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The Diversity of Cold Worlds: Age and Characterization of the Exoplanet COCONUTS-2 b

  • Authors: Rocio Kiman, Charles A. Beichman, Azul Ruiz Diaz, Jacqueline K. Faherty, Brianna Lacy, Genaro Suárez, Federico Marocco, J. Davy Kirkpatrick, Jonathan Gagné, Jessica Copeland, Ben Burningham, Niall Whiteford, Melanie J. Rowland, Daniella C. Bardalez Gagliuffi, Johanna M. Vos, Adam C. Schneider, Eileen C. Gonzales, Sherelyn Alejandro Merchan, Austin Rothermich, Richard Smart, Edgardo Costa, Rene A. Mendez

Rocio Kiman et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 9.

SED for COCONUTS-2 b. We show in orange the Gemini/FLAMINGOS-2 spectrum (Z. Zhang et al. 2025), in blue the G395H NIRSpec JWST spectrum, and in brown points the MIRI photometry. We also included photometry from the literature. MKO label (green, in increasing wavelength): Gemini/FLAMINGOS-2 Y, JMKO (NSFCam J), HMKO (NSFCam H), and KMKO (NSFCam K); WISE label (red): W1 (WISE W1), W2 (WISE W2), and W3 (WISE W3); Spitzer label (purple): [3.6] (IRAC I1) and [4.5] (IRAC I2); and MIRI label (brown): MIRI F1000W, MIRI F1280W, and MIRI F1800W. See Table 1 for the magnitude of each photometry point. The gray line represents the connecting lines, as well as the Wien and RJ approximations, extending beyond the existing data.

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