This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4
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 19.4047* 13 44 15.13 -07 50 18.8 11.5 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,2461118.9047,11.49,0.05,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 20260319.4047 11.49CV 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-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 13:44:15.13 -07:50:18.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20_00sec_-14_90C_LIGHT_0471_fits__*pix.png resample_wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20_00sec_-15_00C_LIGHT_0161_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20_00sec_-14_90C_LIGHT_0471_fits__*pix.png resample_wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20_00sec_-15_00C_LIGHT_0160_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20_00sec_-14_90C_LIGHT_0471_fits__*pix.png resample_wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20_00sec_-15_00C_LIGHT_0161_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20_00sec_-14_90C_LIGHT_0471_fits__*pix.png resample_wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20_00sec_-15_00C_LIGHT_0160_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 19.4047* 13 52 46.39 -09 47 00.4 12.9 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,2461118.9047,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260319.4047 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 13:52:46.39 -09:47:00.4 ;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-12-Q2b1x1_2026-02-11_03-59-41_20_00sec_-14_90C_LIGHT_0471_fits__*pix.png resample_wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20_00sec_-15_00C_LIGHT_0161_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20_00sec_-14_90C_LIGHT_0471_fits__*pix.png resample_wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20_00sec_-15_00C_LIGHT_0160_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20_00sec_-14_90C_LIGHT_0471_fits__*pix.png resample_wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20_00sec_-15_00C_LIGHT_0161_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20_00sec_-14_90C_LIGHT_0471_fits__*pix.png resample_wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20_00sec_-15_00C_LIGHT_0160_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.4047 2461118.9047 14.21 13:49:46.70 -12:34:30.7
324.41529 47.84816 galactic Vir Second-epoch detections are separated by 1.8" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J207.4350-12.5684 | 13:49:46.70 -12:34:30.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 19.4047* 13 49 46.70 -12 34 30.7 14.2 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
ATO J207.4350-12.5684,2461118.9047,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J207.4350-12.5684 20260319.4047 14.21CV 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-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 13:49:46.70 -12:34:30.7 ;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-12-Q2b1x1_2026-02-11_03-59-41_20_00sec_-14_90C_LIGHT_0471_fits__*pix.png resample_wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20_00sec_-15_00C_LIGHT_0161_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20_00sec_-14_90C_LIGHT_0471_fits__*pix.png resample_wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20_00sec_-15_00C_LIGHT_0160_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20_00sec_-14_90C_LIGHT_0471_fits__*pix.png resample_wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20_00sec_-15_00C_LIGHT_0161_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20_00sec_-14_90C_LIGHT_0471_fits__*pix.png resample_wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20_00sec_-15_00C_LIGHT_0160_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 19.4047* 14 10 21.05 -13 18 12.2 11.7 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
Z Vir,2461118.9047,11.69,0.05,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
Z Vir 20260319.4047 11.69CV 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-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:10:21.05 -13:18:12.2 ;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-12-Q2b1x1_2026-02-11_03-59-41_20_00sec_-14_90C_LIGHT_0471_fits__*pix.png resample_wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20_00sec_-15_00C_LIGHT_0161_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20_00sec_-14_90C_LIGHT_0471_fits__*pix.png resample_wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20_00sec_-15_00C_LIGHT_0160_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20_00sec_-14_90C_LIGHT_0471_fits__*pix.png resample_wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20_00sec_-15_00C_LIGHT_0161_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20_00sec_-14_90C_LIGHT_0471_fits__*pix.png resample_wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20_00sec_-15_00C_LIGHT_0160_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 19.4047* 13 21 35.30 -11 29 13.4 12.6 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
NSVS 16038743,2461118.9047,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 16038743 20260319.4047 12.62CV 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-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 13:21:35.30 -11:29:13.4 ;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-12-Q2b1x1_2026-02-11_03-59-41_20_00sec_-14_90C_LIGHT_0471_fits__*pix.png resample_wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20_00sec_-15_00C_LIGHT_0161_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20_00sec_-14_90C_LIGHT_0471_fits__*pix.png resample_wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20_00sec_-15_00C_LIGHT_0160_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20_00sec_-14_90C_LIGHT_0471_fits__*pix.png resample_wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20_00sec_-15_00C_LIGHT_0161_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20_00sec_-14_90C_LIGHT_0471_fits__*pix.png resample_wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20_00sec_-15_00C_LIGHT_0160_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 19.4047* 13 33 38.11 -11 08 00.3 12.3 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,2461118.9047,12.35,0.05,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 20260319.4047 12.35CV 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-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 13:33:38.11 -11:08:00.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20_00sec_-14_90C_LIGHT_0471_fits__*pix.png resample_wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20_00sec_-15_00C_LIGHT_0161_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20_00sec_-14_90C_LIGHT_0471_fits__*pix.png resample_wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20_00sec_-15_00C_LIGHT_0160_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20_00sec_-14_90C_LIGHT_0471_fits__*pix.png resample_wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20_00sec_-15_00C_LIGHT_0161_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20_00sec_-14_90C_LIGHT_0471_fits__*pix.png resample_wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20_00sec_-15_00C_LIGHT_0160_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: 2461082.91657089 11.02.2026 09:59:41.725 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits
First image: 2461082.91657089 11.02.2026 09:59:41.725 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits
Last image: 2461118.90501868 19.03.2026 09:43:03.614 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 16
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.87
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 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): 6395
Objects passed selection criteria: 6386
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 6014.5
Average stars matched: 5712 (94.9705 %)
