Published in

Astronomy & Astrophysics, (598), p. A103, 2017

DOI: 10.1051/0004-6361/201629121

Links

Tools

Export citation

Search in Google Scholar

What determines large scale galaxy clustering: halo mass or local density?

Journal article published in 2017 by Arnau Pujol ORCID, Kai Hoffmann, Noelia Jiménez, Enrique Gaztañaga ORCID
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

Full text: Unavailable

Green circle
Preprint: archiving allowed
Upload
Green circle
Postprint: archiving allowed
Upload
Green circle
Published version: archiving allowed
Upload
Policy details
Data provided by SHERPA/RoMEO
Beta version