The submillimetre properties of ultraluminous infrared galaxies
Open Access
- 8 March 2010
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 403 (1) , 274-286
- https://doi.org/10.1111/j.1365-2966.2009.16064.x
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This publication has 43 references indexed in Scilit:
- The SCUBA Half-Degree Extragalactic Survey (SHADES) – VIII. The nature of faint submillimetre galaxies in SHADES, SWIRE and SXDF surveysMonthly Notices of the Royal Astronomical Society, 2008
- The SCUBA HAlf Degree Extragalactic Survey – VI. 350-μm mapping of submillimetre galaxiesMonthly Notices of the Royal Astronomical Society, 2008
- The Spectral Energy Distribution of Dust Emission in the Edge‐on Spiral Galaxy NGC 4631 as Seen withSpitzerand the James Clerk Maxwell TelescopeThe Astrophysical Journal, 2006
- Cold dust in (some) high-z supernova host galaxiesMonthly Notices of the Royal Astronomical Society, 2005
- A Redshift Survey of the Submillimeter Galaxy PopulationThe Astrophysical Journal, 2005
- Kinematics of Low‐zUltraluminous Infrared Galaxies and Implications for Dynamical Mass Derivations in High‐zStar‐forming GalaxiesThe Astrophysical Journal, 2005
- Optical imaging of ultraluminous IRAS galaxies: how many are mergers?Monthly Notices of the Royal Astronomical Society, 1996
- Submillimetre observations of galaxies – I. First resultsMonthly Notices of the Royal Astronomical Society, 1993
- Fueling starburst galaxies with gas-rich mergersThe Astrophysical Journal, 1991
- On the simultaneous analysis of several complete samples - The V/Vmax and Ve/Va variables, with applications to quasarsThe Astrophysical Journal, 1980