This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87
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 29.1375* 04 26 50.57 +26 41 24.2 12.5 U Tau 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,2461128.6375,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260329.1375 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:26:50.57 +26:41:24.2 ;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_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20_00sec_-15_00C_LIGHT_0086_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20_00sec_-15_00C_LIGHT_0086_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20_00sec_-14_90C_LIGHT_0085_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 29.1375* 04 26 43.52 +31 17 19.3 13.6 U Per 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,2461128.6375,13.56,0.05,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 20260329.1375 13.56CV 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/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:26:43.52 +31:17:19.3 ;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_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20_00sec_-15_00C_LIGHT_0086_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20_00sec_-15_00C_LIGHT_0086_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20_00sec_-14_90C_LIGHT_0085_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 29.1375* 04 18 31.52 +28 16 57.6 13.6 U Tau 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
CZ Tau,2461128.6375,13.59,0.05,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
CZ Tau 20260329.1375 13.59CV 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/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:18:31.52 +28:16:57.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20_00sec_-15_00C_LIGHT_0086_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20_00sec_-15_00C_LIGHT_0086_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1375 2461128.6375 11.67 03:32:59.41 +27:49:07.4
161.35252 -22.75181 galactic Tau Second-epoch detections are separated by 1.0" and 1.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J053.2558+27.8162 | 03:32:59.38 +27:49:08.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G4 (LAMOST DR5) J-Ks=0.659+/-0.030 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1375* 03 32 59.41 +27 49 07.4 11.7 U Tau 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 J053.2558+27.8162,2461128.6375,11.67,0.05,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 J053.2558+27.8162 20260329.1375 11.67CV 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/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:32:59.41 +27:49:07.4 ;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_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20_00sec_-15_00C_LIGHT_0086_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20_00sec_-15_00C_LIGHT_0086_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 29.1375 2461128.6375 11.38 03:32:34.10 +28:00:57.7
161.14007 -22.65589 galactic Tau Second-epoch detections are separated by 1.2" and 1.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 119442735560772736 | 03:32:34.04 +28:00:58.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5) J-Ks=0.348+/-0.027 (G)
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 29.1375* 03 32 34.10 +28 00 57.7 11.4 U Tau 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
Gaia DR3 119442735560772736,2461128.6375,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 119442735560772736 20260329.1375 11.38CV 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/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:32:34.10 +28:00:57.7 ;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_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20_00sec_-15_00C_LIGHT_0086_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20_00sec_-15_00C_LIGHT_0086_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20_00sec_-14_90C_LIGHT_0085_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: 2461049.68555112 09.01.2026 04:27:01.617 /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
First image: 2461049.68555112 09.01.2026 04:27:01.617 /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
Last image: 2461128.63769699 29.03.2026 03:18:07.020 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.50
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: 4 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): 10936
Objects passed selection criteria: 10894
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 8087.5
Average stars matched: 7878.5 (97.4158 %)
Memory usage VmPeak: 117320 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Mar 28 22:21:50 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: 2461049.68555112 09.01.2026 04:27:01.617 /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
First image: 2461049.68555112 09.01.2026 04:27:01.617 /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
Last image: 2461128.63769699 29.03.2026 03:18:07.020 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 136
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.14
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: 17 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): 81612
Objects passed selection criteria: 81412
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 63298.2
Average stars matched: 61264.5 (96.787 %)
Memory usage VmPeak: 2257620 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Mar 28 22:23:09 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/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits
SExtractor catalog cache: saved Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat to cache
SExtractor catalog cache: saved Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.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/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461128.63721307
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits exists and is non-empty
Saving wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits to local_wcs_cache/
'wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits' -> 'local_wcs_cache/wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits'
wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits exists and is non-empty
Saving wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits to local_wcs_cache/
'wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits' -> 'local_wcs_cache/wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits'
wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits exists and is non-empty
Saving wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits to local_wcs_cache/
'wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits' -> 'local_wcs_cache/wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits'
wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits exists and is non-empty
Saving wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits to local_wcs_cache/
'wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits' -> 'local_wcs_cache/wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.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 03:59:59.648 +29:59:56.09
Second-epoch image center 03:59:53.259 +29:55:04.71
Angular distance between the image centers 0.08 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 03:59:59.648 +29:59:56.09
Second-epoch image center 03:59:52.908 +29:55:08.22
Angular distance between the image centers 0.08 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 03:59:53.259 +29:55:04.71
Second-epoch second image center 03:59:52.908 +29:55:08.22
Angular distance between the image centers 0.00160 deg.
