Add to ORKGWe present the rest-frame optical and infrared colours of a complete sample of 1114 z<0.3 galaxies from the Spitzer Wide-area InfraRed Extragalactic Legacy Survey (SWIRE) and the Sloan Digital Sky Survey (SDSS). We discuss the optical and infrared colours of our sample and analyse in detail the contribution of dusty star-forming galaxies and AGN to optically selected red sequence galaxies. We propose that the optical (g-r) colour and infrared log(L_{24}/L_{3.6}) colour of galaxies in our sample are determined primarily by a bulge-to-disk ratio. The (g-r) colour is found to be sensitive to the bulge-to-disk ratio for disk-dominated galaxies, whereas the log(L_{24}/L_{3.6}) colour is more sensitive for bulge-dominated systems. We identify ~18...
We describe the infrared properties of a large sample of early-type galaxies, comparing data from th...
We describe the infrared properties of a large sample of early-type galaxies, comparing data from th...
Searching for active galactic nuclei (AGNs) in dwarf galaxies is important for our understanding of ...
We present the rest-frame optical and infrared colours of a complete sample of 1114 z < 0.3 galaxies...
We present color-magnitude and morphological analysis of 54 low-redshift ultraluminous infrared gala...
We present color-magnitude and morphological analysis of 54 low-redshift ultraluminous infrared gala...
We present color-magnitude and morphological analysis of 54 low-redshift ultraluminous infrared gala...
International audienceWe use empirical techniques to interpret the near-infrared (near-IR) colours o...
We characterize the Spitzer Wide-area Infrared Extragalactic Legacy Survey (SWIRE) galaxy population...
We present color-magnitude and morphological analysis of 54 low-redshift ultraluminous infrared gala...
We present color-magnitude and morphological analysis of 54 low-redshift ultraluminous infrared gala...
We discuss spectral energy distributions, photometric redshifts, redshift distributions, luminosity ...
We use empirical techniques to interpret the near-infrared (near-IR) colours of a sample of 5800 gal...
Covering ~49 square degrees in 6 separate fields, the Spitzer Wide-area InfraRed Extragalactic (SWIR...
The faint stellar halos of galaxies contain key information about the oldest stars and the process o...
We describe the infrared properties of a large sample of early-type galaxies, comparing data from th...
We describe the infrared properties of a large sample of early-type galaxies, comparing data from th...
Searching for active galactic nuclei (AGNs) in dwarf galaxies is important for our understanding of ...
We present the rest-frame optical and infrared colours of a complete sample of 1114 z < 0.3 galaxies...
We present color-magnitude and morphological analysis of 54 low-redshift ultraluminous infrared gala...
We present color-magnitude and morphological analysis of 54 low-redshift ultraluminous infrared gala...
We present color-magnitude and morphological analysis of 54 low-redshift ultraluminous infrared gala...
International audienceWe use empirical techniques to interpret the near-infrared (near-IR) colours o...
We characterize the Spitzer Wide-area Infrared Extragalactic Legacy Survey (SWIRE) galaxy population...
We present color-magnitude and morphological analysis of 54 low-redshift ultraluminous infrared gala...
We present color-magnitude and morphological analysis of 54 low-redshift ultraluminous infrared gala...
We discuss spectral energy distributions, photometric redshifts, redshift distributions, luminosity ...
We use empirical techniques to interpret the near-infrared (near-IR) colours of a sample of 5800 gal...
Covering ~49 square degrees in 6 separate fields, the Spitzer Wide-area InfraRed Extragalactic (SWIR...
The faint stellar halos of galaxies contain key information about the oldest stars and the process o...
We describe the infrared properties of a large sample of early-type galaxies, comparing data from th...
We describe the infrared properties of a large sample of early-type galaxies, comparing data from th...
Searching for active galactic nuclei (AGNs) in dwarf galaxies is important for our understanding of ...