An ALMA survey of submillimetre galaxies in the COSMOS field: Physical properties derived from energy balance spectral energy distribution modelling

We determine the physical properties of a sample of SMGs in the COSMOS field that were pre-selected at the observed wavelength of \(\lambda_{\rm obs}=1.1\) mm, and followed up at \(\lambda_{\rm obs}=1.3\) mm with ALMA. We used MAGPHYS to fit the panchromatic (ultraviolet to radio) SEDs of 124 of the...

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Veröffentlicht in:	arXiv.org 2017-07
Hauptverfasser:	Miettinen, Oskari, Delvecchio, Ivan, Smolčić, Vernesa, Aravena, Manuel, Brisbin, Drew, Karim, Alexander, Magnelli, Benjamin, Novak, Mladen, Schinnerer, Eva, Albrecht, Marcus, Aussel, Hervé, Bertoldi, Frank, Capak, Peter L, Casey, Caitlin M, Hayward, Christopher C, Ilbert, Olivier, Intema, Huib T, Jiang, Chunyan, Olivier Le Fèvre, McCracken, Henry J, Muñoz Arancibia, Alejandra M, Navarrete, Felipe, Padilla, Nelson D, Riechers, Dominik A, Salvato, Mara, Scott, Kimberly S, Sheth, Kartik, Tasca, Lidia A M
Format:	Artikel
Sprache:	eng
Schlagworte:	Compact galaxies Cosmos Dust Galaxies Median (statistics) Molecular gases Morphology Physical properties Physics - Astrophysics of Galaxies Radio Samples (statistical) Spectral energy distribution Star & galaxy formation Star formation
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