###################################
ERROR: no shift applied between second-epoch images! The distance between image centers is 0.00160 deg. (min. required shift: 0.00164 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/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits &> /tmp/tmp.axiFwmESUA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits &> /tmp/tmp.PHzngUStWx
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits &> /tmp/tmp.6ckMLOj32X
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits &> /tmp/tmp.8phdxKlOgA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.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_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits and wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.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_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits and wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat
Found non-empty wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits and wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat
The reference image (wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits) and catalog (wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat) found
'wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.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 6059 out of 13390 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.958785
a=0.000000 b=1.000000 c=22.958785
From vast_summary.log: estimated ref. image limiting mag.: -7.50
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.46
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.46
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
2.0 pix Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
2.3 pix fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits
2.3 pix fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits
Limiting magnitude estimates:
15.5 mag. Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
15.5 mag. Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
14.2 mag. fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits
14.2 mag. fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 11.4 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.axiFwmESUA (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/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.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_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits' -> 'wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
WCS_IMAGE_NAME=wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
WCS-calibrated image found: wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
Checking if the catalog wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat corresponding to the image wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits alredy exist and is non-empty...
Catalog wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat corresponding to the image wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
WCS catalog name: wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1130, passed=13390
Got 13390 stars (including 12252 good ones) from the SExtractor catalog wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat
util/solve_plate_with_UCAC5 got 13390 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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: 0.33"
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 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.33"
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_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits -region wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.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.PHzngUStWx (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/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.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_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits' -> 'wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
WCS_IMAGE_NAME=wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
WCS-calibrated image found: wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
Checking if the catalog wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits.cat corresponding to the image wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits alredy exist and is non-empty...
Catalog wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits.cat corresponding to the image wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
WCS catalog name: wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1130, passed=13513
Got 13513 stars (including 12361 good ones) from the SExtractor catalog wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits.cat
util/solve_plate_with_UCAC5 got 13513 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 978 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: 0.37"
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 977 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: 0.35"
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_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits -region wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.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.6ckMLOj32X (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_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.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_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits
WCS_IMAGE_NAME=wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits
WCS-calibrated image found: wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits
Checking if the catalog wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits.cat corresponding to the image wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits.cat corresponding to the image wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits
WCS catalog name: wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=404, passed=5284
Got 5284 stars (including 4874 good ones) from the SExtractor catalog wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits.cat
util/solve_plate_with_UCAC5 got 5284 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 968 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: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
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 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.51"
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits -region wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.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.8phdxKlOgA (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_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.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_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits
WCS_IMAGE_NAME=wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits
WCS-calibrated image found: wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits
Checking if the catalog wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits.cat corresponding to the image wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits.cat corresponding to the image wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits
WCS catalog name: wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=407, passed=5246
Got 5246 stars (including 4835 good ones) from the SExtractor catalog wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits.cat
util/solve_plate_with_UCAC5 got 5246 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 968 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: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
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 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.51"
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits -region wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.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_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits'
Saving fully-calibrated image wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits'
Saving fully-calibrated image wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits'
Saving fully-calibrated image wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits'
Preparing the HTML report for the field Tau-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20799_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 20799_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 03:51:16.40 +33:02:04.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20805_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 20805_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 03:44:56.08 +30:22:24.2 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Tau-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits
SExtractor catalog cache: saved Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat to cache
SExtractor catalog cache: saved Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
Creating symlink local_wcs_cache/wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.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_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits exists and is non-empty
wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits exists and is non-empty
wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits exists and is non-empty
wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.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 03:59:59.648 +29:59:56.09
Second-epoch image center 03:59:53.259 +29:55:04.71
Angular distance between the image centers 0.08 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 03:59:59.648 +29:59:56.09
Second-epoch image center 03:59:52.908 +29:55:08.22
Angular distance between the image centers 0.08 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 03:59:53.259 +29:55:04.71
Second-epoch second image center 03:59:52.908 +29:55:08.22
Angular distance between the image centers 0.00160 deg.
