Proposed identification of Hubble Deep Field submillimeter source HDF 850.1

D. Downes; R. Neri; A. Greve; S. Guilloteau; F. Casoli; D. Hughes; D. Lutz; K. M. Menten; D. J. Wilner; P. Andreani; F. Bertoldi; C. L. Carilli; J. Dunlop; R. Genzel; F. Gueth; R. J. Ivison; R. G. Mann; Y. Mellier; S. Oliver; J. Peacock; D. Rigopoulou; M. Rowan-Robinson; P. Schilke; S. Serjeant; L. J. Tacconi; M. Wright

Proposed identification of Hubble Deep Field submillimeter source HDF 850.1

D. Downes, R. Neri, A. Greve, S. Guilloteau, F. Casoli, D. Hughes, D. Lutz, K. M. Menten, D. J. Wilner, P. Andreani, F. Bertoldi, C. L. Carilli, J. Dunlop, R. Genzel, F. Gueth, R. J. Ivison, R. G. Mann, Y. Mellier, S. Oliver, J. PeacockD. Rigopoulou, M. Rowan-Robinson, P. Schilke, S. Serjeant, L. J. Tacconi, M. Wright

School of Physics and Astronomy

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Abstract / Description of output

The IRAM Interferometer has been used to detect the submillimeter source HDF 850.1 found by Hughes et al. (1998) in the Hubble Deep Field. The flux density measured at 1.3 mm (236 GHz) is 2.2+/- 0.3 (1sigma ) mJy, in agreement with the flux density measured at the JCMT. The flux densities and upper limits measured at 3.4, 2.8, 1.3, 0.85, and 0.45 mm show that the emission comes from dust. We suggest that the 1.3 mm dust source is associated with the optical arc-like feature, 3-593.0, that has a photometric redshift z~ 1.7. If the HDF 850.1 is at this redshift and unlensed, its spectral energy distribution, combined with that of 3-593.0, matches closely that of the ultraluminous galaxy VII Zw 31. Another possibility is that the dust source may be gravitationally lensed by the elliptical galaxy 3-586.0 at z~ 1. The position of the dust source agrees within the errors with that of the tentative VLA radio source 3651+1226.

Original language	English
Pages (from-to)	809-820
Journal	Astronomy & Astrophysics
Volume	347
Publication status	Published - 1 Jul 1999

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http://adsabs.harvard.edu/abs/1999A%26A...347..809D

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Downes, D., Neri, R., Greve, A., Guilloteau, S., Casoli, F., Hughes, D., Lutz, D., Menten, K. M., Wilner, D. J., Andreani, P., Bertoldi, F., Carilli, C. L., Dunlop, J., Genzel, R., Gueth, F., Ivison, R. J., Mann, R. G., Mellier, Y., Oliver, S., ... Wright, M. (1999). Proposed identification of Hubble Deep Field submillimeter source HDF 850.1. Astronomy & Astrophysics, 347, 809-820. http://adsabs.harvard.edu/abs/1999A%26A...347..809D

@article{5afc01fc119c4ab1b08c6285b1a6ac9b,

title = "Proposed identification of Hubble Deep Field submillimeter source HDF 850.1",

abstract = "The IRAM Interferometer has been used to detect the submillimeter source HDF 850.1 found by Hughes et al. (1998) in the Hubble Deep Field. The flux density measured at 1.3 mm (236 GHz) is 2.2+/- 0.3 (1sigma ) mJy, in agreement with the flux density measured at the JCMT. The flux densities and upper limits measured at 3.4, 2.8, 1.3, 0.85, and 0.45 mm show that the emission comes from dust. We suggest that the 1.3 mm dust source is associated with the optical arc-like feature, 3-593.0, that has a photometric redshift z~ 1.7. If the HDF 850.1 is at this redshift and unlensed, its spectral energy distribution, combined with that of 3-593.0, matches closely that of the ultraluminous galaxy VII Zw 31. Another possibility is that the dust source may be gravitationally lensed by the elliptical galaxy 3-586.0 at z~ 1. The position of the dust source agrees within the errors with that of the tentative VLA radio source 3651+1226.",

