This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ
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!
TCP 2026 03 25.3894* 12 01 21.13 -10 14 42.9 12.8 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461124.8894,12.75,0.05,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
VARIABLE_NAME 20260325.3894 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/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:01:21.13 -10:14:42.9 ;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_Vir-10-Q2b1x1_2026-02-27_02-17-10_20_00sec_-15_00C_LIGHT_0379_fits__*pix.png resample_wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20_00sec_-15_00C_LIGHT_0090_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20_00sec_-15_00C_LIGHT_0379_fits__*pix.png resample_wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20_00sec_-14_90C_LIGHT_0089_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20_00sec_-15_00C_LIGHT_0379_fits__*pix.png resample_wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20_00sec_-15_00C_LIGHT_0379_fits__*pix.png resample_wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461124.8894,12.89,0.05,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
VARIABLE_NAME 20260325.3894 12.89CV 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/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:53:22.96 -12:31:41.4 ;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_Vir-10-Q2b1x1_2026-02-27_02-17-10_20_00sec_-15_00C_LIGHT_0379_fits__*pix.png resample_wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20_00sec_-15_00C_LIGHT_0090_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20_00sec_-15_00C_LIGHT_0379_fits__*pix.png resample_wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20_00sec_-14_90C_LIGHT_0089_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20_00sec_-15_00C_LIGHT_0379_fits__*pix.png resample_wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20_00sec_-15_00C_LIGHT_0379_fits__*pix.png resample_wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 25.3894* 12 09 06.67 -06 29 13.2 13.4 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461124.8894,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260325.3894 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:09:06.67 -06:29:13.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20_00sec_-15_00C_LIGHT_0379_fits__*pix.png resample_wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20_00sec_-15_00C_LIGHT_0090_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20_00sec_-15_00C_LIGHT_0379_fits__*pix.png resample_wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20_00sec_-14_90C_LIGHT_0089_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20_00sec_-15_00C_LIGHT_0379_fits__*pix.png resample_wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20_00sec_-15_00C_LIGHT_0379_fits__*pix.png resample_wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461124.8894,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260325.3894 13.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:48:32.30 -10:23:50.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20_00sec_-15_00C_LIGHT_0379_fits__*pix.png resample_wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20_00sec_-15_00C_LIGHT_0090_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20_00sec_-15_00C_LIGHT_0379_fits__*pix.png resample_wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20_00sec_-14_90C_LIGHT_0089_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20_00sec_-15_00C_LIGHT_0379_fits__*pix.png resample_wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20_00sec_-15_00C_LIGHT_0379_fits__*pix.png resample_wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.3894 2461124.8894 13.91 12:12:41.10 -14:00:50.7
288.86485 47.79639 galactic Crv Second-epoch detections are separated by 2.0" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 3570830385351817856 | 12:12:41.10 -14:00:50.7 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 3570830385351817856,2461124.8894,13.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 3570830385351817856 20260325.3894 13.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:12:41.10 -14:00:50.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20_00sec_-15_00C_LIGHT_0379_fits__*pix.png resample_wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20_00sec_-15_00C_LIGHT_0090_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20_00sec_-15_00C_LIGHT_0379_fits__*pix.png resample_wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20_00sec_-14_90C_LIGHT_0089_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20_00sec_-15_00C_LIGHT_0379_fits__*pix.png resample_wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20_00sec_-15_00C_LIGHT_0379_fits__*pix.png resample_wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461124.8894,14.10,0.05,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
VARIABLE_NAME 20260325.3894 14.10CV 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/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:56:15.89 -08:14:39.0 ;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_Vir-10-Q2b1x1_2026-02-27_02-17-10_20_00sec_-15_00C_LIGHT_0379_fits__*pix.png resample_wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20_00sec_-15_00C_LIGHT_0090_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20_00sec_-15_00C_LIGHT_0379_fits__*pix.png resample_wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20_00sec_-14_90C_LIGHT_0089_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20_00sec_-15_00C_LIGHT_0379_fits__*pix.png resample_wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20_00sec_-15_00C_LIGHT_0379_fits__*pix.png resample_wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20_00sec_-14_90C_LIGHT_0089_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.8894,14.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.3894 14.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:51:30.07 -11:25:25.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20_00sec_-15_00C_LIGHT_0379_fits__*pix.png resample_wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20_00sec_-15_00C_LIGHT_0090_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20_00sec_-15_00C_LIGHT_0379_fits__*pix.png resample_wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20_00sec_-14_90C_LIGHT_0089_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20_00sec_-15_00C_LIGHT_0379_fits__*pix.png resample_wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20_00sec_-15_00C_LIGHT_0090_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20_00sec_-15_00C_LIGHT_0379_fits__*pix.png resample_wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20_00sec_-14_90C_LIGHT_0089_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: 2461098.84537233 27.02.2026 08:17:10.169 /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
First image: 2461098.84537233 27.02.2026 08:17:10.169 /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
Last image: 2461124.88966747 25.03.2026 09:20:57.269 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.07
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: 2 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): 5159
Objects passed selection criteria: 5153
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 4259.25
Average stars matched: 3774.5 (88.6189 %)
