Galaxy And Mass Assembly (GAMA): the 0.013 < z < 0.1 cosmic spectral energy distribution from 0.1 m to 1 mm

Autor: J. Liske, M. L. P. Gunawardhana, E. N. Taylor, E. Andrae, R. G. Sharp, Ivan K. Baldry, Mehmet Alpaslan, William J. Sutherland, Steven P. Bamford, Aaron S. G. Robotham, Matthew Prescott, R. J. Tuffs, D. H. P. Jones, Denis Hill, Michael Brown, L. Kelvin, Peder Norberg, John A. Peacock, Loretta Dunne, H. Parkinson, Stephen M. Wilkins, C. J. Conselice, Jonathan Loveday, Ewan Cameron, Sarah Brough, Matthew Colless, Carlos S. Frenk, J. Bland-Hawthorn, Kevin A. Pimbblet, Simon P. Driver, Scott M. Croom, B. F. Madore, Alister W. Graham, N. Bourne, Mark Seibert, Andrew M. Hopkins, Robert C. Nichol, David Thomas, D. Wijesinghe, K. Kuijken, Cristina Popescu, E. van Kampen, S. Phillipps
Přispěvatelé: Science & Technology Facilities Council, University of St Andrews. University of St Andrews, University of St Andrews. School of Physics and Astronomy
Jazyk: angličtina
Rok vydání: 2012
Předmět:
Zdroj: Monthly notices of the Royal Astronomical Society, 2012, Vol.427(4), pp.3244-3264 [Peer Reviewed Journal]
Monthly Notices of the Royal Astronomical Society, 427(4), 3244-3264
ISSN: 0035-8711
Popis: We use the Galaxy And Mass Assembly survey (GAMA) I data set combined with GALEX, Sloan Digital Sky Survey (SDSS) and UKIRT Infrared Deep Sky Survey (UKIDSS) imaging to construct the low-redshift (z
Databáze: OpenAIRE