Memory usage VmPeak: 112376 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 04:54:12 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: 2461082.91657089 11.02.2026 09:59:41.725 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits
First image: 2461082.91657089 11.02.2026 09:59:41.725 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits
Last image: 2461118.90501868 19.03.2026 09:43:03.614 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 123
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.59
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: 12 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): 39411
Objects passed selection criteria: 39311
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 37963.5
Average stars matched: 36109.2 (95.1157 %)
Memory usage VmPeak: 139728 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 04:54:59 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-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits
SExtractor catalog cache: saved Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits.cat to cache
SExtractor catalog cache: saved Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.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-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.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: 2461118.90447049
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-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits exists and is non-empty
Saving wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits to local_wcs_cache/
'wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits' -> 'local_wcs_cache/wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits'
wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits exists and is non-empty
Saving wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits to local_wcs_cache/
'wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits' -> 'local_wcs_cache/wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits'
wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits exists and is non-empty
Saving wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits to local_wcs_cache/
'wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits' -> 'local_wcs_cache/wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits'
wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits exists and is non-empty
Saving wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits to local_wcs_cache/
'wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits' -> 'local_wcs_cache/wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.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 13:42:39.454 -09:59:06.40
Second-epoch image center 13:42:52.332 -10:00:08.39
Angular distance between the image centers 0.06 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 13:42:39.454 -09:59:06.40
Second-epoch image center 13:42:54.697 -10:00:07.46
Angular distance between the image centers 0.06 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 13:42:52.332 -10:00:08.39
Second-epoch second image center 13:42:54.697 -10:00:07.46
Angular distance between the image centers 0.00971 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-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits &> /tmp/tmp.joBl73D7CO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits &> /tmp/tmp.wu9hKDvJyg
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits &> /tmp/tmp.95OMYfJNhr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits &> /tmp/tmp.Il797U5IwV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.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-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits and wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.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-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits and wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits.cat
Found non-empty wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits and wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits.cat
The reference image (wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits) and catalog (wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits.cat) found
'wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.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 3630 out of 5781 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.883428
a=0.000000 b=1.000000 c=22.883428
From vast_summary.log: estimated ref. image limiting mag.: -7.87
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.01
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.01
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 16 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits
2.1 pix Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits
2.3 pix fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits
2.3 pix fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits
Limiting magnitude estimates:
15.0 mag. Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits
15.0 mag. Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits
15.0 mag. fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits
15.0 mag. fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.0 (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 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.joBl73D7CO (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-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.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_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.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-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.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-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits' -> 'wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits
WCS_IMAGE_NAME=wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits
WCS-calibrated image found: wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits
Checking if the catalog wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits.cat corresponding to the image wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits alredy exist and is non-empty...
Catalog wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits.cat corresponding to the image wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits
WCS catalog name: wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=460, passed=5781
Got 5781 stars (including 5313 good ones) from the SExtractor catalog wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits.cat
util/solve_plate_with_UCAC5 got 5781 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
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: 0.32"
Estimated accuracy of the plate solution: 0.31"
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-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits -region wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.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.wu9hKDvJyg (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-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.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_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.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-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.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-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits' -> 'wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits
WCS_IMAGE_NAME=wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits
WCS-calibrated image found: wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits
Checking if the catalog wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits.cat corresponding to the image wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits alredy exist and is non-empty...
