Science parametrics for missions to search for Earth-like exoplanets by direct imaging

RA Brown�- The Astrophysical Journal, 2015 - iopscience.iop.org
We use N t, the number of exoplanets observed in time t, as a science metric to study direct-
search missions like Terrestrial Planet Finder. In our model, N has 27 parameters, divided�…

Science Parametrics for Missions to Search for Earthlike Exoplanets by Direct Imaging

RA Brown�- arXiv preprint arXiv:1402.2612, 2014 - arxiv.org
We use $ N_ {t} $, the number of exoplanets observed in time $ t $, as a science metric to
study direct-search missions like Terrestrial Planet Finder. In our model, $ N $ has 27�…

Science Parametrics for Missions to Search for Earth-like Exoplanets by Direct Imaging

RA Brown�- The Astrophysical Journal, 2015 - ui.adsabs.harvard.edu
We use N t, the number of exoplanets observed in time t, as a science metric to study direct-
search missions like Terrestrial Planet Finder. In our model, N has 27 parameters, divided�…

SCIENCE PARAMETRICS FOR MISSIONS TO SEARCH FOR EARTH-LIKE EXOPLANETS BY DIRECT IMAGING

RA Brown�- Astrophysical Journal, 2015 - inis.iaea.org
[en] We use N t, the number of exoplanets observed in time t, as a science metric to study
direct-search missions like Terrestrial Planet Finder. In our model, N has 27 parameters�…