Exoplanet Tracker Observations of Sirius-Like Systems

Details Exoplanet Tracker Observations of Sirius-Like Systems Exoplanet Tracker Observations of Sirius-Like Systems

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006noao.prop..157h&link_type=abstract

NOAO Proposal ID #2006B-0157

Computer Science

Scientific paper

We propose Exoplanet Tracker (ET) observations of a selected sample of Sirius-like systems containing luminous primaries (primarily F to K) and hot white dwarfs. The white dwarfs have been long evident from EUV and UV observations from space, but critical knowledge of system parameters have either been limited or lacking altogether. Our proposed ET radial velocity observations should be able to fill in the missing information and to significantly improve the precision of prior data. This improved velocity data is critical for several future space-based programs that will allow the study of the white dwarf components of these systems.

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