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The Transmission Spectrum of the Potentially Rocky Planet L 98-59 c

  • Authors: Thomas Barclay, Kyle B. Sheppard, Natasha Latouf, Avi M. Mandell, Elisa V. Quintana, Emily A. Gilbert, Giuliano Liuzzi, Geronimo L. Villanueva, Giada Arney, Jonathan Brande, Knicole D. Colón, Giovanni Covone, Ian J. M. Crossfield, Mario Damiano, Shawn D. Domagal-Goldman, Thomas J. Fauchez, Stefano Fiscale, Francesco Gallo, Christina L. Hedges, Renyu Hu, Edwin S. Kite, Daniel Koll, Ravi K. Kopparapu, Veselin B. Kostov, Laura Kreidberg, Eric D. Lopez, James Mang, Caroline V. Morley, Fergal Mullally, Susan E. Mullally, Daria Pidhorodetska, Joshua E. Schlieder, Laura D. Vega, Allison Youngblood, Sebastian Zieba

Thomas Barclay et al 2025 The Astronomical Journal 169 .

  • Provider: AAS Journals

Caption: Figure 9.

The reduced χ2 when various different molecules are locked to their best-fit values are shown here. In the top panel, all CO2 values are locked at approximately 10−4 VMR while the other molecules are free. In the lower panel, H2O is locked at approximately 10−6 VMR. The value obtained with a flat transmission spectrum is presented in both panels as a dotted line, portraying the scenario in which there is no atmosphere present. This plot presents at which point every combination of molecules becomes a worse assumption than having no atmosphere, i.e., becomes an unrealistic scenario. The models in the lower panel including CO2 provide a significantly better description of the data over a wide range of VMRs.

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