The evolution of galaxy clustering since z = 3 using the UKIDSS Ultra Deep Survey: The divergence of passive and star-forming galaxies

Monthly Notices of the Royal Astronomical Society

Volumn 407, Issue 2, 2010, Pages 1212-1222

  Hartley, W G ^a   Almaini, O ^a   Cirasuolo, M ^b   Foucaud, S ^a,c   Simpson, C ^d   Conselice, C J ^a   Smail, I ^e   McLure, R J ^b   Dunlop, J S ^b   Chuter, R W ^a   Maddox, S ^a   Lane, K P ^f   Bradshaw, E J ^a  

^a UNIVERSITY OF NOTTINGHAM   (United Kingdom)

^b UNIVERSITY OF EDINBURGH   (United Kingdom)

^c NATIONAL TAIWAN NORMAL UNIVERSITY   (Taiwan)

^d LIVERPOOL JOHN MOORES UNIVERSITY   (United Kingdom)

^e DURHAM UNIVERSITY   (United Kingdom)

^f UNIVERSITY OF OXFORD   (United Kingdom)

Author keywords

Galaxies: evolution; Galaxies: formation; Galaxies: high redshift; Infrared: galaxies; Large scale structure of Universe

Indexed keywords

LUMINANCE; STARS; SURVEYS;

CLUSTERING STRENGTH; GALAXIES:HIGH-REDSHIFT; GALAXY CLUSTERING; GALAXY EVOLUTION; GALAXY FORMATIONS; INFRARED GALAXIES; K BANDS; LARGE SCALE STRUCTURE OF UNIVERSE; STAR FORMING GALAXY;

GALAXIES;

EID: 77956412491     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2010.16972.x     Document Type: Article

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