ISO observations of faint radio sources

José Afonso; Bahram Mobasher; Antonis Georgakakis; Lawrence Cram; Andrew Hopkins

doi:10.1023/A:1012727301274

ISO observations of faint radio sources

José Afonso^*, Bahram Mobasher, Antonis Georgakakis, Lawrence Cram, Andrew Hopkins

^*Corresponding author for this work

Research output: Contribution to journal › Review article › peer-review

2 Citations (Scopus)

Abstract

Deep radio surveys have revealed, below the millijansky level, a population of actively starforming galaxies, undergoing strong luminosity evolution as found from the observed radio source counts. A random sample of 65 sub-mJy radio sources, selected from the Phoenix Deep Survey, was observed at mid and far-infrared wavelengths using the Infrared Space Observatory. Nine sources were detected at both far-infrared and at least one of the mid-infrared wavelengths. A preliminary analysis of the infrared properties of these faint radio sources is carried out by modeling their infrared Spectral Energy Distribution. The radio vs. far-infrared relation, for these faint radio objects, is also presented.

Original language	English
Pages (from-to)	527-530
Number of pages	4
Journal	Astrophysics and Space Science
Volume	277
Issue number	SUPPL.
DOIs	https://doi.org/10.1023/A:1012727301274
Publication status	Published - 2001
Externally published	Yes

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@article{318553502e52410c83709fbb86332f27,

title = "ISO observations of faint radio sources",

abstract = "Deep radio surveys have revealed, below the millijansky level, a population of actively starforming galaxies, undergoing strong luminosity evolution as found from the observed radio source counts. A random sample of 65 sub-mJy radio sources, selected from the Phoenix Deep Survey, was observed at mid and far-infrared wavelengths using the Infrared Space Observatory. Nine sources were detected at both far-infrared and at least one of the mid-infrared wavelengths. A preliminary analysis of the infrared properties of these faint radio sources is carried out by modeling their infrared Spectral Energy Distribution. The radio vs. far-infrared relation, for these faint radio objects, is also presented.",

keywords = "Galaxies: evolution, Infrared: galaxies, Radio continuum: galaxies, Surveys",

author = "Jos{\'e} Afonso and Bahram Mobasher and Antonis Georgakakis and Lawrence Cram and Andrew Hopkins",

year = "2001",

doi = "10.1023/A:1012727301274",

language = "English",

volume = "277",

pages = "527--530",

journal = "Astrophysics and Space Science",

issn = "0004-640X",

publisher = "Springer Netherlands",

number = "SUPPL.",

}

TY - JOUR

T1 - ISO observations of faint radio sources

AU - Afonso, José

AU - Mobasher, Bahram

AU - Georgakakis, Antonis

AU - Cram, Lawrence

AU - Hopkins, Andrew

PY - 2001

Y1 - 2001

N2 - Deep radio surveys have revealed, below the millijansky level, a population of actively starforming galaxies, undergoing strong luminosity evolution as found from the observed radio source counts. A random sample of 65 sub-mJy radio sources, selected from the Phoenix Deep Survey, was observed at mid and far-infrared wavelengths using the Infrared Space Observatory. Nine sources were detected at both far-infrared and at least one of the mid-infrared wavelengths. A preliminary analysis of the infrared properties of these faint radio sources is carried out by modeling their infrared Spectral Energy Distribution. The radio vs. far-infrared relation, for these faint radio objects, is also presented.

AB - Deep radio surveys have revealed, below the millijansky level, a population of actively starforming galaxies, undergoing strong luminosity evolution as found from the observed radio source counts. A random sample of 65 sub-mJy radio sources, selected from the Phoenix Deep Survey, was observed at mid and far-infrared wavelengths using the Infrared Space Observatory. Nine sources were detected at both far-infrared and at least one of the mid-infrared wavelengths. A preliminary analysis of the infrared properties of these faint radio sources is carried out by modeling their infrared Spectral Energy Distribution. The radio vs. far-infrared relation, for these faint radio objects, is also presented.

KW - Galaxies: evolution

KW - Infrared: galaxies

KW - Radio continuum: galaxies

KW - Surveys

UR - http://www.scopus.com/inward/record.url?scp=0035605536&partnerID=8YFLogxK

U2 - 10.1023/A:1012727301274

DO - 10.1023/A:1012727301274

M3 - Review article

SN - 0004-640X

VL - 277

SP - 527

EP - 530

JO - Astrophysics and Space Science

JF - Astrophysics and Space Science

IS - SUPPL.

ER -

ISO observations of faint radio sources

Abstract

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