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The Intrinsic Multiplicity Distribution of Exoplanets Revealed from the Radial Velocity Method. II. Constraints on Giant Planet Multiplicity from Different Surveys

  • Authors: Jiayin Li, 佳音 李, Wei Zhu, 伟 祝

Jiayin Li et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 6.

Ratios of CLS to HARPS values for average number of planets per star (﹩{\bar{n}}_{{\rm{p}}}﹩), average multiplicity (﹩{\bar{m}}_{{\rm{p}}}﹩), and the fraction of stars with planets (Fp). The values are taken for the “all giant” population. Error bars indicate 1σ uncertainties. The dashed line at unity marks equal values between the two samples.

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