util/solve_plate_with_UCAC5 got 21660 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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 957 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: 0.63"
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 957 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 - 953 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits -region wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits'
Saving fully-calibrated image wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits'
Saving fully-calibrated image wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits'
Saving fully-calibrated image wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits'
Preparing the HTML report for the field Vul-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31490.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31491.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31499.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31526.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31527.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31528.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31529.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31537.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31539.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31555.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31559.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31575.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 2s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 31427_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31427_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:25:07.41 +21:09:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31451_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31451_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:26:03.95 +23:22:21.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31454_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31454_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:36:16.68 +18:52:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31460_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31460_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:24:40.70 +21:56:32.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31462_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31462_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:05:00.91 +18:02:40.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31467_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31467_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:45:37.52 +22:51:13.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31471_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31471_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:14:44.60 +18:30:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31473_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31473_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:03:27.66 +17:48:22.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31477_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31477_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:07:16.24 +20:04:58.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31479_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31479_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:16:53.18 +20:23:11.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31487_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31487_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:25:41.39 +22:22:13.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31490_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31490_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:23:36.77 +22:10:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 0.980 2019084501179175424 290.90349117825 +22.18126843518 11.8258 11.3861 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.980#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31491_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31491_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:20:51.83 +21:42:35.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 0.919 2019044201527780352 290.21622985444 +21.70979439356 11.7637 11.2078 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.919#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31495_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31495_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:18:46.06 +23:16:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31499_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31499_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:20:09.50 +22:34:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.00, MAG_FAINT_SEARCH_LIMIT=12.98)GAIADR2_OUTPUT=# 0.717 2022158533858902912 290.03979452476 +22.58262432100 11.8892 11.3760 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.717#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31500_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31500_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:13:56.18 +19:41:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31503_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31503_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:39:20.35 +23:44:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31505_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31505_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:26:45.62 +20:31:02.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31509_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31509_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:19:11.22 +19:28:54.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31513_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31513_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:26:46.79 +22:12:03.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31516_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31516_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:00:42.38 +19:58:24.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31517_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31517_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:19:17.27 +22:38:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31526_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31526_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:16:27.27 +21:56:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 1.324 4520119892657091328 289.11395531869 +21.93885204373 11.8417 11.2996 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.324#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31527_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31527_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:19:47.10 +22:01:34.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 1.551 2019111443538051328 289.94666827502 +22.02638245346 11.8873 11.3453 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.551#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31528_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31528_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:15:07.79 +20:54:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 4.121 4516928701923472768 288.78274737114 +20.91533193502 11.8984 11.3422 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.121#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31529_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31529_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:33:12.11 +20:10:28.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.737 1825600485100121344 293.30058872575 +20.17480301723 12.1795 11.6940 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.737#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31532_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31532_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:18:03.65 +23:17:22.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31533_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31533_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 18:57:18.85 +19:37:08.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31537_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31537_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:01:14.30 +21:48:29.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.08, MAG_FAINT_SEARCH_LIMIT=13.06)GAIADR2_OUTPUT=# 0.872 4520619659372832512 285.30970452605 +21.80826998892 11.7380 10.8854 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.872#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31539_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31539_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:23:09.29 +22:58:24.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.08, MAG_FAINT_SEARCH_LIMIT=13.06)GAIADR2_OUTPUT=# 0.709 2019289426985187712 290.78891891978 +22.97347907971 11.8233 11.2212 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.709#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31542_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31542_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 18:54:03.16 +19:36:34.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31546_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31546_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:14:56.45 +21:44:43.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31555_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31555_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:18:12.62 +22:02:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 2.675 4520113604824960512 289.55308198604 +22.03635953222 11.8582 11.3504 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.675#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31559_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31559_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:13:43.96 +21:17:02.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 5.452 4519979090776785024 288.43309233138 +21.28245941244 11.4215 10.3533 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.452#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31566_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31566_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:02:39.74 +21:35:20.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31575_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31575_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:00:46.14 +23:05:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 2.690 4533051218850418560 285.19165469834 +23.09298075765 11.9171 11.3521 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.690#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31579_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31579_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 18:54:11.21 +21:30:03.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31586_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 31586_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:14:36.16 +25:04:52.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21588_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 21588_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:02:34.30 +25:50:26.1 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 3s
Prepared the HTML report for the field Vul-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits
SExtractor catalog cache: saved Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat to cache
SExtractor catalog cache: saved Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Creating symlink local_wcs_cache/wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
Creating symlink local_wcs_cache/wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits
Creating symlink local_wcs_cache/wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits exists and is non-empty
wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits exists and is non-empty
wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits exists and is non-empty
wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:23:05.554 +21:59:47.51
Second-epoch image center 19:23:04.219 +21:58:21.78
Angular distance between the image centers 0.02 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:23:05.554 +21:59:47.51
Second-epoch image center 19:23:04.737 +21:58:14.01
Angular distance between the image centers 0.03 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 19:23:04.219 +21:58:21.78
Second-epoch second image center 19:23:04.737 +21:58:14.01
Angular distance between the image centers 0.00294 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits &> /tmp/tmp.xYzzygT2LI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits &> /tmp/tmp.AtQXZHZPTC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits &> /tmp/tmp.AA8U6PZeNw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits &> /tmp/tmp.rj1GQmBIDI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits
Calibrating the magnitude scale
Found non-empty wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits and wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits and wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
Found non-empty wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits and wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
The reference image (wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits) and catalog (wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat) found
'wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 15518 out of 221580 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.709941
a=0.000000 b=1.000000 c=22.709941
From vast_summary.log: estimated ref. image limiting mag.: -7.54
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.17
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.17
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 112 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
1.9 pix Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
3.3 pix fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits
3.0 pix fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits
Limiting magnitude estimates:
15.2 mag. Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
15.2 mag. Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
14.6 mag. fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits
14.7 mag. fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 13.9 (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.xYzzygT2LI (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits' -> 'wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WCS_IMAGE_NAME=wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WCS-calibrated image found: wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Checking if the catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits alredy exist and is non-empty...
Catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WCS catalog name: wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=40, blended=30047, passed=221539
Got 221539 stars (including 191094 good ones) from the SExtractor catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
util/solve_plate_with_UCAC5 got 221539 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.46"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits -region wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.AtQXZHZPTC (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits' -> 'wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WCS_IMAGE_NAME=wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WCS-calibrated image found: wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
Checking if the catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits alredy exist and is non-empty...
Catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WCS catalog name: wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=41, blended=30936, passed=228140
Got 228140 stars (including 196813 good ones) from the SExtractor catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat
util/solve_plate_with_UCAC5 got 228140 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.52"
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits -region wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.AA8U6PZeNw (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits
WCS_IMAGE_NAME=wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits
WCS-calibrated image found: wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits
Checking if the catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits
WCS catalog name: wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=16182, passed=119048
Got 119048 stars (including 102742 good ones) from the SExtractor catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits.cat
util/solve_plate_with_UCAC5 got 119048 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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 957 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: 0.67"
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 957 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: 0.75"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits -region wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.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.rj1GQmBIDI (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits
WCS_IMAGE_NAME=wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits
WCS-calibrated image found: wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits
Checking if the catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits
WCS catalog name: wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=18764, passed=138438
Got 138438 stars (including 119523 good ones) from the SExtractor catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits.cat
util/solve_plate_with_UCAC5 got 138438 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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 958 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: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.63"
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 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.63"
Estimated accuracy of the plate solution: 0.71"
Excluding outliers - 955 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits -region wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Saving fully-calibrated image wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
Saving fully-calibrated image wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-02_20.00sec_-14.90C_LIGHT_0491.fits
Saving fully-calibrated image wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_072152_TTUQ2b1x1_21159_kXsNJBuj/wcs_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492.fits
Preparing the HTML report for the field Vul-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out232163.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254444.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254453.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254455.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254456.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254459.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254471.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254472.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254478.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254482.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254488.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254504.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254505.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254513.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254530.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254537.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254547.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254549.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254551.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254558.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254566.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254608.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out256424.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32774.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out146368.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out166249.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171147.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out240013.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254545.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254568.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254574.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254586.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254589.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65894.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 21s
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: 7s
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Considering the candidate 254444_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 254444_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:29:39.96 +24:11:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 4.272 2019835712493134208 292.41617949184 +24.18526109339 14.1257 13.0050 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.272#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254453_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 254453_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:22:11.77 +24:33:19.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)
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Considering the candidate 254455_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 254455_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:40:52.54 +19:51:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 4.037 1825668659159805952 295.22010068395 +19.85175785497 14.2225 13.4735 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.037#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254456_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 254456_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:11:17.76 +19:35:49.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)
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Considering the candidate 254459_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 254459_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:13:56.78 +25:40:03.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)
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Considering the candidate 254471_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 254471_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:14:39.03 +25:18:23.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)
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Considering the candidate 254472_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 254472_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:47:12.67 +20:27:30.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)
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Considering the candidate 254478_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 254478_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 18:59:35.67 +23:19:45.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 5.386 4533071903424422144 284.89787139731 +23.32803476183 13.2426 12.4096 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.386#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254481_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 254481_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 254482_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 254482_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:03:23.16 +23:32:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 5.880 4521436527786255488 285.84552475030 +23.54083898419 13.5786 12.7858 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.880#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254488_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 254488_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:15:33.61 +24:53:40.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)
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Considering the candidate 254489_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 254489_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:18:12.44 +22:49:32.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254503_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 254503_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 254504_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 254504_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:10:09.30 +25:59:36.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 5.594 2035874426004355968 287.53705761543 +25.99312680566 13.4354 12.6560 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.594#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254505_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 254505_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:13:56.80 +24:49:55.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)
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Considering the candidate 254513_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 254513_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 18:58:43.59 +26:02:43.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 3.558 4534812602129514752 284.68144749044 +26.04628092639 13.3243 12.5483 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.558#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254530_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 254530_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:09:10.72 +25:04:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 3.152 2035664728518462592 287.29563319777 +25.07654206962 13.6978 13.1099 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.152#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254537_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 254537_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:16:51.40 +23:35:01.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)
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Considering the candidate 254542_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 254542_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 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 254545_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
Preparing report for the candidate 254545_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
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Considering the candidate 254547_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 254547_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:15:36.28 +21:25:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 1.442 4519973215261002496 288.90141171669 +21.41861519230 13.9571 12.8350 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.442#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254549_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 254549_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:02:49.64 +24:43:25.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)
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Considering the candidate 254551_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 254551_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:41:43.02 +19:13:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 5.623 1824502180424589568 295.43084116756 +19.21967724103 13.2790 12.1890 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.623#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254553_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 254553_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:15:21.39 +24:57:53.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254555_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 254555_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:44:41.59 +21:18:14.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254558_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 254558_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 18:57:37.32 +23:40:11.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 4.881 4533330524868869504 284.40633817175 +23.67092300957 13.5331 12.9925 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.881#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254562_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 254562_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 254566_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 254566_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:40:30.77 +18:55:01.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 5.138 1824467094769714816 295.12789169646 +18.91839549065 12.0620 10.5533 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.138#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254568_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
Preparing report for the candidate 254568_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
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Considering the candidate 254574_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
