A broad-band spectroscopic search for CO line emission in HDF850.1: the brightest submillimetre object in the Hubble Deep Field-North
Authors:
- J. WaggJWJ. Wagg
- D. H. HughesDHD. H. Hughes
- I. AretxagaIAI. Aretxaga
- E. L. ChapinECE. L. Chapin
- J. S. DunlopJDJ. S. Dunlop
- E. GaztanagaE. Gaztanaga
- M. DevlinMDM. Devlin
Open Access
- 21 February 2007
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 375 (2) , 745-752
Abstract
No abstract availableKeywords
All Related Versions
This publication has 57 references indexed in Scilit:
- Confirmation of the effectiveness of submm source redshift estimation based on rest-frame radio-FIR photometryMonthly Notices of the Royal Astronomical Society, 2005
- The Hubble Deep Field North SCUBA Super-map - I. Submillimetre maps, sources and number countsMonthly Notices of the Royal Astronomical Society, 2003
- Breaking the ‘redshift deadlock’- II. The redshift distribution for the submillimetre population of galaxiesMonthly Notices of the Royal Astronomical Society, 2003
- A median redshift of 2.4 for galaxies bright at submillimetre wavelengthsNature, 2003
- The Properties of Microjansky Radio Sources in the Hubble Deep Field–North, SSA 13, and SSA 22 FieldsThe Astrophysical Journal, 2003
- Submillimeter galaxiesPhysics Reports, 2002
- The Scatter in the Relationship between Redshift and the Radio‐to‐Submillimeter Spectral IndexThe Astrophysical Journal, 2000
- Resolving the Submillimeter Background: The 850 Micron Galaxy CountsThe Astrophysical Journal, 1999
- The Radio-to-Submillimeter Spectral Index as a Redshift IndicatorThe Astrophysical Journal, 1999
- Submillimetre-wavelength detection of dusty star-forming galaxies at high redshiftNature, 1998