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A Ground-based Transit Observation of the Long-period Extremely Low-density Planet HIP 41378 f

  • Authors: Juliana García-Mejía, Zoë L. de Beurs, Patrick Tamburo, Andrew Vanderburg, David Charbonneau, Karen A. Collins, Khalid Barkaoui, Cristilyn N. Watkins, Chris Stockdale, Richard P. Schwarz, Raquel Forés-Toribio, Jose A. Muñoz, Giovanni Isopi, Franco Mallia, Aldo Zapparata, Adam Popowicz, Andrzej Brudny, Eric Agol, Munazza K. Alam, Zouhair Benkhaldoun, Jehin Emmanuel, Mourad Ghachoui, Michaël Gillon, Keith Horne, Enric Palle, Ramotholo Sefako, Avi Shporer, Mathilde Timmermans

Juliana García-Mejía et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 5.

The posterior density distribution of TC,6 obtained from the MCMC simulation. Vertical lines indicate the limits of the 68.27% (solid, dark purple), 95.45% (dashed, medium purple), and 99.73% (dotted, light purple) credibility intervals. The posterior is a uniform distribution since we did not catch HIP 41378 f during ingress or egress.

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