The VIMOS Public Extragalactic Redshift Survey (VIPERS)

F. Marulli; M. Bolzonella; E. Branchini; I. Davidzon; S. de la Torre; B. R. Granett; L. Guzzo; A. Iovino; L. Moscardini; A. Pollo; U. Abbas; C. Adami; S. Arnouts; J. Bel; D. Bottini; A. Cappi; J. Coupon; O. Cucciati; G. De Lucia; A. Fritz; P. Franzetti; M. Fumana; B. Garilli; O. Ilbert; J. Krywult; V. Le Brun; O. Le Févre; D. Maccagni; K. Małek; H. J. McCracken; L. Paioro; M. Polletta; H. Schlagenhaufer; M. Scodeggio; L. A. M. Tasca; Rita Tojeiro; D. Vergani; A. Zanichelli; A. Burden; C. Di Porto; A. Marchetti; C. Marinoni; Y. Mellier; R. C. Nichol; J. A. Peacock; Will J. Percival; S. Phleps; M. Wolk; G. Zamorani

doi:10.1051/0004-6361/201321476

Abstract

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Aims. We investigate the dependence of galaxy clustering on luminosity and stellar mass in the redshift range 0.5 < z < 1.1, using the first ~ 55 000 redshifts from the VIMOS Public Extragalactic Redshift Survey (VIPERS).

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synapsesocial.com/papers/6a156a7015658026c082557c https://doi.org/10.1051/0004-6361/201321476

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The VIMOS Public Extragalactic Redshift Survey (VIPERS)

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The VIMOS Public Extragalactic Redshift Survey (VIPERS)

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