High-z Radio Starbursts Host Obscured X-ray AGN

A M S Richards; R Beswick; S T Garrington; T W B Muxlow; H Thrall; M A Garrett; M Kettenis; H J van Langevelde; E Gonzalez-Solarez; N A Walton; M G Allen; H C Ferguson; B Mobasher; R Norris; J Afonso

High-z Radio Starbursts Host Obscured X-ray AGN

A M S Richards
, R Beswick
, S T Garrington
, T W B Muxlow
, H Thrall
, M A Garrett
, M Kettenis
, H J van Langevelde
, E Gonzalez-Solarez
, N A Walton
, M G Allen
, H C Ferguson
, B Mobasher
, R Norris
, J Afonso (Editor)

Research output: Chapter in Book/Conference proceeding › Conference contribution › peer-review

Abstract

We use Virtual Observatory methods to investigate the association between radio and X-ray emission at high redshifts. Fifty-five of the 92 HDF(N) sources resolved by combining MERLIN+VLA data were detected by Chandra, of which 18 are hard enough and bright enough to be obscured AGN. The high-z population of μJy radio sources is dominated by starbursts an order of magnitude more active and more extended than any found at z

Original language	English
Title of host publication	host publication
Editors	J Afonso
Volume	380
Publication status	Published - 2007
Event	Deepest Astronomical Surveys - Duration: 1 Jan 1824 → … http://adsabs.harvard.edu/abs/2007ASPC..380..291T

Conference

Conference	Deepest Astronomical Surveys
Period	1/01/24 → …
Internet address	http://adsabs.harvard.edu/abs/2007ASPC..380..291T

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Richards, A. M. S., Beswick, R., Garrington, S. T., Muxlow, T. W. B., Thrall, H., Garrett, M. A., Kettenis, M., van Langevelde, H. J., Gonzalez-Solarez, E., Walton, N. A., Allen, M. G., Ferguson, H. C., Mobasher, B., Norris, R., & Afonso, J. (Ed.) (2007). High-z Radio Starbursts Host Obscured X-ray AGN. In J. Afonso (Ed.), host publication (Vol. 380) http://adsabs.harvard.edu/abs/2007ASPC..380..279R

@inproceedings{01adbe9b44994fb2a06b3f040f1e2d79,

title = "High-z Radio Starbursts Host Obscured X-ray AGN",

abstract = "We use Virtual Observatory methods to investigate the association between radio and X-ray emission at high redshifts. Fifty-five of the 92 HDF(N) sources resolved by combining MERLIN+VLA data were detected by Chandra, of which 18 are hard enough and bright enough to be obscured AGN. The high-z population of μJy radio sources is dominated by starbursts an order of magnitude more active and more extended than any found at z",

author = "Richards, \{A M S\} and R Beswick and Garrington, \{S T\} and Muxlow, \{T W B\} and H Thrall and Garrett, \{M A\} and M Kettenis and \{van Langevelde\}, \{H J\} and E Gonzalez-Solarez and Walton, \{N A\} and Allen, \{M G\} and Ferguson, \{H C\} and B Mobasher and R Norris and J Afonso",

year = "2007",

language = "English",

volume = "380",

editor = "J Afonso",

booktitle = "host publication",

note = "Deepest Astronomical Surveys ; Conference date: 01-01-1824",

url = "http://adsabs.harvard.edu/abs/2007ASPC..380..291T",

}

Richards, AMS, Beswick, R, Garrington, ST, Muxlow, TWB, Thrall, H, Garrett, MA, Kettenis, M, van Langevelde, HJ, Gonzalez-Solarez, E, Walton, NA, Allen, MG, Ferguson, HC, Mobasher, B, Norris, R & Afonso, J (ed.) 2007, High-z Radio Starbursts Host Obscured X-ray AGN. in J Afonso (ed.), host publication. vol. 380, Deepest Astronomical Surveys, 1/01/24. <http://adsabs.harvard.edu/abs/2007ASPC..380..279R>

TY - GEN

T1 - High-z Radio Starbursts Host Obscured X-ray AGN

AU - Richards, A M S

AU - Beswick, R

AU - Garrington, S T

AU - Muxlow, T W B

AU - Thrall, H

AU - Garrett, M A

AU - Kettenis, M

AU - van Langevelde, H J

AU - Gonzalez-Solarez, E

AU - Walton, N A

AU - Allen, M G

AU - Ferguson, H C

AU - Mobasher, B

AU - Norris, R

A2 - Afonso, J

PY - 2007

Y1 - 2007

N2 - We use Virtual Observatory methods to investigate the association between radio and X-ray emission at high redshifts. Fifty-five of the 92 HDF(N) sources resolved by combining MERLIN+VLA data were detected by Chandra, of which 18 are hard enough and bright enough to be obscured AGN. The high-z population of μJy radio sources is dominated by starbursts an order of magnitude more active and more extended than any found at z

AB - We use Virtual Observatory methods to investigate the association between radio and X-ray emission at high redshifts. Fifty-five of the 92 HDF(N) sources resolved by combining MERLIN+VLA data were detected by Chandra, of which 18 are hard enough and bright enough to be obscured AGN. The high-z population of μJy radio sources is dominated by starbursts an order of magnitude more active and more extended than any found at z

M3 - Conference contribution

VL - 380

BT - host publication

T2 - Deepest Astronomical Surveys

Y2 - 1 January 1824

ER -

High-z Radio Starbursts Host Obscured X-ray AGN

Abstract

Conference

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