Memory usage VmPeak: 111228 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 Wed Mar 25 04:26:24 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: 2461098.84537233 27.02.2026 08:17:10.169 /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
First image: 2461098.84537233 27.02.2026 08:17:10.169 /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
Last image: 2461124.88966747 25.03.2026 09:20:57.269 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 57
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.79
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 9 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 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): 30450
Objects passed selection criteria: 30377
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 26140.2
Average stars matched: 23791.5 (91.0148 %)
Memory usage VmPeak: 131248 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 Wed Mar 25 04:27:03 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/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits
SExtractor catalog cache: saved Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat to cache
SExtractor catalog cache: saved Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.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/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.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: 2461124.88907590
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_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits exists and is non-empty
Saving wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits to local_wcs_cache/
'wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits' -> 'local_wcs_cache/wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits'
wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits exists and is non-empty
Saving wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits to local_wcs_cache/
'wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits' -> 'local_wcs_cache/wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits'
wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits exists and is non-empty
Saving wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits to local_wcs_cache/
'wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits' -> 'local_wcs_cache/wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits'
wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits exists and is non-empty
Saving wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits to local_wcs_cache/
'wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits' -> 'local_wcs_cache/wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.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 11:59:59.182 -10:00:01.72
Second-epoch image center 12:00:00.357 -10:00:22.58
Angular distance between the image centers 0.01 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:59:59.182 -10:00:01.72
Second-epoch image center 11:59:59.380 -09:59:44.72
Angular distance between the image centers 0.00 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 12:00:00.357 -10:00:22.58
Second-epoch second image center 11:59:59.380 -09:59:44.72
Angular distance between the image centers 0.01125 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/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits &> /tmp/tmp.4R3I8Td4ZE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits &> /tmp/tmp.11y8Ugz8Jk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits &> /tmp/tmp.LukprwySeR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits &> /tmp/tmp.DewCdUu5Xm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.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_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits and wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.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_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits and wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat
Found non-empty wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits and wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat
The reference image (wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits) and catalog (wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat) found
'wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.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 3305 out of 4517 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.854368
a=0.000000 b=1.000000 c=22.854368
From vast_summary.log: estimated ref. image limiting mag.: -8.07
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.78
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.78
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
2.0 pix Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
2.3 pix fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits
2.4 pix fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits
Limiting magnitude estimates:
14.8 mag. Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
14.8 mag. Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
14.9 mag. fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits
14.9 mag. fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 11.8 (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.4R3I8Td4ZE (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/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.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_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits' -> 'wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
WCS_IMAGE_NAME=wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
WCS-calibrated image found: wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
Checking if the catalog wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat corresponding to the image wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits alredy exist and is non-empty...
Catalog wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat corresponding to the image wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
WCS catalog name: wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=373, passed=4517
Got 4517 stars (including 4137 good ones) from the SExtractor catalog wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat
util/solve_plate_with_UCAC5 got 4517 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 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: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
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 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits -region wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.11y8Ugz8Jk (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/Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.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_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits' -> 'wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
WCS_IMAGE_NAME=wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
WCS-calibrated image found: wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
Checking if the catalog wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits.cat corresponding to the image wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits alredy exist and is non-empty...
