Aims.The total infrared (TIR: 8-1000 μm) and far-ultraviolet (FUV: ~1500 Å) luminosity functions of galaxies and the related luminosity densities $\rho_{\rm TIR}$ and $\rho_{\rm FUV}$ are known to evolve at differemt rates from $z = 0$ to z ~1: the galaxy populations appear to be brighter in the past at both wavelengths, but the evolution in the TIR is larger than in the FUV. This leads to an increase of the ratio of TIR to FUV luminosity densities $\rho_{\rm TIR}/\rho_{\rm FUV}$ which can be interpreted as a global increase of the dust attenuation from $z = 0$ to z ~ 1. Our aim is to understand the origin of this increase: is it entirely due to a variation of the dust attenuation with the luminosity of the galaxies as seen as $z = 0$ or ar...
Aims.We investigate the role of the luminous infrared galaxy (LIRG) and ultra-luminous infrared gala...
We select far-infrared (FIR: 60 μm) and far-ultraviolet (FUV: 530 Å) samples of nearby galaxies in o...
We select far-infrared (FIR-60 microns) and far-ultraviolet (FUV-1530 A) samples of nearby galaxies ...
The TIR and FUV luminosity functions of galaxies and the related luminosity densities rho(TIR) and r...
Aims. We want to study the IR (>$8\;\mu$m) emission of galaxies selected on the basis of their rest...
The ratio between far-ultraviolet (FUV) and infrared (IR) luminosity densities from z=0 to z=1 is di...
5 pages, 3 figures, accepted for publication in A&A LettersThe ratio between far-ultraviolet (FUV) a...
International audienceWe take advantage of the sensitivity and resolution of the Herschel Space Obse...
International audienceWe take advantage of the sensitivity and resolution of the Herschel Space Obse...
We analyze the dust attenuation properties of a volume-limited, optically selected sample of normal ...
Aims. We derive the evolution of the infrared luminosity function (LF) over the last 4/5ths of cosm...
International audienceDusty galaxies at z similar to 2 span a wide range of relative brightness betw...
Connecting the observed rest-ultraviolet (UV) luminosities of high-z galaxies to their intrinsic lum...
Context. Luminous InfraRed Galaxies (LIRGs) are particularly important for studying the build-up of ...
36 pages, 12 figures, 1 table. Accepted for publication on ApJ Main Journal (scheduled for the ApJ 2...
Aims.We investigate the role of the luminous infrared galaxy (LIRG) and ultra-luminous infrared gala...
We select far-infrared (FIR: 60 μm) and far-ultraviolet (FUV: 530 Å) samples of nearby galaxies in o...
We select far-infrared (FIR-60 microns) and far-ultraviolet (FUV-1530 A) samples of nearby galaxies ...
The TIR and FUV luminosity functions of galaxies and the related luminosity densities rho(TIR) and r...
Aims. We want to study the IR (>$8\;\mu$m) emission of galaxies selected on the basis of their rest...
The ratio between far-ultraviolet (FUV) and infrared (IR) luminosity densities from z=0 to z=1 is di...
5 pages, 3 figures, accepted for publication in A&A LettersThe ratio between far-ultraviolet (FUV) a...
International audienceWe take advantage of the sensitivity and resolution of the Herschel Space Obse...
International audienceWe take advantage of the sensitivity and resolution of the Herschel Space Obse...
We analyze the dust attenuation properties of a volume-limited, optically selected sample of normal ...
Aims. We derive the evolution of the infrared luminosity function (LF) over the last 4/5ths of cosm...
International audienceDusty galaxies at z similar to 2 span a wide range of relative brightness betw...
Connecting the observed rest-ultraviolet (UV) luminosities of high-z galaxies to their intrinsic lum...
Context. Luminous InfraRed Galaxies (LIRGs) are particularly important for studying the build-up of ...
36 pages, 12 figures, 1 table. Accepted for publication on ApJ Main Journal (scheduled for the ApJ 2...
Aims.We investigate the role of the luminous infrared galaxy (LIRG) and ultra-luminous infrared gala...
We select far-infrared (FIR: 60 μm) and far-ultraviolet (FUV: 530 Å) samples of nearby galaxies in o...
We select far-infrared (FIR-60 microns) and far-ultraviolet (FUV-1530 A) samples of nearby galaxies ...