author = "D. Downes and R. Neri and A. Greve and S. Guilloteau and F. Casoli and D. Hughes and D. Lutz and Menten, {K. M.} and Wilner, {D. J.} and P. Andreani and F. Bertoldi and Carilli, {C. L.} and J. Dunlop and R. Genzel and F. Gueth and Ivison, {R. J.} and Mann, {R. G.} and Y. Mellier and S. Oliver and J. Peacock and D. Rigopoulou and M. Rowan-Robinson and P. Schilke and S. Serjeant and Tacconi, {L. J.} and M. Wright",

year = "1999",

month = jul,

day = "1",

language = "English",

volume = "347",

pages = "809--820",

journal = "Astronomy & Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

}

Downes, D, Neri, R, Greve, A, Guilloteau, S, Casoli, F, Hughes, D, Lutz, D, Menten, KM, Wilner, DJ, Andreani, P, Bertoldi, F, Carilli, CL, Dunlop, J, Genzel, R, Gueth, F, Ivison, RJ, Mann, RG, Mellier, Y, Oliver, S, Peacock, J, Rigopoulou, D, Rowan-Robinson, M, Schilke, P, Serjeant, S, Tacconi, LJ & Wright, M 1999, 'Proposed identification of Hubble Deep Field submillimeter source HDF 850.1', Astronomy & Astrophysics, vol. 347, pp. 809-820. <http://adsabs.harvard.edu/abs/1999A%26A...347..809D>

TY - JOUR

T1 - Proposed identification of Hubble Deep Field submillimeter source HDF 850.1

AU - Downes, D.

AU - Neri, R.

AU - Greve, A.

AU - Guilloteau, S.

AU - Casoli, F.

AU - Hughes, D.

AU - Lutz, D.

AU - Menten, K. M.

AU - Wilner, D. J.

AU - Andreani, P.

AU - Bertoldi, F.

AU - Carilli, C. L.

AU - Dunlop, J.

AU - Genzel, R.

AU - Gueth, F.

AU - Ivison, R. J.

AU - Mann, R. G.

AU - Mellier, Y.

AU - Oliver, S.

AU - Peacock, J.

AU - Rigopoulou, D.

AU - Rowan-Robinson, M.

AU - Schilke, P.

AU - Serjeant, S.

AU - Tacconi, L. J.

AU - Wright, M.

PY - 1999/7/1

Y1 - 1999/7/1

N2 - The IRAM Interferometer has been used to detect the submillimeter source HDF 850.1 found by Hughes et al. (1998) in the Hubble Deep Field. The flux density measured at 1.3 mm (236 GHz) is 2.2+/- 0.3 (1sigma ) mJy, in agreement with the flux density measured at the JCMT. The flux densities and upper limits measured at 3.4, 2.8, 1.3, 0.85, and 0.45 mm show that the emission comes from dust. We suggest that the 1.3 mm dust source is associated with the optical arc-like feature, 3-593.0, that has a photometric redshift z~ 1.7. If the HDF 850.1 is at this redshift and unlensed, its spectral energy distribution, combined with that of 3-593.0, matches closely that of the ultraluminous galaxy VII Zw 31. Another possibility is that the dust source may be gravitationally lensed by the elliptical galaxy 3-586.0 at z~ 1. The position of the dust source agrees within the errors with that of the tentative VLA radio source 3651+1226.

AB - The IRAM Interferometer has been used to detect the submillimeter source HDF 850.1 found by Hughes et al. (1998) in the Hubble Deep Field. The flux density measured at 1.3 mm (236 GHz) is 2.2+/- 0.3 (1sigma ) mJy, in agreement with the flux density measured at the JCMT. The flux densities and upper limits measured at 3.4, 2.8, 1.3, 0.85, and 0.45 mm show that the emission comes from dust. We suggest that the 1.3 mm dust source is associated with the optical arc-like feature, 3-593.0, that has a photometric redshift z~ 1.7. If the HDF 850.1 is at this redshift and unlensed, its spectral energy distribution, combined with that of 3-593.0, matches closely that of the ultraluminous galaxy VII Zw 31. Another possibility is that the dust source may be gravitationally lensed by the elliptical galaxy 3-586.0 at z~ 1. The position of the dust source agrees within the errors with that of the tentative VLA radio source 3651+1226.

M3 - Article

SN - 0004-6361

VL - 347

SP - 809

EP - 820

JO - Astronomy & Astrophysics

JF - Astronomy & Astrophysics

ER -

Proposed identification of Hubble Deep Field submillimeter source HDF 850.1

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