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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 5.

Binned rms analysis for each spectral bin, which shows no evidence of red noise. The rms of the data residuals are shown by the colored lines. The solid black line is the theoretical trend from P. Cubillos et al. (2017). The dashed white line is the median value from simulated pure white-noise residuals. The gray regions are the 1 and 2σ ranges for the simulated white-noise residuals, which demonstrates that the observed data are consistent with being largely uncorrelated (e.g., white noise).

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