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Bayesian Analysis for Remote Biosignature Identification on exoEarths (BARBIE). IV. Analyzing CO2 Detections in the Near-IR to Determine the Long-wavelength Cutoff for the Habitable Worlds Observatory Coronagraph

  • Authors: Celeste Hagee, Natasha Latouf, Avi M. Mandell, Michael D. Himes, Michael Dane Moore, Geronimo L. Villanueva

Celeste Hagee et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 6.

Detectability strength of (a) Proterozoic-like, (b) Archean-like, and (c) Venus-like CO2 abundances between 0.8 and 2.0 μm for a subset of SNRs, in this case 6, 10, 14, 18, and 20. The light pink circles portray an unconstrained detection, the magenta diamonds portray a weak detection, and the purple squares portray a strong detection, which align with the lnB classifications defined in Table 2. The 68% credible region is shaded in gray. The true value of the CO2 abundance is marked by the horizontal dashed black line.

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