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HerMES: Current Cosmic Infrared Background Estimates Can be Explained by Known Galaxies and their Faint Companions at z < 4
M. P. Viero, L. Moncelsi, R. F. Quadri +28
We report contributions to cosmic infrared background (CIB) intensities originating from known galaxies and their faint companions at submillimeter wavelengths. Using the publicly-…
A higher efficiency of converting gas to stars push galaxies at z ~ 1.6 well above the star-forming main sequence
J. D. Silverman, E. Daddi, G. Rodighiero +18
Local starbursts have a higher efficiency of converting gas into stars, as compared to typical star-forming galaxies at a given stellar mass, possibly indicative of different modes…
Spitzer Imaging of Strongly-Lensed Herschel-Selected Dusty Star Forming Galaxies
Brian Ma, Asantha Cooray, J. A. Calanog +23
We present the rest-frame optical spectral energy distribution and stellar masses of six Herschel- selected gravitationally lensed dusty, star-forming galaxies (DSFGs) at 1 < z < 3…
Environment of the submillimeter-bright massive starburst HFLS3 at 6.34
N. Laporte, I. Pérez-Fournon, J. A. Calanog +28
We describe the search for Lyman-break galaxies (LBGs) near the sub-millimeter bright starburst galaxy HFLS3 at 6.34 and a study on the environment of this massive galaxy dur…
GOODS-: identification of the individual galaxies responsible for the 80-290m cosmic infrared background
R. Leiton, D. Elbaz, K. Okumura +14
We propose a new method of pushing to its faintest detection limits using universal trends in the redshift evolution of the far infrared over 24m colours in the well-…
Constraining the properties of AGN host galaxies with Spectral Energy Distribution modeling
L. Ciesla, V. Charmandaris, A. Georgakakis +8
[abridged] We use the latest release of CIGALE, a galaxy SED fitting model relying on energy balance, to study the influence of an AGN in estimating both the SFR and stellar mass i…