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Suketu Bhavsar
Theoretical Astrophysics
Office: CP-171 Phone: (859) 257-1697
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Research Interests
- Large Scale Structure Formation
- Visual Perception of Large-Scale Structure
- Quantifying Filamentary Structure
- First-Ranked Galaxies in Galaxy Clusters
- Computational Physics
Education
- B.S., St. Xavier's College (1972)
- M.S., IIT Bombay (1974)
- M.A., Princeton University (1976)
- Ph.D., Theoretical Astrophysics, Princeton University (1978)
Undergraduate Research Projects
Graduate Students
Recent Publications
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"The Size of the Longest Filaments in the Universe"
S.Bharadwaj, S.P. Bhavsar and J.V. Sheth (2004)
Ap.J. (April, 2004 issue)
- "SHUFFLE: A New Statistical Bootstrap Method: Applied to Cosmological Filaments"
S.P. Bhavsar, S. Bharadwaj, and J.V. Sheth (2003)
in The Emergence of Cosmic Structure
eds. Stephen S. Holt and C.S. Reynolds; American Institute of Physics (AIP) pp 303-306
online version
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"The Void Distribution Function for the LCRS Data"
C.M. Brown,
S. P. Bhavsar, Bulletin of the American Astronomical Society, Vol. 34, p.1208
online version
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"Models for the Magnitude-Distribution of Brightest Cluster Galaxies"
J. P. Bernstein and S. P. Bhavsar (2001)
M.N.R.A.S., 322, 625
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"A Catalog of Nearby Poor Clusters of Galaxies"
White, Richard A.; Bliton, Mark; Bhavsar, Suketu P.; Bornmann, Patricia; Burns, Jack O.; Ledlow, Michael J.; Loken, Christen (1999)
A.J., 118, 2014
online version
Last updated April 2004
Department of Physics and Astronomy
University of Kentucky