Catalog wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits.cat corresponding to the image wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
WCS catalog name: wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=364, passed=4553
Got 4553 stars (including 4187 good ones) from the SExtractor catalog wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits.cat
util/solve_plate_with_UCAC5 got 4553 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 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: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
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 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits -region wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.LukprwySeR (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_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.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_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits
WCS_IMAGE_NAME=wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits
WCS-calibrated image found: wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits
Checking if the catalog wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits.cat corresponding to the image wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits.cat corresponding to the image wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits
WCS catalog name: wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=293, passed=5587
Got 5587 stars (including 5293 good ones) from the SExtractor catalog wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits.cat
util/solve_plate_with_UCAC5 got 5587 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 975 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: 0.43"
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 975 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: 0.46"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits -region wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.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.DewCdUu5Xm (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_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.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_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits
WCS_IMAGE_NAME=wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits
WCS-calibrated image found: wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits
Checking if the catalog wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits.cat corresponding to the image wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits.cat corresponding to the image wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits
WCS catalog name: wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=292, passed=5605
Got 5605 stars (including 5310 good ones) from the SExtractor catalog wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits.cat
util/solve_plate_with_UCAC5 got 5605 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 976 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: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
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 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits -region wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.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_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits'
Saving fully-calibrated image wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits'
Saving fully-calibrated image wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits'
Saving fully-calibrated image wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits'
Preparing the HTML report for the field Vir-10-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20676.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20681.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20692.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20711.dat to exclusion_list_gaiadr2.txt
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: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20676_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 20676_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 11:53:50.79 -09:18:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 0.515 3588123263714519296 178.46169900628 -09.30109537792 11.6642 11.2210 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.515#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20681_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 20681_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 12:16:40.60 -10:03:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 0.537 3581035262006906880 184.16926884383 -10.06080447431 11.6975 11.2387 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.537#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20692_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 20692_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 12:02:04.99 -10:32:18.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 0.485 3575560999771173888 180.52066935788 -10.53835568947 11.3122 10.4529 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.485#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20711_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 20711_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 11:57:37.66 -08:48:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.83, MAG_FAINT_SEARCH_LIMIT=12.81)GAIADR2_OUTPUT=# 0.875 3594157967645466496 179.40695627310 -08.81362866359 11.7142 11.2962 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.875#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Vir-10-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/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits
SExtractor catalog cache: saved Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat to cache
SExtractor catalog cache: saved Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
Creating symlink local_wcs_cache/wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.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_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits exists and is non-empty
wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits exists and is non-empty
wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits exists and is non-empty
wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.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 11:59:59.182 -10:00:01.72
Second-epoch image center 12:00:00.357 -10:00:22.58
Angular distance between the image centers 0.01 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:59:59.182 -10:00:01.72
Second-epoch image center 11:59:59.380 -09:59:44.72
Angular distance between the image centers 0.00 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 12:00:00.357 -10:00:22.58
Second-epoch second image center 11:59:59.380 -09:59:44.72
Angular distance between the image centers 0.01125 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/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits &> /tmp/tmp.AaGrYvdEMN
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits &> /tmp/tmp.2HbjvbIZKv
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits &> /tmp/tmp.CYCXz9HqV7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits &> /tmp/tmp.yhp5OGx83r
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.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_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits and wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.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_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits and wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat
Found non-empty wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits and wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat
The reference image (wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits) and catalog (wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat) found
'wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.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 3765 out of 29056 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.705276
a=0.000000 b=1.000000 c=22.705276
From vast_summary.log: estimated ref. image limiting mag.: -7.79
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.92
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.92
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 39 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
1.9 pix Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
2.2 pix fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits
2.3 pix fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits
Limiting magnitude estimates:
14.9 mag. Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
14.9 mag. Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
15.0 mag. fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits
15.0 mag. fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.3 (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.AaGrYvdEMN (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/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.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_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits' -> 'wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
WCS_IMAGE_NAME=wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
WCS-calibrated image found: wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
Checking if the catalog wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat corresponding to the image wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits alredy exist and is non-empty...
Catalog wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat corresponding to the image wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
WCS catalog name: wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1008, passed=29048
Got 29048 stars (including 27997 good ones) from the SExtractor catalog wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat
util/solve_plate_with_UCAC5 got 29048 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 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: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
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 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits -region wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.2HbjvbIZKv (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/Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.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_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits' -> 'wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
WCS_IMAGE_NAME=wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
WCS-calibrated image found: wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
Checking if the catalog wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits.cat corresponding to the image wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits alredy exist and is non-empty...
