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MEASURING THE MEAN AND SCATTER OF THE X-RAY LUMINOSITY-OPTICAL RICHNESS RELATION FOR maxBCG GALAXY CLUSTERS

Author
RYKOFF, E. S1 2 ; MCKAY, T. A2 3 4 ; BECKER, M. R2 ; EVRARD, A2 3 4 ; JOHNSTON, D. E5 ; KOESTER, B. P6 ; ROZO, E7 ; SHELDON, E. S8 ; WECHSLER, R. H9
[1] TABASCO Fellow, Physics Department, University of California at Santa Barbara, Santa Barbara, CA 93106, United States
[2] Physics Department, University of Michigan, Ann Arbor, MI 48109, United States
[3] Astronomy Department, University of Michigan, Ann Arbor, MI 48109, United States
[4] Michigan Center for Theoretical Physics, Ann Arbor, MI 48109, United States
[5] Jet Propulsion Laboratory, Pasadena, CA 91109, United States
[6] Department of Astronomy, University of Chicago, Chicago, IL 60637, United States
[7] CCAPP Fellow, Ohio State University, Columbus, OH 43201, United States
[8] Center for Cosmology and Particle Physics, Physics Department, New York University, New York, NY 10003, United States
[9] Kavli Institute for Particle Astrophysics and Cosmology, Physics Department and Stanford Linear Accelerator Center, Stanford University, Stanford, CA 94305, United States
Source

The Astrophysical journal. 2008, Vol 675, Num 2, pp 1106-1124, 19 p ; 1 ; ref : 1 p

CODEN
ASJOAB
ISSN
0004-637X
Scientific domain
Astronomy earth cosmic environment
Publisher
University of Chicago Press, Chicago, IL
Publication country
United States
Document type
Article
Language
English
Author keyword
X-rays: galaxies: clusters galaxies: clusters: general
Keyword (fr)
Amas galaxies RX Amas galaxies Luminosité Source RX cosmique
Keyword (en)
X ray cluster of galaxies Galaxy clusters Luminosity Cosmic x-ray sources
Keyword (es)
Conglomerado galaxias RX
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
20183927

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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