Tim Milbourne
Graduate Student
Ph.D. Physics, Harvard University, 2014-Present
B.S. Physics, College of William and Mary, 2014
Tim’s research focuses on detecting exoplanets and developing models of stellar activity to help distinguish planetary signals from the host stars. Specifically, he uses the Sun as a test case to build better models of stellar activity, which will later be applied to non-solar targets.
A group paper on Sensitivity of low-degree solar p modes to active and ephemeral regions: frequency shifts back to the Maunder Minimum has been accepted to the Monthly Notices of The Royal Astronomical Society.
A group paper on Three years of Sun-as-a-star radial-velocity observations on the approach to solar minimum has been published in the Monthly Notices of The Royal Astronomical Society.
A group paper on Three years of Sun-as-a-star radial-velocity observations on the approach to solar minimum has been posted on the arXiv.