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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 5.

Minimum SNR required for a strong CO2 detection at each bandpass center for the three highest CO2 abundances that achieve strong detections. Venus-like is plotted in purple stars, Archean-like is plotted in light pink squares, and Proterozoic-like is plotted in magenta circles. The shaded regions represent the spaces in which you could achieve a strong detection for each abundance in their respective colors. The x-axis is bandpass center (μm) and the y-axis is SNR.

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