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- M. Strauss, Michael Blanton, +64 authors Donald G. York
- 2003

Max Tegmark, Michael A. Strauss, Michael R. Blanton, Kevork Abazajian, Scott Dodelson, Havard Sandvik, Xiaomin Wang, David H. Weinberg, Idit Zehavi, Neta A. Bahcall, Fiona Hoyle, David Schlegel,â€¦ (More)

- Max Tegmark, Daniel J. Eisenstein, +64 authors Donald G. York
- 2006

Max Tegmark, Daniel J. Eisenstein, Michael A. Strauss, David H. Weinberg, Michael R. Blanton, Joshua A. Frieman, Masataka Fukugita, James E. Gunn, Andrew J. S. Hamilton, Gillian R. Knapp, Robert C.â€¦ (More)

- Ravi K. Sheth, Hiltunen Mo, Giuseppe Tormen
- 1999

The Pressâ€“Schechter, excursion set approach allows one to make predictions about the shape and evolution of the mass function of bound objects. The approach combines the assumption that objectsâ€¦ (More)

- Ravi K. Sheth, Giuseppe Tormen
- 1998

Dark matter haloes are biased tracers of the underlying dark matter distribution. We use a simple model to provide a relation between the abundance of dark matter haloes and their spatialâ€¦ (More)

- Max Tegmark, Michael Blanton, +62 authors Donald G. York
- 2003

We measure the large-scale real-space power spectrum P (k) using a sample of 205,443 galaxies from the Sloan Digital Sky Survey, covering 2417 effective square degrees with mean redshift z â‰ˆ 0.1. Weâ€¦ (More)

We study galaxy clustering in the framework of halo models, where gravitational clustering is described in terms of dark matter halos. At small scales, dark matter clustering statistics are dominatedâ€¦ (More)

- Ravi K. Sheth
- 2001

We present a simple model for the shape of the distribution function of galaxy peculiar velocities. We show how both nonlinear and linear theory terms combine to produce a distribution which has anâ€¦ (More)

The baryonic acoustic signature in the large-scale clustering pattern of galaxies has been detected in the two-point correlation function. Its precise spatial scale has been forwarded as a rigid-rodâ€¦ (More)

We present accurate predictions of the correlation function of hotspots in the microwave background radiation for gaussian theories such as those predicted in most inflation models. The correlationâ€¦ (More)

- Elena Tundo, Mariangela Bernardi, J. Hyde, Ravi K. Sheth, Alessandro Pizzella
- 2007

Black hole masses are tightly correlated with the stellar velocity dispersions of the bulges which surround them, and slightly less-well correlated with the bulge luminosity. It is common to useâ€¦ (More)