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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

Education

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

Selected Publications

Wolfgang, A., Rogers, L. A. & Ford, E. B. "Probabilistic Mass-Radius Relationship for Sub-Neptune-Sized Planets", 2015, submitted to ApJ, arXiv:1504.07557.

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.

Mullally, F. et al. (59 coauthors, incl. Wolfgang, A.) "Planetary Candidates Observed by Kepler VI: Planet Sample from Q1-Q16 (47 Months)'', 2015, ApJS, 217, 31. 

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 here in our own Solar System, yet we have discovered thousands orbiting other stars.  As a result, what these planets are like and how they came to exist is an enormously exciting mystery.  Given their vast numbers, I tackle these questions by applying models describing the entire super-Earth population to the data from the Kepler Mission; through the power of advanced statistical methods, I am able to constrain different scenarios for how these planets could have evolved to their current states since formation.

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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