The Frequency of Low-mass Exoplanets

Abstract

We report first results from the Anglo-Australian Telescope Rocky Planet Search - an intensive, high-precision Doppler planet search targeting low-mass exoplanets in contiguous 48 night observing blocks. On this run we targeted 24 bright, nearby and intrinsically stable Sun-like stars selected from the Anglo-Australian Planet Search's main sample. These observations have already detected one low-mass planet reported elsewhere (HD16417b), and here we reconfirm the detection of HD4308b. Further, we have Monte-Carlo simulated the data from this run on a star-by-star basis to produce robust detection constraints. These simulations demonstrate clear differences in the exoplanet detectability functions from star to star due to differences in sampling, data quality and intrinsic stellar stability. They reinforce the importance of star-by-star simulation when interpreting the data from Doppler planet searches. The simulations indicate that for some of our target stars we are sensitive to close-orbiting planets as small as a few Earth masses. The two low-mass planets present in our 24 star sample indicate that the exoplanet minimum mass function at low masses is likely to be a flat alpha ~ -1 (for dN/dM proportional to M^alpha) and that between 15+/-10% (at alpha=-0.3) and 48+/-34% (at alpha=-1.3) of stars host planets with orbital periods of less than 16 days and minimum masses greater than 3 Mearth.

11 figures, to appear in The Astrophysical Journal

References in corpus (12)

• The HARPS search for southern extra-solar planets XI. Super-Earths (5 & 8 M_Earth) in a 3-planet system
• Detection Limits from the McDonald Observatory Planet Search Program
• A Low-Mass Planet with a Possible Sub-Stellar-Mass Host in Microlensing Event MOA-2007-BLG-192
• The HARPS search for southern extra-solar planets. XIII. A planetary system with 3 Super-Earths (4.2, 6.9, & 9.2 Earth masses)
• On the Eccentricity Distribution of Exoplanets from Radial Velocity Surveys
• High eccentricity planets from the Anglo-Australian Planet Search
• An Activity Catalogue of Southern Stars
• The 2:1 resonant exoplanetary system orbiting HD73526
• Selection Functions in Doppler Planet Searches
• A Jupiter-like Planet Orbiting the Nearby M Dwarf GJ832
• Testing Disk Instability Models for Giant Planet Formation
• The Impact of Stellar Oscillations on Doppler Velocity Planet Searches

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