Fig. 7 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. 7.

Dependence on absolute FUV magnitude of the correlation length ﹩r_{0}﹩ for low‐ and high‐redshift rest‐frame UV‐selected galaxies (Adelberger et al. 2005, open squares; Arnouts et al. 2002, open star; Foucaud et al. 2003, open triangles; Giavalisco & Dickinson 2001, open circles). Our results are presented as filled circles (FUV) and filled squares (NUV) for the GALEX samples and as filled stars for the CFHTLS samples. The mean redshifts of the samples are color‐coded. Note that the results from a given study (including ours) are not all obtained from independent samples. Hence, we distinguish global samples by plotting them with a bigger symbol size, in this figure and in the following ones as well, unless otherwise stated.

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