University of Hertfordshire

The MWA GLEAM 4Jy Sample; a new large, bright radio source sample at 151 MHz

Research output: Contribution to conferencePaper

Standard

The MWA GLEAM 4Jy Sample; a new large, bright radio source sample at 151 MHz. / Jackson, C A; Franzen, T M O; Seymour, N; White, S V; Murphy, Tara; Sadler, E M; Callingham, J R; Hunstead, R W; Hughes, J; Wall, J V; Bell, M E; Dwarakanath, K S; For, B-Q; Gaensler, B M; Hancock, P J; Hindson, L; Hurley-Walker, N; Johnston-Hollitt, M; Kapinska, A D; Lenc, E; McKinley, B; Morgan, J; Offringa, A R; Procopio, P; Staveley-Smith, L; Wayth, R B; Wu, C; Zheng, Q.

2015. Paper presented at The Many Facests of Extragalactiv Radio Surveys: Towards New Scientific Challenges, Bologne, Italy.

Research output: Contribution to conferencePaper

Harvard

Jackson, CA, Franzen, TMO, Seymour, N, White, SV, Murphy, T, Sadler, EM, Callingham, JR, Hunstead, RW, Hughes, J, Wall, JV, Bell, ME, Dwarakanath, KS, For, B-Q, Gaensler, BM, Hancock, PJ, Hindson, L, Hurley-Walker, N, Johnston-Hollitt, M, Kapinska, AD, Lenc, E, McKinley, B, Morgan, J, Offringa, AR, Procopio, P, Staveley-Smith, L, Wayth, RB, Wu, C & Zheng, Q 2015, 'The MWA GLEAM 4Jy Sample; a new large, bright radio source sample at 151 MHz', Paper presented at The Many Facests of Extragalactiv Radio Surveys: Towards New Scientific Challenges, Bologne, Italy, 20/10/15 - 23/10/15.

APA

Jackson, C. A., Franzen, T. M. O., Seymour, N., White, S. V., Murphy, T., Sadler, E. M., Callingham, J. R., Hunstead, R. W., Hughes, J., Wall, J. V., Bell, M. E., Dwarakanath, K. S., For, B-Q., Gaensler, B. M., Hancock, P. J., Hindson, L., Hurley-Walker, N., Johnston-Hollitt, M., Kapinska, A. D., ... Zheng, Q. (2015). The MWA GLEAM 4Jy Sample; a new large, bright radio source sample at 151 MHz. Paper presented at The Many Facests of Extragalactiv Radio Surveys: Towards New Scientific Challenges, Bologne, Italy.

Vancouver

Jackson CA, Franzen TMO, Seymour N, White SV, Murphy T, Sadler EM et al. The MWA GLEAM 4Jy Sample; a new large, bright radio source sample at 151 MHz. 2015. Paper presented at The Many Facests of Extragalactiv Radio Surveys: Towards New Scientific Challenges, Bologne, Italy.

Author

Jackson, C A ; Franzen, T M O ; Seymour, N ; White, S V ; Murphy, Tara ; Sadler, E M ; Callingham, J R ; Hunstead, R W ; Hughes, J ; Wall, J V ; Bell, M E ; Dwarakanath, K S ; For, B-Q ; Gaensler, B M ; Hancock, P J ; Hindson, L ; Hurley-Walker, N ; Johnston-Hollitt, M ; Kapinska, A D ; Lenc, E ; McKinley, B ; Morgan, J ; Offringa, A R ; Procopio, P ; Staveley-Smith, L ; Wayth, R B ; Wu, C ; Zheng, Q. / The MWA GLEAM 4Jy Sample; a new large, bright radio source sample at 151 MHz. Paper presented at The Many Facests of Extragalactiv Radio Surveys: Towards New Scientific Challenges, Bologne, Italy.

