J/ApJ/727/102: Resource Record Summary

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On the frequency of Jupiter analogs

Short name: J/ApJ/727/102 IVOA Identifier: ivo://CDS.VizieR/J/ApJ/727/102 DOI (Digital Object Identifier): 10.26093/cds/vizier.17270102 Publisher: CDS[+]ivo://CDS[Pub. ID] More Info: https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/727/102 VO Compliance: Level 2: This is a VO-compliant resource.	Status: active Registered: 2012 Oct 10 11:59:37Z
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Description

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