Overlap of quiescent K and M dwarfs (red stars) with transiting exoplanet hosts (black dots) in stellar Teff and metallicity space. The range of targets selected for this proposal (blue circled red stars) allows for broad expansion and testing of model atmospheres in...
Due to the COVID19 panedemic, our AE team suspended most in-person interactions for more than a year; and the AE breakfasts for almost two years. In September 2022, we held our first real, in-person AE breakfast in a while. It has been great to meet team members again...
Protoplanetary disks offer an opportunity to learn about the processes by which planetary systems form and evolve. Images of these young systems also enable us to study, by analogy, the formation of our own Solar System, in which the common orbital plane of the...
The key goal of EOS is to advance our understanding of the formation of habitable planets. As an unusually large and ambitious program, EOS is in a rare position to successfully integrate interdisciplinary knowledge on planet formation – that is, to combine...
