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Angie Wolfgang

Angie Wolfgang

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  • NSF Fellow
403 Davey Lab
University Park, PA 16802
Phone: (814) 863-7946


  1. Ph.D., Astronomy & Astrophysics, 2015, Univ. of California, Santa Cruz
  2. M.S., Astronomy & Astrophysics, 2011, Univ. of California, Santa Cruz
  3. B.A., Physics with Education Concentration, 2009, Cornell University

Selected Publications

Wolfgang, A., Rogers, L. A. & Ford, E. B. "Probabilistic Mass-Radius Relationship for Sub-Neptune-Sized Planets"2016, ApJ, 825, 19.

Coughlin, J. L. et al. (35 coauthors, incl. Wolfgang, A.) “Planetary Candidates Observed by Kepler. VII. The First Fully Uniform Catalog Based on the Entire 48-month Data Set (Q1-Q17 DR24)”, 2016, ApJS, 224, 12.

Jenkins, J. M. et al. (28 coauthors, incl. Wolfgang, A.) "Discovery and Validation of Kepler-452b: A 1.6 Earth Radius Super Earth Exoplanet in the Habitable Zone of a G2 Star", 2015, AJ, 150, 56.

Wolfgang, A., & Lopez, E. D. "How Rocky Are They? The Composition Distribution of Kepler's Sub-Neptune Planet Candidates within 0.15 AU", 2015, ApJ, 806, 183.

Wolfgang, A., & Laughlin, G. "The Effect of Population-wide Mass-to-radius Relationships on the Interpretation of Kepler and HARPS Super-Earth Occurrence Rates'', 2012, ApJ, 750, 148

Curtis, J.L., Wolfgang, A., Wright, J. T., Brewer, John M., & Johnson, John Asher, "Ruprecht 147: The Oldest Nearby Open Cluster as a New Benchmark for Stellar Astrophysics", 2013, AJ, 145, 134.

Trichas, M. et al. (22 coauthors, incl. Wolfgang, A.), "The Chandra Multi-wavelength Project: Optical Spectroscopy and the Broadband Spectral Energy Distributions of X-Ray-selected AGNs", 2012, ApJS, 200, 17.

Research Interests

I study the recently-discovered class of extrasolar planets called “super-Earths”, whose sizes are between that of Earth and Neptune.  There are no planets like them in our own Solar System, yet we have discovered thousands orbiting other stars.  What these planets are like and how they came to exist is therefore an enormously exciting mystery.  Given their vast numbers, I tackle these questions by developing data-driven models of the entire super-Earth population and applying them to the data from planet-hunting surveys like the Kepler Mission.  Through the power of advanced statistical methods, I use these results to explore different scenarios for how these planets could have evolved to their current states.  In doing so, I have begun to establish a framework for probabilistic planetary physics.

Honors and Awards

  • National Science Foundation Astronomy & Astrophysics Postdoctoral Fellow, 2015 - 2018
  • National Science Foundation Graduate Research Fellow, 2011 - 2015
  • Eugene Cota-Robles Graduate Fellow, 2009 - 2011, 2014 - 2015

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