Preparing report for the candidate 254574_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
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Considering the candidate 254578_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 254578_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:37:02.38 +24:45:09.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254586_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
Preparing report for the candidate 254586_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
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Considering the candidate 254589_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
Preparing report for the candidate 254589_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
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Considering the candidate 254599_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 254599_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 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 254606_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 254606_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:04:33.89 +25:57:34.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254608_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 254608_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:47:55.02 +21:14:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 2.091 1827376887910921728 296.97965082819 +21.24802761043 12.9523 12.4046 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.091#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254612_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 254612_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:42:30.36 +25:26:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254944_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 254944_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 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 255009_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 255009_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 18:54:38.19 +22:40:13.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255022_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 255022_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 255211_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 255211_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:36:25.50 +23:56:10.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255286_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 255286_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 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 255459_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 255459_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 255469_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 255469_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 255492_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 255492_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 255496_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 255496_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 255646_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 255646_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 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 255669_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 255669_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 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 255677_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 255677_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 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 255699_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 255699_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 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 255709_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 255709_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 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 255730_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 255730_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 255785_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 255785_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 255837_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 255837_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 255838_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 255838_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 255867_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 255867_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:21:02.96 +20:02:31.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255868_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 255868_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:24:20.56 +20:00:23.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255892_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 255892_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 255897_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 255897_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 255907_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 255907_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 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 255971_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 255971_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 255976_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 255976_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 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 255999_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 255999_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 256020_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 256020_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 256057_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 256057_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 256114_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 256114_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 256126_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 256126_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 256153_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 256153_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:40:16.40 +18:26:55.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256175_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 256175_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 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 256187_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 256187_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 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 256212_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 256212_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 256215_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 256215_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 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 256237_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 256237_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 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 256272_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 256272_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 256297_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 256297_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 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 256334_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 256334_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 256335_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 256335_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 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 256354_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 256354_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 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 256357_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 256357_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 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 256375_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 256375_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:44:52.09 +20:31:47.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256388_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 256388_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 256390_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 256390_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 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 256393_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 256393_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 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 256406_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 256406_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 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 256409_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 256409_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:44:31.22 +24:48:45.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256418_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 256418_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:43:37.16 +24:26:21.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256424_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 256424_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:21:43.23 +22:17:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.65, MAG_FAINT_SEARCH_LIMIT=15.63)GAIADR2_OUTPUT=# 0.553 2019133193256251904 290.43026725008 +22.28403205454 14.4146 13.5345 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.553#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 256426_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 256426_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 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 256427_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 256427_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 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 65894_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
Preparing report for the candidate 65894_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
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Considering the candidate 240013_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
Preparing report for the candidate 240013_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
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Considering the candidate 121912_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 121912_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:45:37.60 +22:51:13.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234184_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 234184_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 18:54:32.03 +19:02:00.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244768_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 244768_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:36:08.30 +25:45:09.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177832_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 177832_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:02:34.34 +25:50:26.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 253844_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 253844_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 63214_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 63214_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 188880_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 188880_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:00:59.62 +25:17:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30752_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 30752_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:05:00.93 +18:02:40.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234683_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 234683_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:49:47.05 +25:35:13.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 110128_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 110128_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 18:58:11.38 +21:52:54.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52335_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 52335_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:27:53.50 +19:17:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70828_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 70828_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 18:54:40.13 +19:48:41.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 146368_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
Preparing report for the candidate 146368_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
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Considering the candidate 171147_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
Preparing report for the candidate 171147_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
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Considering the candidate 232163_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 232163_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:39:31.98 +20:28:15.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)
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Considering the candidate 73036_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 73036_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 19:30:36.16 +20:15:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100687_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 100687_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 178679_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 178679_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 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 32774_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 32774_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks
**** FOUND 18:56:50.94 +18:01:54.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)
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Considering the candidate 140690_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492
The candidate 140690_fd_Vul-01-Q2b1x1_2026-03-27_05-35-46_20.00sec_-15.00C_LIGHT_0492 did not pass the final checks