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Faculty Research

Robert Antonucci

  • Quasars, radio galaxies, Seyfert galaxies
  • Geometrical "Unified Models" for the above
  • Energy sources for the above
  • Scattering in the intergalactic medium

Lars Bildsten

  • Stellar astrophysics, focusing on accreting neutron stars and white dwarfs
  • X-/gamma-ray observations of compact stars
  • Gravitational wave sources
  • Theory of stellar pulsations and explosive thermonuclear instabilities

Omer Blaes

  • Accretion flows onto compact objects, radiation, and MHD processes
  • Theoretical spectral energy distributions, polarization, and variability of active galactic nuclei and quasars
  • Astrophysics of supermassive black holes
 

Tim Brown

  • The Las Cumbres Observatory

Carl Gwinn

  • Pulsars
  • Interstellar wave propagation
  • Gravitational radiation

Andy Howell

  • Supernovae
  • Dark energy
 

Philip Lubin

  • Experimental cosmology
  • Satellite, balloon-born and ground based studies of the early universe
  • Cosmic Background Radiation - spectrum, anisotropy and polarization
  • Galaxy cluster cooling (Sunyaev-Zeldovich) measurements

Crystal Martin

  • Star formation and feedback in galaxies
  • Interplay between galaxies and the intergalactic medium
  • Effect of environment on galaxy evolution

Ben Mazin

  • Microwave Kinetic Inductance Detectors
  • High time resolution observations of compact objects
  • Coronagraphic planet finding

Ben Monreal

  • Particle astrophysics
  • Neutrinos and dark matter

Harry Nelson

  • Experimental particle physics
  • Direct detection of dark matter

Peng Oh

  • Intergalactic medium, Ly-alpha forest
  • 21cm cosmology
  • First stars, reionization
  • Galaxy clusters, AGN feedback

Stan Peale

  • Planetary science
  • Extra-solar planets

Tommaso Treu

  • Galaxy formation and evolution. In particular early-type galaxies, galaxies in clusters, and high redshift galaxies
  • Co-evolution of spheroids and black-holes
  • Gravitational lensing and dark matter in galaxies and clusters of galaxies
  • Hubble constant from gravitational time delays
         

 

 
   

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