The extended counterpart of submm source Lockman 850.1

D  Lutz; J S  Dunlop; O  Almaini; P  Andreani; A  Blain; A  Efstathiou; M  Fox; R  Genzel; G  Hasinger; D  Hughes; R J  Ivison; A  Lawrence; R G  Mann; S  Oliver; J A  Peacock; D  Rigopoulou; M  Rowan-Robinson; S  Scott; S  Serjeant; L  Tacconi

doi:10.1051/0004-6361:20011120

The extended counterpart of submm source Lockman 850.1

D Lutz, J S Dunlop, O Almaini, P Andreani, A Blain, A Efstathiou, M Fox, R Genzel, G Hasinger, D Hughes, R J Ivison, A Lawrence, R G Mann, S Oliver, J A Peacock, D Rigopoulou, M Rowan-Robinson, S Scott, S Serjeant, L Tacconi

School of Physics and Astronomy

Research output: Contribution to journal › Article › peer-review

Abstract / Description of output

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.

Original language	English
Pages (from-to)	70-75
Number of pages	6
Journal	Astronomy & Astrophysics
Volume	378
Issue number	1
DOIs	https://doi.org/10.1051/0004-6361:20011120
Publication status	Published - Oct 2001

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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., & Tacconi, L. (2001). The extended counterpart of submm source Lockman 850.1. Astronomy & Astrophysics, 378(1), 70-75. https://doi.org/10.1051/0004-6361:20011120

@article{b3466f67685b44919ed9348975d6ab8e,

title = "The extended counterpart of submm source Lockman 850.1",

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.",

author = "D Lutz and Dunlop, {J S} and O Almaini and P Andreani and A Blain and A Efstathiou and M Fox and R Genzel and G Hasinger and D Hughes and Ivison, {R J} and A Lawrence and Mann, {R G} and S Oliver and Peacock, {J A} and D Rigopoulou and M Rowan-Robinson and S Scott and S Serjeant and L Tacconi",

year = "2001",

month = oct,

doi = "10.1051/0004-6361:20011120",

language = "English",

volume = "378",

pages = "70--75",

journal = "Astronomy & Astrophysics",

issn = "1432-0746",

publisher = "EDP Sciences",

number = "1",

}

Lutz, D, Dunlop, JS, Almaini, O, Andreani, P, Blain, A, Efstathiou, A, Fox, M, Genzel, R, Hasinger, G, Hughes, D, Ivison, RJ, Lawrence, A , Mann, RG, Oliver, S, Peacock, JA, Rigopoulou, D, Rowan-Robinson, M, Scott, S, Serjeant, S & Tacconi, L 2001, 'The extended counterpart of submm source Lockman 850.1', Astronomy & Astrophysics, vol. 378, no. 1, pp. 70-75. https://doi.org/10.1051/0004-6361:20011120

TY - JOUR

T1 - The extended counterpart of submm source Lockman 850.1

AU - Lutz, D

AU - Dunlop, J S

AU - Almaini, O

AU - Andreani, P

AU - Blain, A

AU - Efstathiou, A

AU - Fox, M

AU - Genzel, R

AU - Hasinger, G

AU - Hughes, D

AU - Ivison, R J

AU - Lawrence, A

AU - Mann, R G

AU - Oliver, S

AU - Peacock, J A

AU - Rigopoulou, D

AU - Rowan-Robinson, M

AU - Scott, S

AU - Serjeant, S

AU - Tacconi, L

PY - 2001/10

Y1 - 2001/10

N2 - 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.

AB - 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.

U2 - 10.1051/0004-6361:20011120

DO - 10.1051/0004-6361:20011120

M3 - Article

SN - 1432-0746

VL - 378

SP - 70

EP - 75

JO - Astronomy & Astrophysics

JF - Astronomy & Astrophysics

IS - 1

ER -

The extended counterpart of submm source Lockman 850.1

Abstract / Description of output

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