10.6k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Centre National de la Recherche ScientifiqueFR5.8k papers
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- Université Pierre-et-Marie-CurieFR2.2k papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR1.4k papers
- California Institute of TechnologyUS1.2k papers
- University of CambridgeGB1.1k papers
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- CEA Paris-SaclayFR992 papers
- University of GenevaCH963 papers
- Observatoire de ParisFR942 papers
6 papers · 1 filter
On the galaxy luminosity function in the central regions of the Coma cluster
A. Biviano, F. Durret, D. Gerbal +4
We have obtained new redshifts for 265 objects in the central 48~~25~arcmin region of the Coma cluster. When supplemented with literature data, our redshift sample is 9…
The Power Spectrum of Galaxies in the Nearby Universe
L. N. da Costa, M. S. Vogeley, M. J. Geller +2
We compute the power spectrum of galaxy density fluctuations in a recently completed redshift survey of optically-selected galaxies in the southern hemisphere (SSRS2). The amplitud…
Simulations of the Microwave Sky and of its ``Observations''
F. R. Bouchet, R. Gispert, N. Aghanim +4
Here follows a preliminary report on the construction of fake millimeter and sub-millimeter skies, as observed by virtual instruments, e.g. the COBRA/SAMBA mission, using theoretic…
A Count Probability Cookbook: Spurious Effects and the Scaling Model
S. Colombi, F. R. Bouchet, R. Schaeffer
We study the errors brought by finite volume effects and dilution effects on the practical determination of the count probability distribution function P_N(n,L), which is the proba…
Kurtosis of Large-Scale Cosmic Fields
Ewa Luiza Lokas, Roman Juszkiewicz, David Weinberg +1
An attractive and simple hypothesis for the formation of large-scale structure is that it developed by gravitational instability from primordial fluctuations with an initially Gaus…
Omega from the skewness of the cosmic velocity divergence
F. Bernardeau, R. Juszkiewicz, A. Dekel +1
We propose a method for measuring the cosmological density parameter from the statistics of the divergence field, , the divergence of peculiar velocity, expr…