Add to ORKGWe discuss results from sensitive, wide-field imaging of the millimeter extragalactic background using the Max-Planck Millimeter Bolometer array (MAMBO) at the IRAM 30m telescope
Direct submm imaging has recently revealed the 850-micron background to be mostly composed of a popu...
A systematic survey measuring the submillimetre continuum luminosity in radio galaxies between redsh...
This thesis investigates the emission of sub-millimetre-wave radiation from galaxies in the Hubble ...
The inner 20 × 20 arcmin^2 of the COSMOS field was imaged at 250 GHz (1.2 mm) to an rms noise level ...
The definitive version is available at www.blackwell-synergy.com '.--Copyright Blackwell Publishing....
The inner 20×20 arcmin2 of the COSMOS field was imaged at 250 GHz (1.2 mm) to an rms noise level of ...
We discuss results from sensitive, wide-field imaging of the millimeter extragalactic background usi...
We review published deep surveys in the submillimeter (sub-mm) regime from the new Sub-millimetre Co...
We present a study of the cosmic infrared background, which is a measure of the dust-obscured activi...
Deep surveys at 850microns from Mauna Kea using the SCUBA camera on the JCMT appear to have discover...
The SCUBA submillimetre camera has opened up new possibilities for tracing the evolution of active s...
We present a study of the cosmic infrared background, which is a measure of the dust obscured activi...
I briefly describe some results about luminous distant dusty galaxies obtained in the 5 years since ...
Determination of the epoch dependent star-formation rate of field galaxies is one of the principal g...
The strength of the submillimeter background light shows directly that much of the energy radiated b...
Direct submm imaging has recently revealed the 850-micron background to be mostly composed of a popu...
A systematic survey measuring the submillimetre continuum luminosity in radio galaxies between redsh...
This thesis investigates the emission of sub-millimetre-wave radiation from galaxies in the Hubble ...
The inner 20 × 20 arcmin^2 of the COSMOS field was imaged at 250 GHz (1.2 mm) to an rms noise level ...
The definitive version is available at www.blackwell-synergy.com '.--Copyright Blackwell Publishing....
The inner 20×20 arcmin2 of the COSMOS field was imaged at 250 GHz (1.2 mm) to an rms noise level of ...
We discuss results from sensitive, wide-field imaging of the millimeter extragalactic background usi...
We review published deep surveys in the submillimeter (sub-mm) regime from the new Sub-millimetre Co...
We present a study of the cosmic infrared background, which is a measure of the dust-obscured activi...
Deep surveys at 850microns from Mauna Kea using the SCUBA camera on the JCMT appear to have discover...
The SCUBA submillimetre camera has opened up new possibilities for tracing the evolution of active s...
We present a study of the cosmic infrared background, which is a measure of the dust obscured activi...
I briefly describe some results about luminous distant dusty galaxies obtained in the 5 years since ...
Determination of the epoch dependent star-formation rate of field galaxies is one of the principal g...
The strength of the submillimeter background light shows directly that much of the energy radiated b...
Direct submm imaging has recently revealed the 850-micron background to be mostly composed of a popu...
A systematic survey measuring the submillimetre continuum luminosity in radio galaxies between redsh...
This thesis investigates the emission of sub-millimetre-wave radiation from galaxies in the Hubble ...