Lincoln J. Greenhill
Work Address:
Harvard-Smithsonian Center for Astrophysics60 Garden St., Mail Stop 42 Cambridge, MA 02138(617) 495-7194 (V) 7345 (F) http://cfa-www.harvard.edu/~lincoln http://scholar.harvard.edu/lgreenhill
Education:
1990 Ph.D., Astronomy, Harvard University
Dissertation: VLBI Observations of Extragalactic H2O masers Supervisor: J. M. Moran
1985 M.A., Astronomy, Harvard University
1984 S.B., Physics, Massachusetts Institute of TechnologyThesis: Reprocessing of Gamma Ray Burst Radiation on Stellar Surfaces Supervisor: S. A. Rappaport
Dissertation: VLBI Observations of Extragalactic H2O masers Supervisor: J. M. Moran
1985 M.A., Astronomy, Harvard University
1984 S.B., Physics, Massachusetts Institute of TechnologyThesis: Reprocessing of Gamma Ray Burst Radiation on Stellar Surfaces Supervisor: S. A. Rappaport
Professional Experience:
| 2009 | Visiting Professor, Miller Institute for Basic Research in Science, University of California – Berkeley (fall semester residence). |
| 2008-2010 | Project Scientist, Murchison Wide-field Array (MWA). |
| 2007- | Senior Research Fellow, Department of Astronomy, Harvard University. |
| 2003-2004 |
Visiting Physicist, Stanford University, Kavli Institute for Particle Astrophysics and Cosmology (sabbatical). |
| 2002-2011 | Lecturer, Department of Astronomy, Harvard University. |
| 2000- | Radio Astronomer, Smithsonian Astrophysical Observatory. |
| 1997 | Assistant Director, Maria Mitchell Observatory. |
| 1992-2000 | Radio Astronomer (term), Smithsonian Astrophysical Observatory |
| 1990-1992 | Fellow, Miller Institute for Basic Research in Science, University of California – Berkeley. Mentors: C. Townes/W. Welch. |
| 1984-1990 | Research Assistant, Harvard-Smithsonian Center for Astrophysics |
| 1983, 1984 | Intern, General Electric Corporate Research and Development Center, Schenectady, NY. |
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Principal Interests:
Cosmology — cosmological dark age and reionization, dark energy, estimation of cosmological parameters. Supermassive black holes — accretion disk geometries, jets, the structure of active galactic nuclei. Star formation — structure and gas dynamics in close proximity to high-mass young stars. Astronomical masers. Interferometry. Signal processing. High Performance Computing. Massively parallel computing (GPGPU).CV upload:
