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Título: | Herschel-ATLAS: Evolution of the 250 µm luminosity function out to z = 0.5 |
Autor: | Dye, S.; Herranz, D. CSIC ORCID ; López-Caniego, M. CSIC ORCID | Palabras clave: | Galaxies: luminosity function, mass function Cosmology: observations Large-scale structure of the universe |
Fecha de publicación: | 2010 | Editor: | EDP Sciences | Citación: | Astronomy and Astrophysics 518: L10 (2010) | Resumen: | We have determined the luminosity function of 250 μm-selected galaxies detected in the ~14 deg2 science demonstration region of the Herschel-ATLAS project out to a redshift of z = 0.5. Our findings very clearly show that the luminosity function evolves steadily out to this redshift. By selecting a sub-group of sources within a fixed luminosity interval where incompleteness effects are minimal, we have measured a smooth increase in the comoving 250 μm luminosity density out to z = 0.2 where it is 3.6+1.4-0.9 times higher than the local value. | Descripción: | 5 páginas, 4 figuras.-- Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA.-- et al. | Versión del editor: | http://dx.doi.org/10.1051/0004-6361/201014614 | URI: | http://hdl.handle.net/10261/46080 | DOI: | 10.1051/0004-6361/201014614 | ISSN: | 0004-6361 | E-ISSN: | 1432-0746 |
Aparece en las colecciones: | (IFCA) Artículos |
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aa14614-10[1].pdf | 131,65 kB | Adobe PDF | Visualizar/Abrir |
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