Image Details

Choose export citation format:

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 7.

Varying detection strength of CO2 with respect to CO2 abundance (on the x-axis) and SNR (on the y-axis) at bandpass centers of 1.44 μm (a and d), 1.52 μm (b and e), and 1.63 μm (c and f). For each abundance and SNR, the color corresponds to the strength of the CO2 detection; the darker the purple, the stronger the detection, and the lighter the pink, the more unconstrained the detection. The top plots (a, b, and c) show CO2 detection strength for modern H2O and Archean CH4. The bottom plots (d, e, and f) show CO2 detection strength for no H2O and modern CH4.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse