The Astronomical Journal (Jan 2023)

The TESS-Keck Survey. XVI. Mass Measurements for 12 Planets in Eight Systems

  • Joseph M. Akana Murphy,
  • Natalie M. Batalha,
  • Nicholas Scarsdale,
  • Howard Isaacson,
  • David R. Ciardi,
  • Erica J. Gonzales,
  • Steven Giacalone,
  • Joseph D. Twicken,
  • Anne Dattilo,
  • Tara Fetherolf,
  • Ryan A. Rubenzahl,
  • Ian J. M. Crossfield,
  • Courtney D. Dressing,
  • Benjamin Fulton,
  • Andrew W. Howard,
  • Daniel Huber,
  • Stephen R. Kane,
  • Erik A. Petigura,
  • Paul Robertson,
  • Arpita Roy,
  • Lauren M. Weiss,
  • Corey Beard,
  • Ashley Chontos,
  • Fei Dai,
  • Malena Rice,
  • Judah Van Zandt,
  • Jack Lubin,
  • Sarah Blunt,
  • Alex S. Polanski,
  • Aida Behmard,
  • Paul A. Dalba,
  • Michelle L. Hill,
  • Lee J. Rosenthal,
  • Casey L. Brinkman,
  • Andrew W. Mayo,
  • Emma V. Turtelboom,
  • Isabel Angelo,
  • Teo Močnik,
  • Mason G. MacDougall,
  • Daria Pidhorodetska,
  • Dakotah Tyler,
  • Molly R. Kosiarek,
  • Rae Holcomb,
  • Emma M. Louden,
  • Lea A. Hirsch,
  • Emily A. Gilbert,
  • Jay Anderson,
  • Jeff A. Valenti

DOI
https://doi.org/10.3847/1538-3881/ace2ca
Journal volume & issue
Vol. 166, no. 4
p. 153

Abstract

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With JWST’s successful deployment and unexpectedly high fuel reserves, measuring the masses of sub-Neptunes transiting bright, nearby stars will soon become the bottleneck for characterizing the atmospheres of small exoplanets via transmission spectroscopy. Using a carefully curated target list and observations from more than 2 yr of APF-Levy and Keck-HIRES Doppler monitoring, the TESS-Keck Survey is working toward alleviating this pressure. Here we present mass measurements for 11 transiting planets in eight systems that are particularly suited to atmospheric follow-up with JWST. We also report the discovery and confirmation of a temperate super-Jovian-mass planet on a moderately eccentric orbit. The sample of eight host stars, which includes one subgiant, spans early-K to late-F spectral types ( T _eff = 5200–6200 K). We homogeneously derive planet parameters using a joint photometry and radial velocity modeling framework, discuss the planets’ possible bulk compositions, and comment on their prospects for atmospheric characterization.

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