Observations of the Hubble Deep Field with the Infrared Space Observatory - IV. Association of sources with Hubble Deep Field galaxies

R. G. Mann; S. J. Oliver; S. B. G. Serjeant; M. Rowan-Robinson; A. Baker; N. Eaton; A. Efstathiou; P. Goldschmidt; B. Mobasher; T. J. Sumner; L. Danese; D. Elbaz; A. Franceschini; E. Egami; M. Kontizas; A. Lawrence; R. McMahon; H. U. Norgaard-Nielsen; I. Perez-Fournon; J. I. Gonzalez-Serrano

doi:10.1093/mnras/289.2.482

Observations of the Hubble Deep Field with the Infrared Space Observatory - IV. Association of sources with Hubble Deep Field galaxies

R. G. Mann, S. J. Oliver, S. B. G. Serjeant, M. Rowan-Robinson, A. Baker, N. Eaton, A. Efstathiou, P. Goldschmidt, B. Mobasher, T. J. Sumner, L. Danese, D. Elbaz, A. Franceschini, E. Egami, M. Kontizas, A. Lawrence, R. McMahon, H. U. Norgaard-Nielsen, I. Perez-Fournon, J. I. Gonzalez-Serrano

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

Abstract / Description of output

We discuss the identification of sources detected by the Infrared Space Observatory (ISO) at 6.7 and 15 μ in the Hubble Deep Field (HDF) region. We conservatively associate ISO sources with objects in existing optical and near-infrared HDF catalogues using the likelihood ratio method, confirming these results (and, in one case, clarifying them) with independent visual searches. We find 15 ISO sources to be reliably associated with bright [I 814(AB) <23] galaxies in the HDF, and one with an I 814(AB)=19.9 star, while a further 11 are associated with objects in the Hubble Flanking Fields (10 galaxies and one star). Amongst optically bright HDF galaxies, ISO tends to detect luminous, star-forming galaxies at fairly high redshift and with disturbed morphologies, in preference to nearby ellipticals.

Original language	English
Pages (from-to)	482-489
Journal	Monthly Notices of the Royal Astronomical Society
Volume	289
Issue number	2
DOIs	https://doi.org/10.1093/mnras/289.2.482
Publication status	Published - 1 Aug 1997

Keywords / Materials (for Non-textual outputs)

STARS: FORMATION
GALAXIES: EVOLUTION
GALAXIES: STARBURST
COSMOLOGY: OBSERVATIONS
INFRARED: GALAXIES

Access to Document

10.1093/mnras/289.2.482

http://adsabs.harvard.edu/abs/1997MNRAS.289..482M

Cite this

Mann, R. G., Oliver, S. J., Serjeant, S. B. G., Rowan-Robinson, M., Baker, A., Eaton, N., Efstathiou, A., Goldschmidt, P., Mobasher, B., Sumner, T. J., Danese, L., Elbaz, D., Franceschini, A., Egami, E., Kontizas, M., Lawrence, A., McMahon, R., Norgaard-Nielsen, H. U., Perez-Fournon, I., & Gonzalez-Serrano, J. I. (1997). Observations of the Hubble Deep Field with the Infrared Space Observatory - IV. Association of sources with Hubble Deep Field galaxies. Monthly Notices of the Royal Astronomical Society, 289(2), 482-489. https://doi.org/10.1093/mnras/289.2.482

@article{b99e4efb75204afbaaaba4462a5abc87,

title = "Observations of the Hubble Deep Field with the Infrared Space Observatory - IV. Association of sources with Hubble Deep Field galaxies",

abstract = "We discuss the identification of sources detected by the Infrared Space Observatory (ISO) at 6.7 and 15 μ in the Hubble Deep Field (HDF) region. We conservatively associate ISO sources with objects in existing optical and near-infrared HDF catalogues using the likelihood ratio method, confirming these results (and, in one case, clarifying them) with independent visual searches. We find 15 ISO sources to be reliably associated with bright [I 814(AB) <23] galaxies in the HDF, and one with an I 814(AB)=19.9 star, while a further 11 are associated with objects in the Hubble Flanking Fields (10 galaxies and one star). Amongst optically bright HDF galaxies, ISO tends to detect luminous, star-forming galaxies at fairly high redshift and with disturbed morphologies, in preference to nearby ellipticals.",

