UV to IR SEDs of UV-Selected Galaxies in the ELAIS Fields: Evolution of Dust Attenuation and Star Formation Activity from z = 0.7 to 0.2

Author affiliations

¹ Instituto de Astrofísica de Andalucía (IAA, CSIC), Camino Bajo de Huétor 50, 18008 Granada, Spain

² Observatoire Astronomique Marseille Provence, Laboratoire d'Astrophysique de Marseille, 13012, Marseille, France

³ California Institute of Technology, MC 405-47, 1200 East California Boulevard, Pasadena, CA 91125

⁴ Infrared Processing and Analysis Center, California Institute of Technology, 100-22, Pasadena, CA 91125

⁵ Institute for Advanced Research, Nagoya University, Furo-cho, Chikusa-ku, Nagoya 464-8601, Japan

⁶ Spitzer Science Center, California Institute of Technology, Mail Stop 220-6, Pasadena, CA 91125

⁷ Astrophysics Group, Blackett Laboratory, Imperial College of Science, Technology and Medicine, Prince Consort Road, London SW7 2BZ, UK

⁸ Department of Astronomy, Cornell University, Ithaca, NY 14853

⁹ Institute of Astronomy, Madingley Road, Cambridge CB3 0HA, UK

¹⁰ Center for Astrophysics and Space Sciences, University of California, San Diego, La Jolla, CA 92093-0424

¹¹ Laboratory for Astronomy and Solar Physics, NASA Goddard Space Flight Center, Greenbelt, MD 20771

¹² Department of Astronomy, Columbia University, New York, NY 10027

¹³ Center for Astrophysical Sciences, The Johns Hopkins University, 3400 North Charles Street, Baltimore, MD 21218

¹⁴ Department of Physics and Astronomy, The Johns Hopkins University, Homewood Campus, Baltimore, MD 21218

¹⁵ Center for Space Astrophysics, Yonsei University, Seoul 120-749, Korea

¹⁶ Observatories of the Carnegie Institution of Washington, 813 Santa Barbara Street, Pasadena, CA 91101

¹⁷ Department of Physics and Astronomy, University of California, Los Angeles, CA 90095

¹⁸ Space Sciences Laboratory, University of California at Berkeley, 601 Campbell Hall, Berkeley, CA 94720