Masses of Extrasolar Planets
P.Butler, G.Marcy, D.Fischer, S.Vogt
20 Sept 2003

Our group has found 75 planets in our Doppler survey of 1,300 FGKM stars, using the Lick, Keck, and AAT telescopes. The mass distribution from this survey is particularly valuable because our detectability of planets is uniform with all three telescopes (3 m/s precision). So, the mass distribution of planets seen in this plot has just one detection threshold, that associated with the highest precision of 3 m/s.
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