Fig. 4 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. 4.

Redshift distribution of the CFHTLS sample. The dashed histogram shows the photometric redshift distribution of the galaxies selected with the color criterion alone, while the solid histogram shows the final redshift distribution after selecting objects with ﹩0.7< z_{\mathrm{phot}\,}< 1.3﹩. The dotted and dot‐dashed histograms show the redshift distributions of ﹩\mathrm{FUV}\,_{\mathrm{abs}\,}< -19.41﹩ and ﹩\mathrm{FUV}\,_{\mathrm{abs}\,}> -19.41﹩, respectively.

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