#### Filter Results:

- Full text PDF available (107)

#### Publication Year

1986

2018

- This year (1)
- Last 5 years (24)
- Last 10 years (46)

#### Publication Type

#### Co-author

#### Journals and Conferences

Learn More

- Max Tegmark, Michael A. Strauss, +69 authors Donald G. York
- 2003

Department of Physics, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USA Department of Physics, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA Princetonâ€¦ (More)

The formation of galaxy clusters in hierarchically clustering universes is investigated by means of high resolution N-body simulations. The simulations are performed using a newly developedâ€¦ (More)

- L. Van Waerbeke, Yannick Mellier, +10 authors Peter Schneider
- 2000

We report the detection of a significant (5.5 Ïƒ) excess of correlation between galaxy ellipticities at scales ranging from 0.5 to 3.5 arc-minutes. This detection of a gravitational lensing signal byâ€¦ (More)

- Max Tegmark, Daniel J. Eisenstein, +68 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)

- Max Tegmark, Michael Blanton, +70 authors Donald G. York
- 2003

We measure the large-scale real-space power spectrum PÃ°kÃž by using a sample of 205,443 galaxies from the Sloan Digital Sky Survey, covering 2417 effective square degrees with mean redshift z 0:1. Weâ€¦ (More)

We examine how lensing tomography with the bispectrum and power spectrum can constrain cosmological parameters and the equation of state of dark energy. Our analysis uses the full information at theâ€¦ (More)

- Bhuvnesh Jain
- 1999

We investigate weak lensing by large-scale structure using ray tracing through N-body simulations. Photon trajectories are followed through high resolution simulations of structure formation to makeâ€¦ (More)

- M. Jarvis, Paul Schechter, Bhuvnesh Jain
- 2008

In weak lensing investigations, galaxy shapes are correcte d for the convolution by the point spread function (PSF) using stellar images. In this paper we use physical models of the telescope opticsâ€¦ (More)

Given the basic parameters of a cosmic shear weak lensing survey, how well can systematic errors due to anisotropy in the point spread function (PSF) be corrected? The largest source of error in thisâ€¦ (More)

- L. Van Waerbeke, Yannick Mellier, Roser Pello, U-L. Pen, H J Mccracken, Bhuvnesh Jain
- 2002

We present a maximum likelihood analysis of cosmological parameters from measurements of the aperture mass up to 35 arcmin, using simulated and real cosmic shear data. A four-dimensional parameterâ€¦ (More)