Fig. 5 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. 5.

Angular correlation function of the GALEX subsamples cut in absolute UV magnitude: ﹩M< \langle M\rangle ﹩ is shown by squares, and ﹩M> \langle M\rangle ﹩ is shown by triangles; for comparison, the total sample (circles) is shown. Left: FUV. Right: NUV. The curves show the best‐fit power law, not corrected for the integral constraint bias. The upper axis shows the comoving scales corresponding to angular scales at ﹩z=0.18﹩ (left) or ﹩z=0.24﹩ (right).

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