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most citedCosmology and the Bispectrum

270 citations · 4.8k across the 154 of their papers we have counts for

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astro-ph2008★ 19 cited

Weak Lensing Effects on the Galaxy Three-Point Correlation Function

Fabian Schmidt, Alberto Vallinotto, Emiliano Sefusatti +1

We study the corrections to the galaxy three-point correlation function (3PCF) induced by weak lensing magnification due to the matter distribution along the line of sight. We cons…

astro-ph2008★ 95 cited

The Correlation Function of Optically Selected Galaxy Clusters in the Sloan Digital Sky Survey

Juan Estrada, Emiliano Sefusatti, Joshua A. Frieman

We measure the two-point spatial correlation function for clusters selected from the photometric MaxBCG galaxy cluster catalog for the Sloan Digital Sky Survey (SDSS). We evaluate…

astro-ph2007★ 242 cited

The bispectrum of galaxies from high-redshift galaxy surveys: primordial non-Gaussianity and non-linear galaxy bias

Emiliano Sefusatti, Eiichiro Komatsu

The greatest challenge in the interpretation of galaxy clustering data from any surveys is galaxy bias. Using a simple Fisher matrix analysis, we show that the bispectrum provides…

astro-ph2006★ 41 cited

Primordial non-Gaussianity and Dark Energy constraints from Cluster Surveys

Emiliano Sefusatti, Chris Vale, Kenji Kadota +1

Galaxy cluster surveys will be a powerful probe of dark energy. At the same time, cluster abundance is sensitive to any non-Gaussianity of the primordial density field. It is there…

astro-ph2006★ 270 cited

Cosmology and the Bispectrum

Emiliano Sefusatti, Martin Crocce, Sebastian Pueblas +1

The present spatial distribution of galaxies in the Universe is non-Gaussian, with 40% skewness in 50 Mpc/h spheres, and remarkably little is known about the information encoded in…

astro-ph2004★ 82 cited

Galaxy Bias and Halo-Occupation Numbers from Large-Scale Clustering

Emiliano Sefusatti, Roman Scoccimarro

We show that current surveys have at least as much signal to noise in higher-order statistics as in the power spectrum at weakly nonlinear scales. We discuss how one can use this i…