Fig. 10 from Clustering Properties of Rest‐Frame UV‐Selected Galaxies. II. Migration of Star Formation Sites with Cosmic Time from GALEX and CFHTLS

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Clustering Properties of Rest‐Frame UV‐Selected Galaxies. II. Migration of Star Formation Sites with Cosmic Time from GALEX and CFHTLS

Authors: Sébastien Heinis, Bruno Milliard, Stéphane Arnouts, Jérémy Blaizot, David Schiminovich, Tamás Budavári, Olivier Ilbert, José Donas, Marie Treyer, Ted K. Wyder, Henry J. McCracken, Tom A. Barlow, Karl Forster, Peter G. Friedman, D. Christopher Martin, Patrick Morrissey, Susan G. Neff, Mark Seibert, Todd Small, Luciana Bianchi, Timothy M. Heckman, Young-Wook Lee, Barry F. Madore, R. Michael Rich, Alex S. Szalay, Barry Y. Welsh, Sukyoung K. Yi, and C. K. Xu

Heinis et al. 2007 The Astrophysical Journal Supplement Series 173 503.

Provider: AAS Journals

Caption: Fig. 10.

Evolution with redshift of the bias of rest‐frame UV‐selected galaxies (symbols are the same as in Fig. 7). The curves show the effective bias of halos more massive than ﹩M_{\mathrm{min}\,}﹩ (color‐coded) according to Mo & White (2002; see also Paper I). The inset is an enlargement of the low‐redshift area.

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