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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 1.

Sky-projected field of view of the observatories from where multi-night datasets were gathered, in R.A. and decl. coordinates. The field outlines are color-coded as follows: Tierras is shown in pink, TRAPPIST-North in violet, LCOGT McD 0.35 m in teal, McDonald 1.0 m (T1) in light blue, and McDonald 1.0 m (T2) in dark blue. The thick black outline shows the flux-limited overlapping field of view between facilities, which contains only ∼6% of HIP 41378’s flux in available comparison stars. HIP 41378 is highlighted with a red star symbol.

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