Fig. 9 from Clustering Properties of Rest‐Frame UV‐Selected Galaxies. II. Migration of Star Formation Sites with Cosmic Time from GALEX and CFHTLS

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution

Export to PDF PPT Format

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. 9.

Dependence on absolute FUV magnitude of the slope δ of the correlation function for low‐ and high‐redshift rest‐frame UV‐selected galaxies. Results shown here come from studies allowing δ as a free parameter (Adelberger et al. 2005, open squares; Giavalisco & Dickinson 2001, open circles; Ouchi et al. 2005, crosses) (results from the fit with integral constraint). 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 error on δ comes from the fitting procedure, and the horizontal bars for our samples reflect the standard deviations of ﹩\mathrm{FUV}\,_{\mathrm{abs}\,}﹩. The mean redshifts of the samples are color‐coded.

Other Images in This Article

Copyright and Terms & Conditions