Catalog wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits.cat corresponding to the image wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits
WCS catalog name: wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=490, passed=5748
Got 5748 stars (including 5246 good ones) from the SExtractor catalog wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits.cat
util/solve_plate_with_UCAC5 got 5748 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
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: 0.35"
Estimated accuracy of the plate solution: 0.34"
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-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits -region wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.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.95OMYfJNhr (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_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.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_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits
WCS_IMAGE_NAME=wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits
WCS-calibrated image found: wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits
Checking if the catalog wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits.cat corresponding to the image wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits.cat corresponding to the image wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits
WCS catalog name: wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=449, passed=6364
Got 6364 stars (including 5909 good ones) from the SExtractor catalog wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits.cat
util/solve_plate_with_UCAC5 got 6364 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 974 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: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
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 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.45"
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits -region wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.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.Il797U5IwV (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_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.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_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits
WCS_IMAGE_NAME=wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits
WCS-calibrated image found: wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits
Checking if the catalog wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits.cat corresponding to the image wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits.cat corresponding to the image wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits
WCS catalog name: wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=444, passed=6351
Got 6351 stars (including 5902 good ones) from the SExtractor catalog wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits.cat
util/solve_plate_with_UCAC5 got 6351 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 974 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: 0.44"
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 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.45"
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits -region wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.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-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits'
Saving fully-calibrated image wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits'
Saving fully-calibrated image wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits'
Saving fully-calibrated image wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits'
Preparing the HTML report for the field Vir-12-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20325.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20339.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20340.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20341.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20348.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20317.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 20317_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
Preparing report for the candidate 20317_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20325_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 20325_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 14:10:21.09 -13:18:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.66, MAG_FAINT_SEARCH_LIMIT=12.64)GAIADR2_OUTPUT=# 5.041 6303159386450566272 212.58912774315 -13.30413339455 11.1195 9.6973 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.041#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20338_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 20338_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 13:40:20.89 -11:04:39.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20339_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 20339_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 13:22:24.81 -07:32:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 1.548 3631318501429508992 200.60378483222 -07.54339091570 12.1657 11.6558 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.548#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20340_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 20340_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 13:17:24.21 -13:37:21.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 0.814 3609176433189982080 199.35108401701 -13.62271046863 11.9629 11.4644 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.814#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20341_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 20341_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 13:22:22.31 -13:47:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.00, MAG_FAINT_SEARCH_LIMIT=12.98)GAIADR2_OUTPUT=# 0.874 3608463846576397440 200.59303801462 -13.79948007988 11.8721 11.2536 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.874#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20342_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 20342_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 13:33:34.16 -09:50:41.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20343_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 20343_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 13:28:58.95 -10:23:01.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20344_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 20344_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 13:30:49.00 -10:13:29.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20345_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 20345_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 13:36:57.81 -12:16:40.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20346_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 20346_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 13:37:07.71 -10:47:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20347_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 20347_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 13:33:00.41 -11:17:35.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20348_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 20348_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 13:33:57.62 -10:48:29.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 0.780 3611520488901400448 203.49020283978 -10.80848750471 12.0363 11.6572 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.780#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20349_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 20349_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 13:50:48.67 -07:49:41.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20350_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 20350_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 13:28:26.52 -12:18:15.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20351_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 20351_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 13:35:18.35 -10:43:51.2 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 5s
Prepared the HTML report for the field Vir-12-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 ####
13:44:15.13 -07:50:18.8
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits
SExtractor catalog cache: saved Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits.cat to cache
SExtractor catalog cache: saved Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.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-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits
Creating symlink local_wcs_cache/wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.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-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits exists and is non-empty
wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits exists and is non-empty
wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits exists and is non-empty
wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.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 13:42:39.454 -09:59:06.40
Second-epoch image center 13:42:52.332 -10:00:08.39
Angular distance between the image centers 0.06 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 13:42:39.454 -09:59:06.40
Second-epoch image center 13:42:54.697 -10:00:07.46
Angular distance between the image centers 0.06 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 13:42:52.332 -10:00:08.39
Second-epoch second image center 13:42:54.697 -10:00:07.46
Angular distance between the image centers 0.00971 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-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits &> /tmp/tmp.llW3MjmQWi
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits &> /tmp/tmp.xOjSYx2aPm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits &> /tmp/tmp.hhIdY8zpqb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits &> /tmp/tmp.uRGFNC6JX5
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.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-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits and wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.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-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits and wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits.cat
Found non-empty wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits and wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits.cat
The reference image (wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits) and catalog (wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits.cat) found
'wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.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 3804 out of 37853 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.745847
a=0.000000 b=1.000000 c=22.745847
From vast_summary.log: estimated ref. image limiting mag.: -7.59
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.16
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.16
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 37 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits
1.9 pix Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits
2.1 pix fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits
2.1 pix fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits
Limiting magnitude estimates:
15.2 mag. Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits
15.2 mag. Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits
15.2 mag. fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits
15.2 mag. fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 14.5 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.llW3MjmQWi (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-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.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_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.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-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.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-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits' -> 'wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits
WCS_IMAGE_NAME=wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits
WCS-calibrated image found: wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits
Checking if the catalog wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits.cat corresponding to the image wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits alredy exist and is non-empty...
