This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K
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
NSVS J1915544+225916,2461128.8506,12.79,0.05,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 J1915544+225916 20260329.3506 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:15:55.04 +22:59:10.1 ;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_2026-03-29_03-25-08_20_00sec_-15_00C_LIGHT_0312_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_2026-03-29_03-24-19_20_00sec_-15_00C_LIGHT_0311_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_2026-03-29_03-25-08_20_00sec_-15_00C_LIGHT_0312_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_2026-03-29_03-24-19_20_00sec_-15_00C_LIGHT_0311_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 J192721.70+245236.3,2461128.8506,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J192721.70+245236.3 20260329.3506 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:27:21.75 +24:52:37.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20_00sec_-15_00C_LIGHT_0312_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_2026-03-29_03-24-19_20_00sec_-15_00C_LIGHT_0311_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_2026-03-29_03-25-08_20_00sec_-15_00C_LIGHT_0312_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_2026-03-29_03-24-19_20_00sec_-15_00C_LIGHT_0311_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
V0474 Vul,2461128.8506,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0474 Vul 20260329.3506 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:41:51.01 +22:24:12.3 ;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_2026-03-29_03-25-08_20_00sec_-15_00C_LIGHT_0312_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_2026-03-29_03-24-19_20_00sec_-15_00C_LIGHT_0311_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_2026-03-29_03-25-08_20_00sec_-15_00C_LIGHT_0312_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_2026-03-29_03-24-19_20_00sec_-15_00C_LIGHT_0311_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 J193237.30+235100.4,2461128.8506,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J193237.30+235100.4 20260329.3506 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:32:37.35 +23:50:59.6 ;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_2026-03-29_03-25-08_20_00sec_-15_00C_LIGHT_0312_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_2026-03-29_03-24-19_20_00sec_-15_00C_LIGHT_0311_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_2026-03-29_03-25-08_20_00sec_-15_00C_LIGHT_0312_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_2026-03-29_03-24-19_20_00sec_-15_00C_LIGHT_0311_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 J1918392+211216,2461128.8506,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J1918392+211216 20260329.3506 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:18:39.29 +21:12:24.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20_00sec_-15_00C_LIGHT_0312_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_2026-03-29_03-24-19_20_00sec_-15_00C_LIGHT_0311_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_2026-03-29_03-25-08_20_00sec_-15_00C_LIGHT_0312_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_2026-03-29_03-24-19_20_00sec_-15_00C_LIGHT_0311_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.3506 2461128.8506 12.79 19:40:48.37 +18:25:30.1
54.89501 -2.08381 galactic Sge Second-epoch detections are separated by 0.3" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J295.2040+18.4313 | 19:40:48.46 +18:25:28.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=1.197+/-0.028 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J295.2040+18.4313,2461128.8506,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J295.2040+18.4313 20260329.3506 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:40:48.37 +18:25:30.1 ;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_2026-03-29_03-25-08_20_00sec_-15_00C_LIGHT_0312_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_2026-03-29_03-24-19_20_00sec_-15_00C_LIGHT_0311_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_2026-03-29_03-25-08_20_00sec_-15_00C_LIGHT_0312_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_2026-03-29_03-24-19_20_00sec_-15_00C_LIGHT_0311_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.3506 2461128.8506 11.84 19:42:35.13 +20:07:08.5
56.57586 -1.61091 galactic Vul Second-epoch detections are separated by 1.5" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J295.6549+20.1119 | 19:42:35.61 +20:07:04.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J295.6549+20.1119,2461128.8506,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J295.6549+20.1119 20260329.3506 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:42:35.13 +20:07:08.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20_00sec_-15_00C_LIGHT_0312_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_2026-03-29_03-24-19_20_00sec_-15_00C_LIGHT_0311_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_2026-03-29_03-25-08_20_00sec_-15_00C_LIGHT_0312_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_2026-03-29_03-24-19_20_00sec_-15_00C_LIGHT_0311_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 J1947128+205819,2461128.8506,11.50,0.05,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 J1947128+205819 20260329.3506 11.50CV 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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:47:12.22 +20:58:17.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20_00sec_-15_00C_LIGHT_0312_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_2026-03-29_03-24-19_20_00sec_-15_00C_LIGHT_0311_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_2026-03-29_03-25-08_20_00sec_-15_00C_LIGHT_0312_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_2026-03-29_03-24-19_20_00sec_-15_00C_LIGHT_0311_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 11223386,2461128.8506,12.11,0.05,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 11223386 20260329.3506 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:24:47.95 +21:28:17.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20_00sec_-15_00C_LIGHT_0312_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_2026-03-29_03-24-19_20_00sec_-15_00C_LIGHT_0311_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_2026-03-29_03-25-08_20_00sec_-15_00C_LIGHT_0312_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_2026-03-29_03-24-19_20_00sec_-15_00C_LIGHT_0311_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 J1928552+211114,2461128.8506,13.12,0.05,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 J1928552+211114 20260329.3506 13.12CV 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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:28:55.19 +21:11:15.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20_00sec_-15_00C_LIGHT_0312_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_2026-03-29_03-24-19_20_00sec_-15_00C_LIGHT_0311_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_2026-03-29_03-25-08_20_00sec_-15_00C_LIGHT_0312_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_2026-03-29_03-24-19_20_00sec_-15_00C_LIGHT_0311_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 J1929301+212217,2461128.8506,12.32,0.05,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 J1929301+212217 20260329.3506 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:29:30.17 +21:22:18.8 ;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_2026-03-29_03-25-08_20_00sec_-15_00C_LIGHT_0312_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_2026-03-29_03-24-19_20_00sec_-15_00C_LIGHT_0311_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_2026-03-29_03-25-08_20_00sec_-15_00C_LIGHT_0312_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_2026-03-29_03-24-19_20_00sec_-15_00C_LIGHT_0311_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 11233406,2461128.8506,12.53,0.05,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 11233406 20260329.3506 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:31:54.04 +20:40:23.6 ;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_2026-03-29_03-25-08_20_00sec_-15_00C_LIGHT_0312_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_2026-03-29_03-24-19_20_00sec_-15_00C_LIGHT_0311_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_2026-03-29_03-25-08_20_00sec_-15_00C_LIGHT_0312_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_2026-03-29_03-24-19_20_00sec_-15_00C_LIGHT_0311_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: 2461128.85090285 29.03.2026 08:25:08.006 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.87
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 17429
Objects passed selection criteria: 17360
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 13497.2
Average stars matched: 13154.5 (97.4606 %)
Memory usage VmPeak: 124056 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 Sun Mar 29 03:27:27 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: 2461128.85090285 29.03.2026 08:25:08.006 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 135
