Santa Cruz, CA 95064
Phone: (831) 459-2844
Fax: (831) 459-5265
Email: dept
Maps & Directions
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Rebecca
Bernstein
Galaxy formation and evolution. Astronomical instrumentation and optical design. rab 831-459-2835 ISB 281 |
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George R.
Blumenthal
(Chancellor) Cosmological issues such as the role played by dark matter on the origin and evolution of structure in the universe, the generation of primordial density fluctuations and fluctuations in the CMB. Other areas of his research include galaxy formation, gamma-ray bursts, accretion disks, and active galactic nuclei. george 831-459-4291 Kerr Hall |
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Michael J.
Bolte
(Director - UCO Lick Observatories) Observation of old stellar populations in globular clusters and measurements of the ages and chemical abundances of the individual stars. Among other research interests are the dynamics of globular clusters, identifying the main sequence critical mass for white dwarf formation, and extremely metal poor (EMP) stars. bolte 831-459-2991 ISB 379 |
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Jean P.
Brodie
Studies extra-galactic globular clusters systems, young massive star clusters, and galaxy formation. Brodie also works on instrumentation for for astronomy, such as the development of a multi-object spectrograph. brodie 831-459-2987 ISB 345 |
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Harland W.
Epps
Optical design of high-performance astronomical instruments such as the LRIS and HIRES spectrograph cameras for Keck, Flamingos-2 for Gemini-South, the BINOSPEC binocular spectrograph for MMT, among others. epps 831-459-3454 Nat Sci II 191 |
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Sandra
Faber
(Department Chair) Galaxy formation and evolution, study of stellar populations in globular clusters, elliptical galaxies, and distant galaxy clusters. Additionally, Faber is involved in the DEIMOS project -a multi-object spectrograph for Keck- and is a core member of the DEEP team. faber 831-459-2944 CfAO 101 |
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Jonathan
Fortney
Planetary physics, with a goal of understanding planets as a class of astronomical objects. Fortney studies planetary atmospheres, the interior structure and thermal evolution of exoplanets, as well as brown dwarfs and our solar system's giant planets. jfortney 831-502-7285 ISB 275 |
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Puragra (Raja)
GuhaThakurta
Galaxy formation and evolution: assembly, internal structure/dynamics, and chemical enrichment. Spectroscopy of resolved stellar populations in the Local Group. Distant galaxies raja 831-459-5169 ISB 271 |
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Garth
Illingworth
Studies high-redshift galaxies to understand the process of galaxy formation, using both ground-based and Space telescopes. He is also interested in the development of next-generation telescopes. gdi 831-459-2843 ISB 267 |
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David C.
Koo
Observational cosmology. Origin and evolution of high-redshift galaxies, quasars, and gas clouds. Koo is also an active collaborator of DEEP and the center for Adaptive Optics. koo 831-459-2130 ISB 263 |
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Mark
Krumholz
Formation of massive stars and star clusters, origin of the stellar initial mass function, life cycle of molecular clouds. krumholz 831-459-1312 ISB 273 |
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Gregory
Laughlin
Theoretical astrophysics with a focus on extra-solar planetary systems, the hydrodynamics of self-gravitating disks, stellar evolution, and the long-term evolution of the universe. laughlin 831-459-3208 ISB 279 |
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Douglas N.C.
Lin
The origin of the solar system, star and planet formation, planetary atmosphere and structure, dynamical evolution of planetary systems, astrophysical fluid dynamics, interstellar medium, dynamics of stellar clusters, structure of galaxies, active galactic nuclei, and galaxy formation. lin 831-459-2732 ISB 337 |
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Piero
Madau
Theoretical cosmology with an emphasis on the re-ionization of the early universe, early black holes and first mini-quasars, the star formation history of the universe, and high-resolution cosmological simulations. pmadau 831-459-3839 ISB 361 |
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Bruce H.
Margon
(Vice Chancellor-Research) High energy astrophysics, x-ray astronomy, close binary systems, digital sky surveys. margon 831-459-1596 Kerr Hall 281 |
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Claire
Max
(Director of Center for Adaptive Optics) Development of adaptive optics systems for both ground-based and space telescopes. She uses adaptive optics to resolve astronomical objects such as active galactic nuclei in infrared wavelengths. max 831-459-2049 CfAO 205 |
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Jerry
Nelson
Design and construction of large telescopes, project Scientist for Keck telescope and Thirty Meter telescope, development of adaptive optics systems. jnelson 831-459-5132 CfAO 215 |
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Jason X.
Prochaska
Damped Ly-alpha systems, Lyman limit systems, stellar abundances, thick disk imaging, cosmological simulations, fine structure evolution, and deuterium abundance. xavier 831-459-2135 ISB 359 |
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Enrico
Ramirez-Ruiz
Studies the violent universe with an emphasis on stellar explosions, gamma-ray bursts, and accretion phenomena near compact objects. enrico 831-459-3400 ISB 363 |
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Constance
Rockosi
Galactic structure and the formation of the Milky Way. Current interests include the formation of the thick disk, structure and stellar populations at the Galactic anticenter, and the dynamics of the stellar halo crockosi 831-459-5246 ISB 261 |
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Graeme H.
Smith
Old Stellar populations in the Milky Way, their evolution and contribution to the galaxy's chemical enrichment. Study of abundances in globular cluster stars. graeme 831-459-2907 ISB 135 |
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Stephen E.
Thorsett
(Dean - Physical and Biological Sciences) Main interest lies in the observation of compact objects, radioastronomy with an emphasis on radio pulsars, and high-energy astrophysics thorsett 831-459-2931 Dean's Office |
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Steven S.
Vogt
Extra-solar planet search, astronomical instrumentation, and high-dispersion spectroscopy vogt 831-459-2151 ISB 343 |
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Stanford E.
Woosley
Theoretical astrophysics with a focus on supernovae explosions and gamma-ray bursts and the nucleosynthetic, hydrodynamic and energy transport processes involved in these events. Other areas of interest include aspects of nuclear astrophysics and the fate of very massive, early stars. woosley 831-459-2976 ISB 259 |
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Adjunct Faculty | |
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Rachel
Dewey
Radio astronomy, pulsar astrophysics, VLBI astrometry. dewey 831-459-3081 ISB 269 |
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Adriane
Steinacker
Magneto-hydrodynamical (MHD) simulations of protoplanetary accretion disks and the interaction between turbulent accretion disks and planetary cores. asteinac 831-459-2790 ISB 157 |
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