Catalog wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits.cat corresponding to the image wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits
WCS catalog name: wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=26, blended=1525, passed=37827
Got 37827 stars (including 36237 good ones) from the SExtractor catalog wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits.cat
util/solve_plate_with_UCAC5 got 37827 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 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: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
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: 0.34"
Estimated accuracy of the plate solution: 0.33"
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_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits -region wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.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.xOjSYx2aPm (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-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.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_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.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-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.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-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits' -> 'wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits
WCS_IMAGE_NAME=wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits
WCS-calibrated image found: wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits
Checking if the catalog wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits.cat corresponding to the image wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits alredy exist and is non-empty...
Catalog wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits.cat corresponding to the image wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits
WCS catalog name: wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=1500, passed=38104
Got 38104 stars (including 36531 good ones) from the SExtractor catalog wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits.cat
util/solve_plate_with_UCAC5 got 38104 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 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: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
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: 0.37"
Estimated accuracy of the plate solution: 0.37"
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_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits -region wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.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.hhIdY8zpqb (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_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.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_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits
WCS_IMAGE_NAME=wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits
WCS-calibrated image found: wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits
Checking if the catalog wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits.cat corresponding to the image wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits.cat corresponding to the image wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits
WCS catalog name: wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=1612, passed=38709
Got 38709 stars (including 37046 good ones) from the SExtractor catalog wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits.cat
util/solve_plate_with_UCAC5 got 38709 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 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
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 977 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: 0.43"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits -region wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.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.uRGFNC6JX5 (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_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.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_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits
WCS_IMAGE_NAME=wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits
WCS-calibrated image found: wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits
Checking if the catalog wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits.cat corresponding to the image wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits.cat corresponding to the image wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits
WCS catalog name: wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1637, passed=38469
Got 38469 stars (including 36772 good ones) from the SExtractor catalog wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits.cat
util/solve_plate_with_UCAC5 got 38469 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: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
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: 0.45"
Estimated accuracy of the plate solution: 0.44"
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-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits -region wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.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-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.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_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/wcs_Vir-12-Q2b1x1_2026-02-11_03-59-41_20.00sec_-14.90C_LIGHT_0471.fits
Saving fully-calibrated image wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.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_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/wcs_Vir-12-Q2b1x1_2026-02-11_04-00-22_20.00sec_-15.00C_LIGHT_0472.fits
Saving fully-calibrated image wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.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_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-42-16_20.00sec_-15.00C_LIGHT_0160.fits
Saving fully-calibrated image wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.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_2026-03-19_CI_Vir-12-Q2b1x1_045150_TTUQ2b1x1_2536_DgNaEwv4/wcs_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161.fits
Preparing the HTML report for the field Vir-12-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out53255.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53257.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53258.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53263.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53267.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53269.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53530.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53534.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53614.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53624.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53634.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53650.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53656.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53670.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53686.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53695.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53705.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53707.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53716.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53719.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53763.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53772.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53776.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53786.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53822.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53868.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53918.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out53509.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out53659.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out06627.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13401.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14942.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53379.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53646.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 13s
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: 3s
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Considering the candidate 53255_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 53255_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 13:13:22.26 -06:33:51.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 3.186 3628693387354156544 198.34186669398 -06.56433736882 13.9890 13.4721 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.186#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53257_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 53257_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 14:12:06.38 -11:33:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 2.425 6304191449912137984 213.02616547101 -11.55231254138 13.7009 12.6282 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.425#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53258_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 53258_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 13:15:35.56 -05:03:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.41, MAG_FAINT_SEARCH_LIMIT=15.39)GAIADR2_OUTPUT=# 1.596 3635692981455761920 198.89782170650 -05.06335890593 13.6912 13.2109 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.596#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53263_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 53263_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 13:47:58.17 -14:45:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.25, MAG_FAINT_SEARCH_LIMIT=15.23)GAIADR2_OUTPUT=# 2.283 3605812859617803648 206.99231377233 -14.75424247679 14.4386 13.8279 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.283#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53267_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 53267_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 13:39:57.68 -07:35:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 1.204 3618605093291340672 204.99040884498 -07.59254819902 13.7251 13.0813 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.204#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53269_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 53269_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 13:48:01.26 -07:53:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 1.354 3619809676999040256 207.00518084526 -07.89445328959 13.9462 13.4608 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.354#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53295_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 53295_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 13:44:15.13 -07:50:18.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53379_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