Bibtex

@conference{4793a2583af540cd8c883d3c49e80c74,
title = "The MWA GLEAM 4Jy Sample; a new large, bright radio source sample at 151 MHz",
abstract = "This paper outlines how the new GaLactic and Extragalactic All-sky MWA Survey (GLEAM, Wayth et al. 2015), observed by the Murchison Widefield Array covering the frequency range 72 - 231 MHz, allows identification of a new large, complete, sample of more than 2000 bright extragalactic radio sources selected at 151 MHz. With a flux density limit of 4 Jy this sample is significantly larger than the canonical fully-complete sample, 3CRR (Laing, Riley & Longair 1983). In analysing this small bright subset of the GLEAM survey we are also providing a first user check of the GLEAM catalogue ahead of its public release (Hurley-Walker et al. in prep). Whilst significant work remains to fully characterise our new bright source sample, in time it will provide important constraints to evolutionary behaviour, across a wide redshift and intrinsic radio power range, as well as being highly complementary to results from targeted, small area surveys.",
keywords = "astro-ph.GA, astro-ph.CO",
author = "Jackson, {C A} and Franzen, {T M O} and N Seymour and White, {S V} and Tara Murphy and Sadler, {E M} and Callingham, {J R} and Hunstead, {R W} and J Hughes and Wall, {J V} and Bell, {M E} and Dwarakanath, {K S} and B-Q For and Gaensler, {B M} and Hancock, {P J} and L Hindson and N Hurley-Walker and M Johnston-Hollitt and Kapinska, {A D} and E Lenc and B McKinley and J Morgan and Offringa, {A R} and P Procopio and L Staveley-Smith and Wayth, {R B} and C Wu and Q Zheng",
note = "C.A. Jackson, T.M.O. Franzen, N. Seymour, S.V. White, Tara Murphy, E.M. Sadler, J.R. Callingham, R.W. Hunstead, J. Hughes, J.V. Wall, M.E. Bell, K.S. Dwarakanath, B.Q. For, B.M. Gaensler, P.J. Hancock, L, Hindson, N. Hurley-Walker, M. Johnston-Hollitt, A.D. Kapinska, E. Lenc, B. McKinley, J. Morgan, A.R. Offringa, P. Procopio, L. Staveley-Smith, R.B. Wayth, C. Wu, Q. Zheng, {\textquoteleft}The MWA GLEAM 4Jy Sample; a new large, bright radio source sample at 151 MHz{\textquoteright}, paper presented at The Many Facests of Extragalactiv Radio Surveys: Towards New Scientific Challenges, Bologna, Italy, 20-23 October, 2015. ; The Many Facests of Extragalactiv Radio Surveys: Towards New Scientific Challenges ; Conference date: 20-10-2015 Through 23-10-2015",
year = "2015",
month = oct,
day = "20",
language = "English",

}

RIS

TY - CONF

T1 - The MWA GLEAM 4Jy Sample; a new large, bright radio source sample at 151 MHz

AU - Jackson, C A

AU - Franzen, T M O

AU - Seymour, N

AU - White, S V

AU - Murphy, Tara

AU - Sadler, E M

AU - Callingham, J R

AU - Hunstead, R W

AU - Hughes, J

AU - Wall, J V

AU - Bell, M E

AU - Dwarakanath, K S

AU - For, B-Q

AU - Gaensler, B M

AU - Hancock, P J

AU - Hindson, L

AU - Hurley-Walker, N

AU - Johnston-Hollitt, M

AU - Kapinska, A D

AU - Lenc, E

AU - McKinley, B

AU - Morgan, J

AU - Offringa, A R

AU - Procopio, P

AU - Staveley-Smith, L

AU - Wayth, R B

AU - Wu, C

AU - Zheng, Q

N1 - C.A. Jackson, T.M.O. Franzen, N. Seymour, S.V. White, Tara Murphy, E.M. Sadler, J.R. Callingham, R.W. Hunstead, J. Hughes, J.V. Wall, M.E. Bell, K.S. Dwarakanath, B.Q. For, B.M. Gaensler, P.J. Hancock, L, Hindson, N. Hurley-Walker, M. Johnston-Hollitt, A.D. Kapinska, E. Lenc, B. McKinley, J. Morgan, A.R. Offringa, P. Procopio, L. Staveley-Smith, R.B. Wayth, C. Wu, Q. Zheng, ‘The MWA GLEAM 4Jy Sample; a new large, bright radio source sample at 151 MHz’, paper presented at The Many Facests of Extragalactiv Radio Surveys: Towards New Scientific Challenges, Bologna, Italy, 20-23 October, 2015.

PY - 2015/10/20

Y1 - 2015/10/20

N2 - This paper outlines how the new GaLactic and Extragalactic All-sky MWA Survey (GLEAM, Wayth et al. 2015), observed by the Murchison Widefield Array covering the frequency range 72 - 231 MHz, allows identification of a new large, complete, sample of more than 2000 bright extragalactic radio sources selected at 151 MHz. With a flux density limit of 4 Jy this sample is significantly larger than the canonical fully-complete sample, 3CRR (Laing, Riley & Longair 1983). In analysing this small bright subset of the GLEAM survey we are also providing a first user check of the GLEAM catalogue ahead of its public release (Hurley-Walker et al. in prep). Whilst significant work remains to fully characterise our new bright source sample, in time it will provide important constraints to evolutionary behaviour, across a wide redshift and intrinsic radio power range, as well as being highly complementary to results from targeted, small area surveys.

AB - This paper outlines how the new GaLactic and Extragalactic All-sky MWA Survey (GLEAM, Wayth et al. 2015), observed by the Murchison Widefield Array covering the frequency range 72 - 231 MHz, allows identification of a new large, complete, sample of more than 2000 bright extragalactic radio sources selected at 151 MHz. With a flux density limit of 4 Jy this sample is significantly larger than the canonical fully-complete sample, 3CRR (Laing, Riley & Longair 1983). In analysing this small bright subset of the GLEAM survey we are also providing a first user check of the GLEAM catalogue ahead of its public release (Hurley-Walker et al. in prep). Whilst significant work remains to fully characterise our new bright source sample, in time it will provide important constraints to evolutionary behaviour, across a wide redshift and intrinsic radio power range, as well as being highly complementary to results from targeted, small area surveys.

KW - astro-ph.GA

KW - astro-ph.CO

M3 - Paper

T2 - The Many Facests of Extragalactiv Radio Surveys: Towards New Scientific Challenges

Y2 - 20 October 2015 through 23 October 2015

ER -