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: 45 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): 172093
Objects passed selection criteria: 171676
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 131536
Average stars matched: 125406 (95.3397 %)
Memory usage VmPeak: 2355924 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 Sun Mar 29 03:31:28 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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.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: 2461128.85034285
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_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_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits exists and is non-empty
Saving wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits to local_wcs_cache/
'wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits' -> 'local_wcs_cache/wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits'
wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits exists and is non-empty
Saving wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits to local_wcs_cache/
'wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits' -> 'local_wcs_cache/wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:23:05.554 +21:59:47.51
Second-epoch image center 19:22:59.002 +21:58:37.57
Angular distance between the image centers 0.03 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:23:05.554 +21:59:47.51
Second-epoch image center 19:22:57.902 +21:58:03.13
Angular distance between the image centers 0.04 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 19:22:59.002 +21:58:37.57
Second-epoch second image center 19:22:57.902 +21:58:03.13
Angular distance between the image centers 0.01047 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.JDBH6CvLX8
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.12kWu5X9d5
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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits &> /tmp/tmp.871FLp6h9L
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits &> /tmp/tmp.OUiSfkrwsk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.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 2 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
2.8 pix fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits
2.8 pix fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits
Limiting magnitude estimates:
15.0 mag. Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
15.0 mag. Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
14.0 mag. fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits
14.0 mag. fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 11.3 (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.JDBH6CvLX8 (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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/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.12kWu5X9d5 (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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/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.871FLp6h9L (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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits
WCS_IMAGE_NAME=wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits
WCS-calibrated image found: wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits
Checking if the catalog wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.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_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits
WCS catalog name: wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=611, passed=9782
Got 9782 stars (including 9162 good ones) from the SExtractor catalog wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits.cat
util/solve_plate_with_UCAC5 got 9782 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.1'
Seting catalog search parameters based on the expected field of view 939.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013043 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010434 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.77"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.78"
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 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.79"
Estimated accuracy of the plate solution: 0.90"
Excluding outliers - 950 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits -region wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.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.OUiSfkrwsk (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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits
WCS_IMAGE_NAME=wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits
WCS-calibrated image found: wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits
Checking if the catalog wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.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_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits
WCS catalog name: wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=637, passed=9935
Got 9935 stars (including 9286 good ones) from the SExtractor catalog wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits.cat
util/solve_plate_with_UCAC5 got 9935 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.76"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.78"
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 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.79"
Estimated accuracy of the plate solution: 0.91"
Excluding outliers - 950 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits -region wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/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_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits'
Saving fully-calibrated image wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits'
Preparing the HTML report for the field Vul-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 1s
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: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21588_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 21588_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:02:34.22 +25:50:26.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30071_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 30071_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:46:16.41 +20:22:01.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.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_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits
Creating symlink local_wcs_cache/wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.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_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits exists and is non-empty
wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:23:05.554 +21:59:47.51
Second-epoch image center 19:22:59.002 +21:58:37.57
Angular distance between the image centers 0.03 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:23:05.554 +21:59:47.51
Second-epoch image center 19:22:57.902 +21:58:03.13
Angular distance between the image centers 0.04 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 19:22:59.002 +21:58:37.57
Second-epoch second image center 19:22:57.902 +21:58:03.13
Angular distance between the image centers 0.01047 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.ooziX8UDta
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.4zcgecQBb8
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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits &> /tmp/tmp.qZqnBHADjz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits &> /tmp/tmp.gzSgcqq9cM
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.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 92 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
2.5 pix fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits
2.5 pix fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits
Limiting magnitude estimates:
15.2 mag. Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
15.2 mag. Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
14.0 mag. fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits
14.0 mag. fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 13.5 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.ooziX8UDta (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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/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.4zcgecQBb8 (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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/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.qZqnBHADjz (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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits
WCS_IMAGE_NAME=wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits
WCS-calibrated image found: wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits
