We present new deep images of the Coma Cluster from the ESA Herschel Space Observatory at wavelengths of 70, 100 and 160 mu m, covering an area of 1.75 x 1.0 square degrees encompassing the core and south-west infall region. Our data display an excess of sources at flux densities above 100 mJy compared to blank-field surveys, as expected. We use extensive optical spectroscopy of this region to identify cluster members and hence produce cluster luminosity functions in all three photometric bands. We compare our results to the local field galaxy luminosity function, and the luminosity functions from the Herschel Virgo Cluster Survey. We find consistency between the shapes of the Coma and field galaxy luminosity functions at all three waveleng...
We describe a far-infrared survey of the Coma cluster and the galaxy filament it resides within. O...
We describe the Herschel Virgo Cluster Survey and the first data that cover the complete survey are...
International audienceContext: Environmental effects are known to have an important influence on clu...
We present new deep images of the Coma Cluster from the ESA Herschel Space Observatory at wavelength...
We present new deep images of the Coma Cluster from the ESA Herschel Space Observatory at wavelength...
This thesis presents results from the deepest ever far-infrared study of the Coma cluster (Abell 165...
An infrared survey of the central 650 arcmin$^2$ of the Coma cluster is used to determine the $H$ ba...
We describe a far-infrared survey of the Coma cluster and the galaxy filament it resides within. Our...
We present a deep multicolour CCD mosaic of the Coma cluster (Abell 1656), covering 5.2 deg(2) in th...
We describe the Herschel Virgo Cluster Survey (HeViCS) and the first data obtained as part of the sc...
We describe the Herschel Virgo Cluster Survey (HeViCS) and the first data obtained as part of the sc...
We describe the Herschel Virgo Cluster Survey (HeViCS) and the first data obtained as part of the sc...
We describe a far-infrared survey of the Coma cluster and the galaxy filament it resides within. O...
We describe the Herschel Virgo Cluster Survey and the first data that cover the complete survey are...
International audienceContext: Environmental effects are known to have an important influence on clu...
We present new deep images of the Coma Cluster from the ESA Herschel Space Observatory at wavelength...
We present new deep images of the Coma Cluster from the ESA Herschel Space Observatory at wavelength...
This thesis presents results from the deepest ever far-infrared study of the Coma cluster (Abell 165...
An infrared survey of the central 650 arcmin$^2$ of the Coma cluster is used to determine the $H$ ba...
We describe a far-infrared survey of the Coma cluster and the galaxy filament it resides within. Our...
We present a deep multicolour CCD mosaic of the Coma cluster (Abell 1656), covering 5.2 deg(2) in th...
We describe the Herschel Virgo Cluster Survey (HeViCS) and the first data obtained as part of the sc...
We describe the Herschel Virgo Cluster Survey (HeViCS) and the first data obtained as part of the sc...
We describe the Herschel Virgo Cluster Survey (HeViCS) and the first data obtained as part of the sc...
We describe a far-infrared survey of the Coma cluster and the galaxy filament it resides within. O...
We describe the Herschel Virgo Cluster Survey and the first data that cover the complete survey are...
International audienceContext: Environmental effects are known to have an important influence on clu...