Author: Nevalainen J. Tempel E. Liivamägi L. J. Branchini E. Roncarelli M. Giocoli C. Heinämäki P. Saar E. Tamm A. Finoguenov A. Nurmi P. Bonamente M.
Publisher: Edp Sciences
E-ISSN: 1432-0746|583|issue|A142-A142
ISSN: 0004-6361
Source: Astronomy & Astrophysics, Vol.583, Iss.issue, 2015-11, pp. : A142-A142
Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.
Abstract
Related content
Missing baryons in shells around galaxy clusters
Astronomy & Astrophysics, Vol. 492, Iss. 3, 2008-12 ,pp. :
What determines large scale galaxy clustering: halo mass or local density?
By Pujol Arnau Hoffmann Kai Jiménez Noelia Gaztañaga Enrique
Astronomy & Astrophysics, Vol. 598, Iss. issue, 2017-02 ,pp. :
Large-scale galaxy correlations as a test for dark energy
Astronomy & Astrophysics, Vol. 449, Iss. 3, 2006-04 ,pp. :
Large-scale variations of the dust optical properties in the Galaxy
Astronomy & Astrophysics, Vol. 435, Iss. 1, 2005-05 ,pp. :
Very large-scale correlations in the galaxy distribution
EPL (EUROPHYSICS LETTERS), Vol. 96, Iss. 5, 2011-11 ,pp. :