Submillimetre and far-infrared spectral energy distributions of galaxies: the luminosity-temperature relation and consequences for photometric redshifts
Open Access
- 1 January 2003
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 338 (3), 733-744
- https://doi.org/10.1046/j.1365-8711.2003.06086.x
Abstract
No abstract availableOther Versions
This publication has 43 references indexed in Scilit:
- Submillimeter galaxiesPhysics Reports, 2002
- A 250 GHz Survey of High‐Redshift Quasars from the Sloan Digital Sky SurveyThe Astrophysical Journal, 2001
- Millimetre/submillimetre-wave emission-line searches for high-redshift galaxiesMonthly Notices of the Royal Astronomical Society, 2000
- 350 Micron Dust Emission from High-Redshift ObjectsThe Astrophysical Journal, 1999
- The differential magnification of high-redshift ultraluminous infrared galaxiesMonthly Notices of the Royal Astronomical Society, 1999
- The Radio-to-Submillimeter Spectral Index as a Redshift IndicatorThe Astrophysical Journal, 1999
- The history of star formation in dusty galaxiesMonthly Notices of the Royal Astronomical Society, 1999
- Deep Submillimeter Images of NGC 891—Cold Dust at Larger Galactic RadiiThe Astrophysical Journal, 1998
- The Planck Surveyor mission and gravitational lensesMonthly Notices of the Royal Astronomical Society, 1998
- The FIRST Survey: Faint Images of the Radio Sky at Twenty CentimetersThe Astrophysical Journal, 1995