Radio imaging of the Subaru/XMM–NewtonDeep Field– III. Evolution of the radio luminosity function beyond z= 1

C. Simpson; S. Rawlings; R. Ivison; M. Akiyama; O. Almaini; E. Bradshaw; S. Chapman; R. Chuter; S. Croom; J. Dunlop; S. Foucaud; W. Hartley

doi:10.1111/j.1365-2966.2012.20529.x

Radio imaging of the Subaru/XMM–NewtonDeep Field– III. Evolution of the radio luminosity function beyond z= 1

C. Simpson, S. Rawlings, R. Ivison, M. Akiyama, O. Almaini, E. Bradshaw, S. Chapman, R. Chuter, S. Croom, J. Dunlop, S. Foucaud, W. Hartley

School of Physics and Astronomy

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

Abstract

Many of the spectra presented here were obtained as part of the European Southern Observatory (ESO) programme P074.A-0333, undertaken using the Visible Multi-Object Spectrograph (VIMOS) instrument on UT3/Melipal, VIMOS. Several observational campaigns have obtained spectra of objects within the Subaru/XMM-Newton Deep Field (SXDF), and Paper II (Vardoulaki et al., 2008MNRAS.387..505V) presented spectra for 28 of the brightest 37 radio sources, obtained from a variety of sources. The near-infrared data used here come from the third data release (DR3) of the UKIRT (United Kingdom Infrared telescope) Infrared Deep Sky Survey. The optical data in the UDS come from the SXDF, which comprises five separate Suprime-Cam pointings. (1 data file).

Original language	English
Pages (from-to)	3060-3083
Journal	Monthly Notices of the Royal Astronomical Society
Volume	421
Issue number	4
DOIs	https://doi.org/10.1111/j.1365-2966.2012.20529.x
Publication status	Published - 1 Mar 2013

Keywords

Surveys
Radio sources
Active gal. nuclei
Redshifts

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10.1111/j.1365-2966.2012.20529.x

http://adsabs.harvard.edu/abs/2013yCat..74213060S

Cite this

Simpson, C., Rawlings, S., Ivison, R., Akiyama, M., Almaini, O., Bradshaw, E., Chapman, S., Chuter, R., Croom, S., Dunlop, J., Foucaud, S., & Hartley, W. (2013). Radio imaging of the Subaru/XMM–NewtonDeep Field– III. Evolution of the radio luminosity function beyond z= 1. Monthly Notices of the Royal Astronomical Society, 421(4), 3060-3083. https://doi.org/10.1111/j.1365-2966.2012.20529.x

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title = "Radio imaging of the Subaru/XMM–NewtonDeep Field– III. Evolution of the radio luminosity function beyond z= 1",

abstract = "Many of the spectra presented here were obtained as part of the European Southern Observatory (ESO) programme P074.A-0333, undertaken using the Visible Multi-Object Spectrograph (VIMOS) instrument on UT3/Melipal, VIMOS. Several observational campaigns have obtained spectra of objects within the Subaru/XMM-Newton Deep Field (SXDF), and Paper II (Vardoulaki et al., 2008MNRAS.387..505V) presented spectra for 28 of the brightest 37 radio sources, obtained from a variety of sources. The near-infrared data used here come from the third data release (DR3) of the UKIRT (United Kingdom Infrared telescope) Infrared Deep Sky Survey. The optical data in the UDS come from the SXDF, which comprises five separate Suprime-Cam pointings. (1 data file).",

keywords = "Surveys, Radio sources, Active gal. nuclei, Redshifts",

author = "C. Simpson and S. Rawlings and R. Ivison and M. Akiyama and O. Almaini and E. Bradshaw and S. Chapman and R. Chuter and S. Croom and J. Dunlop and S. Foucaud and W. Hartley",

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doi = "10.1111/j.1365-2966.2012.20529.x",

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Simpson, C, Rawlings, S, Ivison, R, Akiyama, M, Almaini, O, Bradshaw, E, Chapman, S, Chuter, R, Croom, S, Dunlop, J, Foucaud, S & Hartley, W 2013, 'Radio imaging of the Subaru/XMM–NewtonDeep Field– III. Evolution of the radio luminosity function beyond z= 1', Monthly Notices of the Royal Astronomical Society, vol. 421, no. 4, pp. 3060-3083. https://doi.org/10.1111/j.1365-2966.2012.20529.x

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T1 - Radio imaging of the Subaru/XMM–NewtonDeep Field– III. Evolution of the radio luminosity function beyond z= 1

AU - Simpson, C.

AU - Rawlings, S.

AU - Ivison, R.

AU - Akiyama, M.

AU - Almaini, O.

AU - Bradshaw, E.

AU - Chapman, S.

AU - Chuter, R.

AU - Croom, S.

AU - Dunlop, J.

AU - Foucaud, S.

AU - Hartley, W.

PY - 2013/3/1

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N2 - Many of the spectra presented here were obtained as part of the European Southern Observatory (ESO) programme P074.A-0333, undertaken using the Visible Multi-Object Spectrograph (VIMOS) instrument on UT3/Melipal, VIMOS. Several observational campaigns have obtained spectra of objects within the Subaru/XMM-Newton Deep Field (SXDF), and Paper II (Vardoulaki et al., 2008MNRAS.387..505V) presented spectra for 28 of the brightest 37 radio sources, obtained from a variety of sources. The near-infrared data used here come from the third data release (DR3) of the UKIRT (United Kingdom Infrared telescope) Infrared Deep Sky Survey. The optical data in the UDS come from the SXDF, which comprises five separate Suprime-Cam pointings. (1 data file).

AB - Many of the spectra presented here were obtained as part of the European Southern Observatory (ESO) programme P074.A-0333, undertaken using the Visible Multi-Object Spectrograph (VIMOS) instrument on UT3/Melipal, VIMOS. Several observational campaigns have obtained spectra of objects within the Subaru/XMM-Newton Deep Field (SXDF), and Paper II (Vardoulaki et al., 2008MNRAS.387..505V) presented spectra for 28 of the brightest 37 radio sources, obtained from a variety of sources. The near-infrared data used here come from the third data release (DR3) of the UKIRT (United Kingdom Infrared telescope) Infrared Deep Sky Survey. The optical data in the UDS come from the SXDF, which comprises five separate Suprime-Cam pointings. (1 data file).

KW - Surveys

KW - Radio sources

KW - Active gal. nuclei

KW - Redshifts

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DO - 10.1111/j.1365-2966.2012.20529.x

M3 - Article

VL - 421

SP - 3060

EP - 3083

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 4

ER -

Radio imaging of the Subaru/XMM–NewtonDeep Field– III. Evolution of the radio luminosity function beyond z= 1

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Keywords

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