keywords = "STARS: FORMATION, GALAXIES: EVOLUTION, GALAXIES: STARBURST, COSMOLOGY: OBSERVATIONS, INFRARED: GALAXIES",

author = "Mann, {R. G.} and Oliver, {S. J.} and Serjeant, {S. B. G.} and M. Rowan-Robinson and A. Baker and N. Eaton and A. Efstathiou and P. Goldschmidt and B. Mobasher and Sumner, {T. J.} and L. Danese and D. Elbaz and A. Franceschini and E. Egami and M. Kontizas and A. Lawrence and R. McMahon and Norgaard-Nielsen, {H. U.} and I. Perez-Fournon and Gonzalez-Serrano, {J. I.}",

year = "1997",

month = aug,

day = "1",

doi = "10.1093/mnras/289.2.482",

language = "English",

volume = "289",

pages = "482--489",

journal = "Monthly Notices of the Royal Astronomical Society",

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Mann, RG, Oliver, SJ, Serjeant, SBG, Rowan-Robinson, M, Baker, A, Eaton, N, Efstathiou, A, Goldschmidt, P, Mobasher, B, Sumner, TJ, Danese, L, Elbaz, D, Franceschini, A, Egami, E, Kontizas, M, Lawrence, A, McMahon, R, Norgaard-Nielsen, HU, Perez-Fournon, I & Gonzalez-Serrano, JI 1997, 'Observations of the Hubble Deep Field with the Infrared Space Observatory - IV. Association of sources with Hubble Deep Field galaxies', Monthly Notices of the Royal Astronomical Society, vol. 289, no. 2, pp. 482-489. https://doi.org/10.1093/mnras/289.2.482

TY - JOUR

T1 - Observations of the Hubble Deep Field with the Infrared Space Observatory - IV. Association of sources with Hubble Deep Field galaxies

AU - Mann, R. G.

AU - Oliver, S. J.

AU - Serjeant, S. B. G.

AU - Rowan-Robinson, M.

AU - Baker, A.

AU - Eaton, N.

AU - Efstathiou, A.

AU - Goldschmidt, P.

AU - Mobasher, B.

AU - Sumner, T. J.

AU - Danese, L.

AU - Elbaz, D.

AU - Franceschini, A.

AU - Egami, E.

AU - Kontizas, M.

AU - Lawrence, A.

AU - McMahon, R.

AU - Norgaard-Nielsen, H. U.

AU - Perez-Fournon, I.

AU - Gonzalez-Serrano, J. I.

PY - 1997/8/1

Y1 - 1997/8/1

N2 - We discuss the identification of sources detected by the Infrared Space Observatory (ISO) at 6.7 and 15 μ in the Hubble Deep Field (HDF) region. We conservatively associate ISO sources with objects in existing optical and near-infrared HDF catalogues using the likelihood ratio method, confirming these results (and, in one case, clarifying them) with independent visual searches. We find 15 ISO sources to be reliably associated with bright [I 814(AB) <23] galaxies in the HDF, and one with an I 814(AB)=19.9 star, while a further 11 are associated with objects in the Hubble Flanking Fields (10 galaxies and one star). Amongst optically bright HDF galaxies, ISO tends to detect luminous, star-forming galaxies at fairly high redshift and with disturbed morphologies, in preference to nearby ellipticals.

AB - We discuss the identification of sources detected by the Infrared Space Observatory (ISO) at 6.7 and 15 μ in the Hubble Deep Field (HDF) region. We conservatively associate ISO sources with objects in existing optical and near-infrared HDF catalogues using the likelihood ratio method, confirming these results (and, in one case, clarifying them) with independent visual searches. We find 15 ISO sources to be reliably associated with bright [I 814(AB) <23] galaxies in the HDF, and one with an I 814(AB)=19.9 star, while a further 11 are associated with objects in the Hubble Flanking Fields (10 galaxies and one star). Amongst optically bright HDF galaxies, ISO tends to detect luminous, star-forming galaxies at fairly high redshift and with disturbed morphologies, in preference to nearby ellipticals.

KW - STARS: FORMATION

KW - GALAXIES: EVOLUTION

KW - GALAXIES: STARBURST

KW - COSMOLOGY: OBSERVATIONS

KW - INFRARED: GALAXIES

U2 - 10.1093/mnras/289.2.482

DO - 10.1093/mnras/289.2.482

M3 - Article

SN - 0035-8711

VL - 289

SP - 482

EP - 489

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 2

ER -

Observations of the Hubble Deep Field with the Infrared Space Observatory - IV. Association of sources with Hubble Deep Field galaxies

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Keywords / Materials (for Non-textual outputs)

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