Fig. 1 from Galaxy Evolution Explorer Ultraviolet Spectroscopy and Deep Imaging of Luminous Infrared Galaxies in the European Large‐Area ISO Survey S1 Field

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Galaxy Evolution Explorer Ultraviolet Spectroscopy and Deep Imaging of Luminous Infrared Galaxies in the European Large‐Area ISO Survey S1 Field

Authors: Denis Burgarella, Véronique Buat, Todd Small, Tom A. Barlow, Samuel Boissier, Armando Gil de Paz, Timothy M. Heckman, Barry F. Madore, D. Christopher Martin, R. Michael Rich, Luciana Bianchi, Yong-Ik Byun, Jose Donas, Karl Forster, Peter G. Friedman, Patrick N. Jelinsky, Young-Wook Lee, Roger F. Malina, Bruno Milliard, Patrick Morrissey, Susan G. Neff, David Schiminovich, Oswald H. W. Siegmund, Alex S. Szalay, Barry Y. Welsh, and Ted K. Wyder

Burgarella et al. 2005 The Astrophysical Journal Letters 619 L63.

Provider: AAS Journals

Caption: Fig. 1.

One of the best fits of a power law on the spectrum of ELAISC15 J003828−433848 at ﹩z=0.048﹩ (﹩\beta =-1.58\pm 0.04﹩) (top) and one of the worst for ELAISC15 J003531−434448 at ﹩z=0.286﹩ (﹩\beta =-2.04\pm 0.27﹩) (bottom). Note that because of its redshift, the fit of the latter spectrum was performed on fewer pixels, since we do not use pixels at ﹩\lambda \leq 1200\,\Å ﹩.

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