Catalog wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits.cat corresponding to the image wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
WCS catalog name: wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=1003, passed=28852
Got 28852 stars (including 27808 good ones) from the SExtractor catalog wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits.cat
util/solve_plate_with_UCAC5 got 28852 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 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: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
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 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits -region wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.CYCXz9HqV7 (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_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.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_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits
WCS_IMAGE_NAME=wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits
WCS-calibrated image found: wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits
Checking if the catalog wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits.cat corresponding to the image wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits.cat corresponding to the image wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits
WCS catalog name: wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1196, passed=30404
Got 30404 stars (including 29166 good ones) from the SExtractor catalog wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits.cat
util/solve_plate_with_UCAC5 got 30404 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 975 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: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
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 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.43"
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits -region wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.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.yhp5OGx83r (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_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.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_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits
WCS_IMAGE_NAME=wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits
WCS-calibrated image found: wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits
Checking if the catalog wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits.cat corresponding to the image wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits.cat corresponding to the image wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits
WCS catalog name: wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1157, passed=30084
Got 30084 stars (including 28890 good ones) from the SExtractor catalog wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits.cat
util/solve_plate_with_UCAC5 got 30084 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 975 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: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
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 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits -region wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.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_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.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_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/wcs_Vir-10-Q2b1x1_2026-02-27_02-17-10_20.00sec_-15.00C_LIGHT_0379.fits
Saving fully-calibrated image wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.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_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/wcs_Vir-10-Q2b1x1_2026-02-27_02-17-55_20.00sec_-15.00C_LIGHT_0380.fits
Saving fully-calibrated image wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.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_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-06_20.00sec_-14.90C_LIGHT_0089.fits
Saving fully-calibrated image wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.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_2026-03-25_CI_Vir-10-Q2b1x1_042231_TTUQ2b1x1_18522_pKN2yzTQ/wcs_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090.fits
Preparing the HTML report for the field Vir-10-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out31834.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31835.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out34548.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out34629.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out34723.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out34751.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out34766.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out34786.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out34806.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out35011.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out35031.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out35052.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out35065.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out35068.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out35095.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out35106.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out35108.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out35114.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out35137.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out35142.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out35180.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out35194.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out35206.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out35217.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out35221.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out35239.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out35270.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out35348.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out35392.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out35453.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out35504.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out35537.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out32897.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33029.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33425.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34369.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34389.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34841.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34846.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
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: 4s
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Considering the candidate 31834_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 31834_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 11:51:33.14 -06:17:55.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 0.849 3598525571427670144 177.88797566142 -06.29907126229 14.1249 13.4644 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.849#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31835_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 31835_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 12:21:34.53 -10:02:06.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 1.852 3578069157592125184 185.39366836598 -10.03547249626 14.0153 13.4537 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.852#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32897_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
Preparing report for the candidate 32897_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
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Considering the candidate 33029_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
Preparing report for the candidate 33029_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
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Considering the candidate 33425_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
Preparing report for the candidate 33425_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
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Considering the candidate 34369_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
Preparing report for the candidate 34369_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
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Considering the candidate 34389_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
Preparing report for the candidate 34389_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
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Considering the candidate 34548_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 34548_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 12:23:48.64 -06:26:19.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 2.422 3584369015622118784 185.95200390872 -06.43877700881 14.4721 13.9736 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.422#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 34629_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 34629_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 12:22:23.52 -09:58:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 1.579 3578082553594497664 185.59772965256 -09.98273745963 13.7180 12.6317 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.579#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 34723_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 34723_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 12:14:22.14 -13:00:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 2.195 3571051112311035008 183.59178273655 -13.00481655861 14.2723 13.6851 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.195#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 34751_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 34751_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 11:59:12.10 -13:18:58.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 3.003 3573933104087479936 179.80054501099 -13.31713017938 14.3297 13.6270 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.003#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 34766_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 34766_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 12:03:01.04 -10:58:11.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 1.395 3575465685856968320 180.75403488971 -10.97011473716 14.2860 13.7944 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.395#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 34786_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 34786_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 12:23:30.02 -11:48:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 1.432 3576805818731846656 185.87494543531 -11.81490209379 14.0919 13.5827 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.432#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 34806_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 34806_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 11:41:56.75 -11:06:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 1.750 3585979319121419776 175.48609781822 -11.10666671094 14.0724 13.2047 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.750#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 34841_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
