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Table · dataset · 2012

On the frequency of Jupiter analogs

Listed in IVOA Registry (Virtual Observatory)

The Anglo-Australian Planet Search has now accumulated 12 years of radial-velocity data with long-term instrumental precision better than 3m/s.

Description

In this paper, we expand on earlier simulation work, to probe the frequency of near-circular, long-period gas-giant planets residing at orbital distances of 3-6AU -the so-called Jupiter analogs. We present the first comprehensive analysis of the frequency of these objects based on radial-velocity data.

We find that 3.3% of stars in our sample host Jupiter analogs; detailed, star-by-star simulations show that no more than 37% of stars host a giant planet between 3 and 6AU.

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Documentation and papers

Catalogue records · 2

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Provenance · 1 source records, 9 field assertions
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IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/apj/727/10214 d agoJSON v1
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concepts[method].local:method:simulationenrichment · IVOA Registrykeyword-concept-rules@1.0.0title+description (75%)
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