Checking if the catalog wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.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_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits
WCS catalog name: wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=5660, passed=79964
Got 79964 stars (including 74190 good ones) from the SExtractor catalog wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits.cat
util/solve_plate_with_UCAC5 got 79964 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.1'
Seting catalog search parameters based on the expected field of view 939.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013043 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010434 (37.6 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 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.72"
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 953 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: 0.77"
Excluding outliers - 948 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits -region wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.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.gzSgcqq9cM (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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits
WCS_IMAGE_NAME=wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits
WCS-calibrated image found: wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits
Checking if the catalog wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.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_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits
WCS catalog name: wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=5786, passed=80525
Got 80525 stars (including 74630 good ones) from the SExtractor catalog wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits.cat
util/solve_plate_with_UCAC5 got 80525 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.75"
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 955 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: 0.78"
Excluding outliers - 951 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits -region wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/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_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-24-19_20.00sec_-15.00C_LIGHT_0311.fits
Saving fully-calibrated image wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.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_2026-03-29_CI_Vul-01-Q2b1x1_032547_TTUQ2b1x1_14844_8QaSj88K/wcs_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312.fits
Preparing the HTML report for the field Vul-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out254461.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254464.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254479.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254480.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254481.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254482.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254487.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254506.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254508.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254569.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254852.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254875.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255177.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255181.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255292.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255298.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255357.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255418.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255426.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255447.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255540.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255616.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255620.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out255644.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out26083.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out113146.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out143051.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out165991.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254502.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33243.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80490.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out86251.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90334.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out92079.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out93934.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out96543.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 15s
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: 5s
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Considering the candidate 254453_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 254453_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:47:02.21 +20:14:47.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254461_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 254461_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:30:45.78 +22:51:11.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 5.155 2019415870832831488 292.68959647225 +22.85404259336 13.2050 12.2101 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.155#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254464_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 254464_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:13:16.64 +22:48:21.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 1.364 4520456313180147200 288.31906283140 +22.80622959126 12.8884 11.8153 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.364#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 254473_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 254473_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:08:56.61 +26:07:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254479_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 254479_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:30:12.54 +25:03:33.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)
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Considering the candidate 254480_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 254480_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:49:01.18 +23:38:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 2.345 1828306761172067840 297.25562320768 +23.63592706207 12.0920 10.7620 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.345#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254481_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 254481_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:49:05.41 +20:49:23.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)
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Considering the candidate 254482_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 254482_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:47:57.59 +26:00:08.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)
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Considering the candidate 254487_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 254487_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:40:22.85 +19:16:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 5.457 1824511423195004800 295.09595169120 +19.27028796753 12.7696 12.2043 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.457#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254493_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 254493_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:00:25.11 +25:26:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254496_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 254496_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:46:51.93 +22:02:51.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254502_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
Preparing report for the candidate 254502_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
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Considering the candidate 254504_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 254504_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 254505_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 254505_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:47:24.26 +20:19:35.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254506_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 254506_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:48:41.34 +23:43:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 2.794 1828311159218560640 297.17307649662 +23.71902243683 11.8539 10.8031 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.794#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254508_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 254508_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 18:56:05.80 +23:50:12.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)
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Considering the candidate 254510_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 254510_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:11:34.50 +25:01:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254512_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 254512_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:40:20.50 +20:28:49.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 254513_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 254513_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 18:53:10.12 +25:40:09.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254569_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 254569_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:28:53.42 +24:38:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.50, MAG_FAINT_SEARCH_LIMIT=11.48)GAIADR2_OUTPUT=# 1.548 2022870020968531328 292.22213670957 +24.64730831981 10.8698 10.5753 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.548#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254850_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 254850_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:07:57.57 +21:42:41.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 254852_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 254852_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:04:45.19 +23:18:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 0.991 4521391099897471488 286.18799330265 +23.30491369056 12.0672 11.1926 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.991#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254874_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 254874_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 18:54:38.17 +22:40:13.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254875_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 254875_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:04:53.24 +23:19:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 1.254 4521391035490811136 286.22201262986 +23.32311236510 12.1870 11.3486 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.254#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255089_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 255089_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:01:01.26 +19:17:49.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 255177_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 255177_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 18:54:29.04 +20:20:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 1.203 4518902595853157632 283.62079691478 +20.33825317077 13.2964 12.6490 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.203#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255181_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 255181_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:07:57.06 +19:52:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 2.959 4519379032300778240 286.98841036699 +19.86751076991 12.5970 11.6350 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.959#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255182_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 255182_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:25:27.11 +20:15:14.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 255196_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 255196_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:48:51.22 +21:32:15.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255207_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 255207_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:36:25.43 +23:56:03.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255292_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 255292_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:08:11.75 +25:22:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 0.869 2035688058780778496 287.04872864381 +25.38045669058 13.1665 12.5523 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.869#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255297_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 255297_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:21:03.11 +20:02:32.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255298_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 255298_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:09:08.73 +25:19:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 3.324 2035677407261658752 287.28617668161 +25.32837786360 12.8938 12.1006 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.324#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255331_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 255331_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:25:28.82 +24:56:32.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 255347_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 255347_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:03:21.20 +23:38:48.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255357_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 255357_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:27:20.80 +20:41:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 3.721 2017928128506843136 291.83655457397 +20.68622269753 12.9883 12.1344 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.721#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255381_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 255381_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:16:13.40 +21:21:52.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 255418_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 255418_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:19:57.88 +26:01:26.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)
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Considering the candidate 255426_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 255426_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:08:46.22 +24:10:50.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 1.222 4521541806022375936 287.19283145768 +24.18083633045 13.1518 12.2689 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.222#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255435_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 255435_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:17:43.68 +25:49:45.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255447_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 255447_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:35:56.72 +23:52:18.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 3.369 2021021054747350784 293.98682167845 +23.87262793090 12.8519 11.8935 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.369#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255462_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 255462_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:01:57.39 +19:09:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255468_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 255468_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:04:34.50 +22:06:41.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255529_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 255529_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:24:20.77 +20:00:25.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255538_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 255538_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:06:20.26 +20:40:15.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255540_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 255540_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:18:13.37 +24:26:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 3.556 2022675884108225664 289.55553141507 +24.43802999241 13.2267 12.3010 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.556#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255545_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 255545_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:18:23.68 +26:09:31.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255571_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 255571_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 18:58:34.55 +22:23:44.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255600_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 255600_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:37:55.88 +18:36:47.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255609_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 255609_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:36:27.94 +21:59:07.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255612_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 255612_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:06:23.70 +21:24:20.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 255616_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 255616_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:06:20.19 +21:22:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 3.455 4519869311409308160 286.58309563825 +21.37712017689 13.3630 12.6599 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.455#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255620_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 255620_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:20:56.39 +23:03:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 1.646 2022281404285182208 290.23467647722 +23.05017886544 13.4064 12.7510 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.646#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 255644_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 255644_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 18:56:47.03 +26:06:26.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 0.259 4534986943437030912 284.19603832758 +26.10721893763 13.3369 12.5549 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.259#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 174572_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 174572_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:25:20.42 +26:12:29.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 147973_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 147973_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:20:12.11 +24:00:43.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 140690_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 140690_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:39:20.34 +23:44:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 165991_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
Preparing report for the candidate 165991_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
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Considering the candidate 121912_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 121912_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:45:37.46 +22:51:12.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234337_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 234337_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:46:16.38 +20:22:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234683_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 234683_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:49:47.13 +25:35:14.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113146_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
Preparing report for the candidate 113146_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
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Considering the candidate 143051_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
Preparing report for the candidate 143051_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
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Considering the candidate 94148_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 94148_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:38:24.37 +21:23:13.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177832_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 177832_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:02:34.26 +25:50:26.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 136123_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 136123_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:10:13.63 +23:20:39.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 150311_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 150311_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:43:58.64 +24:09:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78573_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 78573_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:48:15.16 +20:36:07.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92079_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
Preparing report for the candidate 92079_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
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Considering the candidate 154477_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 154477_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:30:08.09 +24:22:53.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30752_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 30752_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:05:00.97 +18:02:40.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52335_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 52335_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:27:53.60 +19:17:38.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71341_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 71341_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:43:04.66 +20:14:34.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101939_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 101939_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:47:17.40 +21:50:02.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 112797_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 112797_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:35:41.33 +22:20:06.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 110128_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 110128_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 18:58:11.55 +21:52:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 233042_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 233042_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:42:44.56 +21:15:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33243_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
Preparing report for the candidate 33243_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
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Considering the candidate 74440_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 74440_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:48:26.03 +20:23:48.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 68990_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
Preparing report for the candidate 68990_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
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Considering the candidate 86251_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
Preparing report for the candidate 86251_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
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Considering the candidate 84895_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 84895_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:35:01.37 +20:55:53.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 182417_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 182417_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:28:47.22 +25:53:04.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 135961_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 135961_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:31:10.35 +23:30:33.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 69096_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 69096_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:48:33.80 +20:08:08.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96543_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
Preparing report for the candidate 96543_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
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Considering the candidate 90334_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
Preparing report for the candidate 90334_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
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Considering the candidate 93934_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
Preparing report for the candidate 93934_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
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Considering the candidate 26083_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 26083_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:33:23.93 +18:01:02.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.86, MAG_FAINT_SEARCH_LIMIT=11.84)
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Considering the candidate 80490_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
Preparing report for the candidate 80490_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
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Considering the candidate 96854_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 96854_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks
**** FOUND 19:48:41.72 +21:33:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 120276_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312
The candidate 120276_fd_Vul-01-Q2b1x1_2026-03-29_03-25-08_20.00sec_-15.00C_LIGHT_0312 did not pass the final checks