Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

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 3.

The stellar property distribution encompassed within the EVE fields is plotted over the color–magnitude diagram (top), and as a function of stellar mass, radius, effective temperature, magnitude, and age (bottom). The zero-age main sequence (ZAMS) and the 50 Myr solar metallicity nonrotating isochrone as per A. Dotter (2016) is marked by the dashed and dotted lines, respectively. The simulated planet hosts are marked by stars. Stellar properties are adopted from the TESS input catalog (K. G. Stassun et al. 2019).

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article

Show More

Copyright and Terms & Conditions

Additional terms of reuse