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Preparing for the Early eVolution Explorer: Detecting the Primordial, Transiting Exoplanet Population

  • Authors: George Zhou, James G. Rogers, Jennifer A. Burt, Eve J. Lee, Sydney Vach, Ann Marie Cody, Mark Swain, Neal J. Turner, Andrew W. Mann, Madyson G. Barber, Eric Gaidos, Ward Howard, Laura Venuti, Damon F. Landau, Valerie Scott, Alan Didion, David Makowski, Jamie Nastal, Evgenya L. Shkolnik, Meredith A. MacGregor

George Zhou et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 14.

EVE will probe transit depth differences in the optical and infrared. Spectral models of K2-33 b and HIP 67522b are shown, and transit depths and uncertainties are computed over the EVE bands over these models assuming a distance of 350 pc—a characteristic distance for regions targeted in Figure 2. The K2-33 b model is adopted from P. C. Thao et al. (2023), showing absorption due to Tholin haze. The HIP 67522b model for a clear and non-star-spot-affected atmosphere is adopted from P. C. Thao et al. (2024).

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