Preparing report for the candidate 34841_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
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Considering the candidate 34846_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
Preparing report for the candidate 34846_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
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Considering the candidate 35011_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 35011_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 12:17:22.82 -08:39:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 2.110 3581466682881844352 184.34453385567 -08.65777545669 14.6450 14.1423 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.110#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 35031_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 35031_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 12:11:54.65 -13:49:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 2.049 3570851241712975872 182.97824910267 -13.82363631111 14.4747 13.9356 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.049#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 35052_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 35052_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 11:40:26.92 -12:31:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 0.931 3585711553680560000 175.11227741038 -12.52931817041 14.2747 13.7829 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.931#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 35065_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 35065_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 12:23:56.26 -06:24:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 0.644 3584370561810347008 185.98458786717 -06.41516611558 14.5752 13.9962 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.644#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 35068_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 35068_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 12:19:16.54 -06:59:28.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.57, MAG_FAINT_SEARCH_LIMIT=15.55)GAIADR2_OUTPUT=# 0.864 3583992054932386816 184.81889478353 -06.99143337245 14.5504 13.8938 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.864#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 35095_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 35095_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 12:22:20.16 -06:42:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)GAIADR2_OUTPUT=# 2.355 3584334209207112576 185.58366070458 -06.70744969645 14.3161 13.6378 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.355#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 35106_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 35106_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 12:23:23.18 -09:37:42.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 0.906 3579608542590506624 185.84634238885 -09.62825055588 14.2258 13.6278 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.906#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 35108_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 35108_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 12:23:45.14 -07:42:48.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 1.648 3583098495576489344 185.93795671107 -07.71396803499 14.4952 13.9924 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.648#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 35114_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 35114_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 12:14:21.32 -12:53:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.56, MAG_FAINT_SEARCH_LIMIT=15.54)GAIADR2_OUTPUT=# 1.526 3571053002096604928 183.58843928466 -12.89956793597 14.5222 13.9425 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.526#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 35137_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 35137_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 12:19:37.45 -07:33:08.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.51, MAG_FAINT_SEARCH_LIMIT=15.49)GAIADR2_OUTPUT=# 1.655 3583888013644616960 184.90558377413 -07.55240543851 14.2686 13.4499 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.655#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 35142_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 35142_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 12:18:16.17 -09:41:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.53, MAG_FAINT_SEARCH_LIMIT=15.51)GAIADR2_OUTPUT=# 1.183 3581142876707388288 184.56731322027 -09.68601730372 14.5508 14.0375 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.183#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 35180_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 35180_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 12:15:12.07 -12:43:15.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 1.926 3577062348538472960 183.79988784923 -12.72133410990 14.5043 14.0033 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.926#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 35194_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 35194_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 12:08:18.01 -10:00:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.52, MAG_FAINT_SEARCH_LIMIT=15.50)GAIADR2_OUTPUT=# 0.897 3581635286118590208 182.07517692668 -10.00682173116 14.6874 14.1434 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.897#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 35206_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 35206_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 12:22:08.35 -11:14:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.57, MAG_FAINT_SEARCH_LIMIT=15.55)GAIADR2_OUTPUT=# 0.684 3577658558718737280 185.53466473954 -11.24661564259 14.6496 14.0407 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.684#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 35217_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 35217_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 12:16:37.69 -05:48:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.56, MAG_FAINT_SEARCH_LIMIT=15.54)GAIADR2_OUTPUT=# 1.207 3596693441458493056 184.15697973553 -05.80124630661 15.1004 14.4893 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.207#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 35221_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 35221_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 12:13:33.09 -11:37:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 0.985 3577396222116114688 183.38767813446 -11.62747172914 14.3654 13.7558 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.985#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 35239_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 35239_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 12:12:22.04 -11:03:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 0.737 3580480146073757952 183.09165734996 -11.06544335362 14.4115 13.8267 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.737#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 35270_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 35270_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 12:06:03.21 -14:11:45.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.54, MAG_FAINT_SEARCH_LIMIT=15.52)GAIADR2_OUTPUT=# 1.282 3570664256016796416 181.51301987376 -14.19611862012 14.5576 14.0518 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.282#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 35348_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 35348_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 11:48:53.54 -10:50:43.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 0.898 3587257467028836480 177.22311279612 -10.84552551335 14.4644 13.8536 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.898#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 35392_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 35392_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 11:38:50.44 -13:41:34.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 0.914 3584933546124226944 174.70990563044 -13.69295897702 14.3824 13.8723 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.914#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 35453_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 35453_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 11:39:43.22 -11:44:31.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 1.272 3585836245170982400 174.93008989690 -11.74251991673 14.3920 13.9043 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.272#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 35504_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 35504_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks
**** FOUND 11:49:43.15 -12:16:05.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)
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Considering the candidate 35537_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090
The candidate 35537_fd_Vir-10-Q2b1x1_2026-03-25_04-20-57_20.00sec_-15.00C_LIGHT_0090 did not pass the final checks