Preparing report for the candidate 53379_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
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Considering the candidate 53509_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 53509_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 13:11:30.58 -13:00:46.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)
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Considering the candidate 53513_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 53513_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 13:15:52.87 -12:22:10.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53530_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 53530_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 13:19:17.00 -14:45:14.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 2.275 3607925330692532352 199.82096028015 -14.75461987237 13.8887 13.3468 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.275#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53534_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 53534_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 13:25:15.12 -09:49:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.08, MAG_FAINT_SEARCH_LIMIT=15.06)GAIADR2_OUTPUT=# 1.784 3623830453582887424 201.31315979196 -09.82821984358 14.1651 13.7088 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.784#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53597_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 53597_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 13:31:56.91 -11:01:13.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53614_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 53614_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 13:28:00.79 -13:33:29.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.35, MAG_FAINT_SEARCH_LIMIT=15.33)GAIADR2_OUTPUT=# 0.457 3609928984475633792 202.00317585684 -13.55816328606 14.5694 13.9905 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.457#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53624_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 53624_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 14:07:54.12 -11:28:06.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)
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Considering the candidate 53634_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 53634_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 14:09:08.45 -14:09:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 1.628 6301541863111758720 212.28558107721 -14.15163303461 14.1546 13.4423 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.628#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53646_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
Preparing report for the candidate 53646_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
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Considering the candidate 53650_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 53650_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 14:02:57.39 -12:42:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 1.882 6302727450179364992 210.73965405520 -12.70341668241 14.4375 13.9490 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.882#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53656_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 53656_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 13:47:41.67 -05:09:28.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 1.461 3632831261926219904 206.92374763255 -05.15747419840 14.6445 14.1181 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.461#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53659_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 53659_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 14:12:07.68 -10:04:42.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)
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Considering the candidate 53670_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 53670_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 14:10:53.16 -08:50:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.35, MAG_FAINT_SEARCH_LIMIT=15.33)GAIADR2_OUTPUT=# 1.014 3615189048102912896 212.72159051665 -08.83920517605 14.8670 14.2117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.014#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53686_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 53686_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 13:38:31.07 -13:34:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 5.466 3607116399371988864 204.63005183880 -13.56823771542 14.3906 13.8384 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.466#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53695_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 53695_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 13:17:27.15 -14:45:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.41, MAG_FAINT_SEARCH_LIMIT=15.39)GAIADR2_OUTPUT=# 2.618 3608685265025930752 199.36376780987 -14.76076607589 14.5181 13.9830 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.618#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53705_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 53705_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 14:02:38.69 -06:18:26.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 3.478 3643540024144509568 210.66173680835 -06.30817178565 14.6166 14.1856 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.478#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53707_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 53707_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 14:11:58.00 -12:37:32.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)
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Considering the candidate 53716_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 53716_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 13:42:18.13 -08:19:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 0.589 3618312417039927552 205.57568319806 -08.31860968232 14.5112 13.8767 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.589#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53719_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 53719_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 13:38:48.25 -10:53:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 0.887 3616702732016964736 204.70090131002 -10.89093482363 14.5954 14.0912 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.887#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53763_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 53763_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 14:10:43.33 -09:42:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 3.511 3614919667754048000 212.68134334803 -09.71404383685 14.4903 13.9533 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.511#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53772_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 53772_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 13:58:36.64 -08:49:17.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 2.335 3615795600564097024 209.65316366384 -08.82195156953 14.6215 13.9938 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.335#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53776_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 53776_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 14:13:58.62 -11:02:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 0.880 6304606240673575936 213.49449870849 -11.04334442590 14.4420 13.8217 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.880#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53786_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 53786_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 14:09:09.21 -05:35:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 0.740 3644003021619048960 212.28856563631 -05.59369018997 14.5967 13.9908 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.740#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53822_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 53822_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 14:11:21.23 -13:00:51.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 0.373 6303193608750042112 212.83837557800 -13.01431496849 14.4028 13.7752 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.373#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53868_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 53868_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks
**** FOUND 14:07:47.28 -09:40:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 1.323 3615026320381942656 211.94669211165 -09.66870740029 14.4005 13.6100 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.323#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53918_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161
The candidate 53918_fd_Vir-12-Q2b1x1_2026-03-19_04-43-03_20.00sec_-15.00C_LIGHT_0161 did not pass the final checks