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.
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|DOI (Digital Object Identifier) Link:||https://doi.org/10.1051/0004-6361:20011120|
|Google Scholar:||Look up in Google Scholar|
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.
|Item Type:||Journal Article|
|Copyright Holders:||2001 ESO|
|Keywords:||active galaxies; Lockman 850.1; starburst galaxies; infrared|
|Academic Unit/Department:||Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||Users 13 not found.|
|Date Deposited:||07 Nov 2006|
|Last Modified:||06 Oct 2016 05:54|
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