Fig. 1 from The GALEX‐VVDS Measurement of the Evolution of the Far‐Ultraviolet Luminosity Density and the Cosmic Star Formation Rate

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The GALEX‐VVDS Measurement of the Evolution of the Far‐Ultraviolet Luminosity Density and the Cosmic Star Formation Rate

Authors: D. Schiminovich, O. Ilbert, S. Arnouts, B. Milliard, L. Tresse, O. Le Fèvre, M. Treyer, T. K. Wyder, T. Budavári, E. Zucca, G. Zamorani, D. C. Martin, C. Adami, M. Arnaboldi, S. Bardelli, T. Barlow, L. Bianchi, M. Bolzonella, D. Bottini, Y.-I. Byun, A. Cappi, T. Contini, S. Charlot, J. Donas, K. Forster, S. Foucaud, P. Franzetti, P. G. Friedman, B. Garilli, I. Gavignaud, L. Guzzo, T. M. Heckman, C. Hoopes, A. Iovino, P. Jelinsky, V. Le Brun, Y.-W. Lee, D. Maccagni, B. F. Madore, R. Malina, B. Marano, C. Marinoni, H. J. McCracken, A. Mazure, B. Meneux, P. Morrissey, S. Neff, S. Paltani, R. Pellò, J. P. Picat, A. Pollo, L. Pozzetti, M. Radovich, R. M. Rich, R. Scaramella, M. Scodeggio, M. Seibert, O. Siegmund, T. Small, A. S. Szalay, G. Vettolani, B. Welsh, C. K. Xu, and A. Zanichelli

Schiminovich et al. 2005 The Astrophysical Journal Letters 619 L47.

Provider: AAS Journals

Caption: Fig. 1.

FUV LD vs. redshift. Filled circles indicate LF fit to full sample with unconstrained slope α. Filled squares denote LF fit with fixed ﹩\alpha =-1.6﹩. Purple (GALEX) and dark green (HDF) symbols are from this work. Black filled circle (bottom left) is taken from local LF (Wyder et al. 2005) and green square from Steidel et al. (1999). Open circles denote ﹩\rho _{1500}﹩ determined using V_max. Errors do not include cosmic variance. Lines indicate ﹩( 1+z) ^{n}﹩ evolution. Dotted, solid, and dashed lines correspond to ﹩n=1.5,\,2.5,\,\mathrm{and}\,\,3.5﹩, respectively.

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