The extended counterpart of submm source Lockman 850.1

Lutz, D.; Dunlop, J.S.; Almaini, O.; Andreani, P.; Blain, A.; Efstathiou, A.; Fox, M.; Genzel, R.; Hasinger, G.; Hughes, D.; Ivison, R.J.; Lawrence, A.; Mann, R.G.; Oliver, S.; Peacock, J.A.; Rigopoulou, D.; Rowan-Robinson, M.; Scott, S.; Serjeant, S. and Tacconi, L. (2001). The extended counterpart of submm source Lockman 850.1. Astronomy and Astrophysics, 378 pp. 70–75.

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URL:	http://arxiv.org/abs/astro-ph/0108131
DOI (Digital Object Identifier) Link:	http://dx.doi.org/doi:10.1051/0004-6361:20011120
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Abstract

The IRAM Plateau de Bure mm interferometer and deep K-band imaging have been used to identify the brightest submm source detected in the Lockman field of the UK 8 mJy SCUBA survey. The near infrared counterpart is an extended (20-30 kpc), clumpy, and extremely red object. The spectral energy distribution suggests it to be a dusty star forming object at a redshift of about 3 (2-4). Its star formation rate and near-infrared properties are consistent with Lockman 850.1 being a massive elliptical in formation. Based on Observations carried out with the IRAM Plateau de Bure Interferometer. IRAM is supported by INSU/CNRS (France), MPG (Germany) and ING (Spain).

Item Type:	Journal Article
ISSN:	1432-0746
Extra Information:	Some of the symbols may not have transferred correctly into this bibliographic record and/or abstract. Article published by EDP Sciences and available at http://www.edpsciences.org/aa or http://dx.doi.org/10.1051/0004-6361:20011120
Keywords:	galaxies; Lockman 850.1
Academic Unit/Department:	Science > Physical Sciences
Interdisciplinary Research Centre:	Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)
Item ID:	5812
Depositing User:	Users 13 not found.
Date Deposited:	07 Nov 2006
Last Modified:	14 Feb 2012 05:05
URI:	http://oro.open.ac.uk/id/eprint/5812

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