SIMBAD references

2012A&A...537A.147H - Astronomy and Astrophysics, volume 537A, 147-147 (2012/1-1)

Optimizing exoplanet transit searches around low-mass stars with inclination constraints.


Abstract (from CDS):

We investigate a method to increase the efficiency of a targeted exoplanet search with the transit technique by preselecting a subset of candidates from large catalogs of stars. Assuming spin-orbit alignment, this can be achieved by considering stars that have a higher probability to be oriented nearly equator-on (inclination close to 90°). We used activity-rotation velocity relations for low-mass stars with a convective envelope to study the dependence of the position in the activity-vsin i diagram on the stellar axis inclination. We composed a catalog of G-, K-, M-type main-sequence simulated stars using isochrones, an isotropic inclination distribution and empirical relations to obtain their rotation periods and activity indexes. Then the activity-vsin i diagram was completed and statistics were applied to trace the areas containing the higher ratio of stars with inclinations above 80°. A similar statistics was applied to stars from real catalogs with log(R'HK) and vsin i data to find their probability of being oriented equator-on. We present our method to generate the simulated star catalog and the subsequent statistics to find the highly inclined stars from real catalogs using the activity-vsin i diagram. Several catalogs from the literature are analyzed and a subsample of stars with the highest probability of being equator-on is presented. Assuming spin-orbit alignment, the efficiency of an exoplanet transit search in the resulting subsample of probably highly inclined stars is estimated to be two to three times higher than with a general search without preselection.

Abstract Copyright:

Journal keyword(s): stars: activity - planets and satellites: detection - stars: rotation

VizieR on-line data: <Available at CDS (J/A+A/537/A147): table4.dat>

Simbad objects: 1053

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