###################################
ERROR: no shift applied between second-epoch images! The distance between image centers is 0.00160 deg. (min. required shift: 0.00164 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/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits &> /tmp/tmp.wJ2hkRfJtD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits &> /tmp/tmp.5Fv7zI8nGO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits &> /tmp/tmp.4OGbrl6b7l
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits &> /tmp/tmp.AfAGICSDY2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.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_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits and wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.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_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits and wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat
Found non-empty wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits and wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat
The reference image (wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits) and catalog (wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat) found
'wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.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 6106 out of 99190 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.803967
a=0.000000 b=1.000000 c=22.803967
From vast_summary.log: estimated ref. image limiting mag.: -7.14
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.66
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.66
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 66 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.8 pix Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
1.9 pix Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
2.1 pix fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits
2.1 pix fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits
Limiting magnitude estimates:
15.7 mag. Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
15.6 mag. Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
14.4 mag. fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits
14.4 mag. fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 13.9 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.wJ2hkRfJtD (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/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.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_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits' -> 'wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
WCS_IMAGE_NAME=wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
WCS-calibrated image found: wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
Checking if the catalog wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat corresponding to the image wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits alredy exist and is non-empty...
Catalog wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat corresponding to the image wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
WCS catalog name: wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=7855, passed=99168
Got 99168 stars (including 91148 good ones) from the SExtractor catalog wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat
util/solve_plate_with_UCAC5 got 99168 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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: 0.34"
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: 0.35"
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_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits -region wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.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.5Fv7zI8nGO (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/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.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_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits' -> 'wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
WCS_IMAGE_NAME=wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
WCS-calibrated image found: wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
Checking if the catalog wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits.cat corresponding to the image wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits alredy exist and is non-empty...
Catalog wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits.cat corresponding to the image wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
WCS catalog name: wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=25, blended=7957, passed=98800
Got 98800 stars (including 90693 good ones) from the SExtractor catalog wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits.cat
util/solve_plate_with_UCAC5 got 98800 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
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: 0.36"
Estimated accuracy of the plate solution: 0.36"
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_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits -region wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.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.4OGbrl6b7l (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_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.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_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits
WCS_IMAGE_NAME=wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits
WCS-calibrated image found: wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits
Checking if the catalog wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits.cat corresponding to the image wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits.cat corresponding to the image wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits
WCS catalog name: wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits.cat
SExtractor catalog parsing summary: zero_flux=3, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=1790, passed=40539
Got 40539 stars (including 38701 good ones) from the SExtractor catalog wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits.cat
util/solve_plate_with_UCAC5 got 40539 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
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 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.47"
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits -region wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.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.AfAGICSDY2 (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_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.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_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits
WCS_IMAGE_NAME=wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits
WCS-calibrated image found: wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits
Checking if the catalog wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits.cat corresponding to the image wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits.cat corresponding to the image wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits
WCS catalog name: wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1923, passed=40563
Got 40563 stars (including 38590 good ones) from the SExtractor catalog wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits.cat
util/solve_plate_with_UCAC5 got 40563 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 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: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.52"
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_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits -region wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.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_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.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_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
Saving fully-calibrated image wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.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_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
Saving fully-calibrated image wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.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_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-17-25_20.00sec_-14.90C_LIGHT_0085.fits
Saving fully-calibrated image wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.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_2026-03-28_CI_Tau-01-Q2b1x1_221934_TTUQ2b1x1_30071_4cLVee87/wcs_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086.fits
Preparing the HTML report for the field Tau-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out116819.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116823.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116829.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116833.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116834.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116890.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116893.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116895.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116907.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116941.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117011.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117032.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117104.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out95306.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out116911.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117039.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90201.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out92781.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out98116.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 15s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 116819_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 116819_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 04:05:28.96 +28:25:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 0.450 164117129950070400 061.37076286956 +28.41910249728 13.6882 13.0998 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.450#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116820_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 116820_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 04:04:36.29 +33:59:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116823_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 116823_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 04:13:29.18 +27:36:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.539 163128462836584064 063.37187223831 +27.60781474921 13.1660 12.5138 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.539#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116825_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 116825_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 03:36:19.69 +26:02:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116829_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 116829_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 03:32:57.48 +29:08:55.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)
