The Astronomical Journal (Jan 2023)

Searching for Planets Orbiting Fomalhaut with JWST/NIRCam

  • Marie Ygouf,
  • Charles A. Beichman,
  • Jorge Llop-Sayson,
  • Geoffrey Bryden,
  • Jarron M. Leisenring,
  • András Gáspár,
  • John E. Krist,
  • Marcia J. Rieke,
  • George H. Rieke,
  • Schuyler Grace Wolff,
  • Thomas L. Roellig,
  • Kate Su,
  • Kevin N. Hainline,
  • Klaus W. Hodapp,
  • Thomas P. Greene,
  • Michael R. Meyer,
  • Douglas M. Kelly,
  • Karl Misselt,
  • John Stansberry,
  • Martha Boyer,
  • Doug Johnstone,
  • Scott Horner,
  • Alexandra Z. Greenbaum

DOI
https://doi.org/10.3847/1538-3881/ad08c8
Journal volume & issue
Vol. 167, no. 1
p. 26

Abstract

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We report observations with the JWST/NIRCam coronagraph of the Fomalhaut ( α PsA) system. This nearby A star hosts a complex debris disk system discovered by the IRAS satellite. Observations in F444W and F356W filters using the round 430R mask achieve a contrast ratio of ∼4 × 10 ^−7 at 1″ and ∼4 × 10 ^−8 outside of 3″. These observations reach a sensitivity limit of 0.7 mag (Vega) color. Whether this object is a background galaxy, brown dwarf, or a Jovian-mass planet in the Fomalhaut system will be determined by an approved Cycle 2 follow-up program. Finally, we set upper limits to any scattered light from the outer ring, placing a weak limit on the dust albedo at F356W and F444W.

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