International audienceWe present Herschel/PACS 100 and 160 mu m integrated photometry for the 323 galaxies in the Herschel Reference Survey (HRS), a K-band, volume-limited sample of galaxies in the local Universe. Once combined with the Herschel/SPIRE observations already available, these data make the HRS the largest representative sample of nearby galaxies with homogeneous coverage across the 100-500 mu m wavelength range. In this paper, we take advantage of this unique data set to investigate the properties and shape of the far-infrared/submillimetre spectral energy distribution in nearby galaxies. We show that, in the stellar mass range covered by the HRS (8 less than or similar to log (M-*/M-circle dot) less than or similar to 12), the...
New far-infrared and sub-millimeter photometry from the Herschel Space Observatory is presented for ...
We present infrared colours (in the 25-500 mu m spectral range) and UV to radio continuum spectral e...
We study a sample of 61submillimetre galaxies (SMGs) selected from ground-based surveys, with known ...
International audienceWe present Herschel/PACS 100 and 160 mu m integrated photometry for the 323 ga...
We present Herschel/PACS 100 and 160 μm integrated photometry for the 323 galaxies in the Herschel R...
We present Herschel/PACS 100 and 160 mu m integrated photometry for the 323 galaxies in the Herschel...
We study the dust properties of galaxies in the redshift range 0.1 ≲z≲ 2.8 observed by the Herschel ...
We study a sample of 61submillimetre galaxies (SMGs) selected from ground-based surveys, with known ...
We study the far infrared (60-500 mu m) colours of late-type galaxies in the Herschel Reference Surv...
International audienceWe study the far infrared (60-500 mu m) colours of late-type galaxies in the H...
International audienceNew far-infrared and submillimeter photometry from the Herschel Space Observat...
Although it accounts only for a small fraction of the baryonic mass, dust has a profound impact on t...
New far-infrared and sub-millimeter photometry from the Herschel Space Observatory is presented for ...
We present infrared colours (in the 25-500 mu m spectral range) and UV to radio continuum spectral e...
We study a sample of 61submillimetre galaxies (SMGs) selected from ground-based surveys, with known ...
International audienceWe present Herschel/PACS 100 and 160 mu m integrated photometry for the 323 ga...
We present Herschel/PACS 100 and 160 μm integrated photometry for the 323 galaxies in the Herschel R...
We present Herschel/PACS 100 and 160 mu m integrated photometry for the 323 galaxies in the Herschel...
We study the dust properties of galaxies in the redshift range 0.1 ≲z≲ 2.8 observed by the Herschel ...
We study a sample of 61submillimetre galaxies (SMGs) selected from ground-based surveys, with known ...
We study the far infrared (60-500 mu m) colours of late-type galaxies in the Herschel Reference Surv...
International audienceWe study the far infrared (60-500 mu m) colours of late-type galaxies in the H...
International audienceNew far-infrared and submillimeter photometry from the Herschel Space Observat...
Although it accounts only for a small fraction of the baryonic mass, dust has a profound impact on t...
New far-infrared and sub-millimeter photometry from the Herschel Space Observatory is presented for ...
We present infrared colours (in the 25-500 mu m spectral range) and UV to radio continuum spectral e...
We study a sample of 61submillimetre galaxies (SMGs) selected from ground-based surveys, with known ...