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Considering the candidate 116831_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 116831_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 03:33:08.55 +26:36:10.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116832_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 116832_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 03:42:42.35 +26:53:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116833_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 116833_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 03:33:50.60 +26:55:21.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 0.229 69784972223854080 053.46076498792 +26.92250950391 12.3505 11.7880 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.229#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116834_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 116834_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 03:33:01.38 +27:48:59.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 1.142 119424662338509440 053.25589105510 +27.81623604575 12.0355 11.0044 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.142#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116865_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 116865_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 04:10:49.10 +33:34:36.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 116885_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 116885_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 03:40:07.65 +26:36:34.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116890_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 116890_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 03:32:42.06 +25:39:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 0.877 69372449204156928 053.17525799544 +25.66306198714 11.8748 11.0974 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.877#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116893_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 116893_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 03:33:33.37 +25:38:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 0.861 69369258044929280 053.38889619005 +25.64524448157 11.7711 10.9010 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.861#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116895_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 116895_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 03:32:44.35 +25:32:29.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)
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Considering the candidate 116907_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 116907_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 04:14:54.53 +30:50:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 0.802 165993721420195712 063.72724338382 +30.84316525977 12.7360 12.1898 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.802#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116910_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 116910_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 04:19:29.33 +30:51:26.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116911_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
Preparing report for the candidate 116911_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
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Considering the candidate 116928_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 116928_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 04:15:31.54 +33:49:29.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116941_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 116941_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 04:01:55.89 +31:58:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 0.830 170044322257873792 060.48273502732 +31.98036441537 12.7374 11.9442 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.830#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116957_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 116957_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 04:15:32.79 +33:50:12.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116967_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 116967_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 04:09:16.88 +26:50:45.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116969_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 116969_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 04:08:24.92 +32:27:45.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116971_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 116971_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 03:55:53.04 +32:10:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116981_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 116981_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 03:44:23.92 +32:11:00.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116982_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 116982_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 04:18:23.32 +33:51:36.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116983_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 116983_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 04:11:06.86 +33:36:15.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 116984_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 116984_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 03:44:35.45 +27:52:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116990_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 116990_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 04:13:29.75 +33:27:03.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116998_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 116998_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 04:07:46.83 +33:39:12.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117002_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 117002_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 117009_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 117009_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 04:00:12.47 +29:34:22.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117011_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 117011_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 04:01:00.30 +32:25:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 1.085 170139017696442240 060.25159555545 +32.42197978746 13.4260 12.8482 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.085#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117013_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 117013_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 04:07:46.09 +33:41:33.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117021_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 117021_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 04:11:38.80 +29:48:37.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117025_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 117025_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 04:11:45.33 +31:32:27.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117028_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 117028_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 117032_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 117032_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 04:02:58.55 +28:26:29.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 1.197 164175129188532352 060.74379765066 +28.44133784955 13.6065 12.8767 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.197#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117037_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 117037_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 117039_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
Preparing report for the candidate 117039_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
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Considering the candidate 117040_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 117040_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 04:21:11.52 +30:56:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117045_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 117045_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 03:45:19.74 +26:53:23.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117046_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 117046_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 04:13:17.99 +33:49:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117052_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 117052_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 04:21:46.61 +30:12:41.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117053_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 117053_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 03:50:54.39 +29:40:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117056_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 117056_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 03:44:11.41 +25:53:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117061_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 117061_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 03:48:32.43 +32:16:44.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117069_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 117069_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 04:13:21.40 +33:28:52.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117072_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 117072_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 03:57:11.57 +32:58:00.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117075_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 117075_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 03:41:35.62 +28:26:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117084_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 117084_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 04:12:18.82 +33:14:18.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117090_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 117090_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 04:09:46.95 +32:48:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117095_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 117095_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 03:59:00.84 +29:49:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117099_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 117099_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 03:51:05.93 +32:33:58.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117104_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 117104_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 04:02:26.88 +31:28:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 0.818 169262328972044032 060.61225431759 +31.47293192482 13.8735 13.1691 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.818#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117113_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 117113_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 04:02:30.89 +31:30:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117123_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 117123_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 03:50:54.52 +29:40:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 110127_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 110127_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 03:51:16.34 +33:02:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 112044_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 112044_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 03:39:03.25 +32:52:28.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 98116_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
Preparing report for the candidate 98116_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
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Considering the candidate 81784_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 81784_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 04:07:01.25 +28:53:02.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23744_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 23744_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 03:44:44.88 +33:15:13.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72300_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 72300_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 03:47:34.42 +26:16:54.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90201_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
Preparing report for the candidate 90201_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
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Considering the candidate 92781_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
Preparing report for the candidate 92781_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
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Considering the candidate 52535_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 52535_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks
**** FOUND 03:44:56.09 +30:22:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 95306_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086
The candidate 95306_fd_Tau-01-Q2b1x1_2026-03-28_22-18-07_20.00sec_-15.00C_LIGHT_0086 did not pass the final checks