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Hot Rocks Survey. V. Secondary Eclipse Photometry of GJ 3473 b with JWST/MIRI

  • Authors: Måns Holmberg, Hannah Diamond-Lowe, João M. Mendonça, Daniel Kitzmann, Néstor Espinoza, Natalie H. Allen, Prune C. August, Mark Fortune, Amélie Gressier, Jegug Ih, Erik Meier Valdés, Merlin Zgraggen, Lars A. Buchhave, Brice-Olivier Demory, Chloe Fisher, Neale P. Gibson, Kevin Heng, Bibiana Prinoth, Adam J. Burgasser

Måns Holmberg et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 2.

Phase-folded and systematics-corrected MIRI data and secondary eclipse model of GJ 3473 b. The unbinned and binned data are shown in light gray and purple, respectively. To detrend the data, we subtracted the predicted GP models and divided by the systematic models. The pink curve corresponds to an eclipse model with parameters from Table 5, corresponding to our canonical case.

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