The clustering of galaxies in the SDSS-III baryon oscillation spectroscopic survey: Measuring H(z) and DA (z) at z = 0.57 with clustering wedges

Monthly Notices of the Royal Astronomical Society

Volumn 435, Issue 1, 2013, Pages 64-86

  Kazin, Eyal A ^a,b   Sánchez, Ariel G ^c   Cuesta, Antonio J ^d   Beutler, Florian ^e   Chuang, Chia Hsun ^f   Eisenstein, Daniel J ^g   Manera, Marc ^h   Padmanabhan, Nikhil ^d   Percival, Will J ^h   Prada, Francisco ^f,i,j   Ross, Ashley J ^h   Seo, Hee Jong ^e   Tinker, Jeremy ^k   Tojeiro, Rita ^h   Xu, Xiaoying ^l   Brinkmann, J ^m   Joel, Brownstein ⁿ   Nichol, Robert C ^h   Schlegel, David J ^e   Schneider, Donald P ^o   Thomas, Daniel ^h   more..

^a SWINBURNE UNIVERSITY OF TECHNOLOGY   (Australia)

^b ARC CENTRE OF EXCELLENCE FOR ALL SKY ASTROPHYSICS CAASTRO   (Australia)

^c MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^d Yale University   (United States)

^e LAWRENCE BERKELEY NATIONAL LABORATORY   (United States)

^f CSIC   (Spain)

^g HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^h UNIVERSITY OF PORTSMOUTH   (United Kingdom)

ⁱ INSTITUTO DE ASTROFÍSICA DE ANDALUCÍA CSIC   (Spain)

^j Campus of International Excellence   (Spain)

^k NEW YORK UNIVERSITY   (United States)

^l CARNEGIE MELLON UNIVERSITY   (United States)

^m APACHE POINT OBSERVATORY   (United States)

ⁿ UNIVERSITY OF UTAH   (United States)

^o PENNSYLVANIA STATE UNIVERSITY   (United States)

more..

Author keywords

Cosmological parameters; Distance scale; Large scale structure of Universe

Indexed keywords

EID: 84885151285     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1093/mnras/stt1261     Document Type: Article

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