A 1200 micron MAMBO Survey of the ELAIS N2 and Lockman Hole East Fields
Using the MPIfR Max Planck Millimeter Bolometer array (MAMBO) on the IRAM 30m Telescope we have mapped the ELAIS N2
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A gravitational lens survey with Planck Surveyor
The Planck Surveyor cosmic microwave background (CMB) imaging mission will make very sensitive maps of the whole sky at microwave,
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A Submillimetre Survey of the Hubble Deep Field: Unveiling Dust-Enshrouded Star Formation in the Early Universe
The advent of sensitive sub-mm array cameras now allows a proper census of dust-enshrouded massive star-formation in very distant galaxies,
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A Submm View of the Universe: Clues to the Formation of Massive Galaxies
We discuss recent advances in the study of dusty, massive galaxies at z>1 arising from the first extensive spectroscopic surveys.
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Confusion noise in millimetre/submillimetre surveys
The flux density from undetected sources in the observing beam of a telescope produces source confusion noise in the resulting
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Dust temperature and the submillimeter-radio flux density ratio as a redshift indicator
It is difficult to identify the distant galaxies selected in existing submillimeter (submm)-wave surveys, because their positional accuracy is only
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Future millimeter, submillimeter and far-infrared surveys and their successful follow up
The first unbiased surveys for high-redshift galaxies in the submillimeter (submm) and far-infrared (FIR) wavebands have been made over the
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Galactic morning: the Atacama Large Millimeter Array (ALMA) and the evolution of galaxies
The importance of the Atacama Large Millimeter Array (ALMA) to the study of high-redshift dusty gas-rich galaxies is described. ALMA
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Galaxy counts at 450 and 850 microns
Surveys of the distant Universe have been made using the SCUBA submillimeter(submm)-wave camera at the JCMT. 450- and 850-micron data
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Lensed submillimetre-wave foregrounds and the CMBR
Samples of high-redshift galaxies are easy to select in the millimetre/submillimetre (mm/submm) waveband using sensitive telescopes, because their flux density-redshift
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Probing the Invisible Universe: The Case for Far-IR/Submillimeter Interferometry
The question "How did we get here and what will the future bring?" captures the human imagination and the attention
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Prospects for future far-infrared/submillimeter studies of the high-redshift Universe
Observations made using COBE, SCUBA, ISO and MAMBO have provided a reasonable working knowledge of both the intensity of the
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SCUBA's first-born: SMM J02399-0136
We discuss observations of the submm-selected galaxy, SMM J02399-0136, and what has been learnt about it during the year following
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Searching for gravitational lenses in the distant universe
The ESA cornerstone mission The Far-Infrared and Submillimetre Sapce Telescope (FIRST) has the ideal combination of sensitivity and angular resolving
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Submillimeter-selected galaxies
The first generation of submillimeter(submm)-wave surveys are being carried out using the 450/850-micron SCUBA camera at the JCMT on Mauna
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Submillimetre-wave surveys: first results and prospects
The population of distant dusty submm-luminous galaxies was first detected last year (Smail, Ivison and Blain 1997). Forms of evolution
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Submm Continuum Surveys for Obscured Galaxies
We discuss deep surveys in the submm regime using the SCUBA bolometer array on the JCMT. At 850um SCUBA has
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The differential magnification of high-redshift ultraluminous infrared galaxies
A class of extremely luminous high-redshift galaxies has recently been detected in unbiased submillimetre-wave surveys using the Submillimetre Common-User Bolometer
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The history of starburst galaxies
Dusty galaxies with luminosities in excess of 10^11 solar luminosities have been detected out to redshifts of about unity by
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The spectroscopic redshifts of SCUBA galaxies: implications for spheroid formation
We present spectroscopic identifications for a sample of 55 submillimeter(submm)-selected `SCUBA' galaxies, lying at redshifts z=0.7 to 3.7, that were
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