Home > Research > Publications & Outputs > The XMM Cluster Survey

Research

Associated organisational units

Links

Text available via DOI:

Keywords

View graph of relations

The XMM Cluster Survey: Testing chameleon gravity using the profiles of clusters

Research output: Contribution to Journal/Magazine › Journal article › peer-review

Published

Standard

The XMM Cluster Survey: Testing chameleon gravity using the profiles of clusters. / Wilcox, Harry; Bacon, David; Nichol, Robert C. et al.
In: Monthly Notices of the Royal Astronomical Society, Vol. 452, No. 2, 14.07.2015, p. 1171-1183.

Research output: Contribution to Journal/Magazine › Journal article › peer-review

Harvard

Wilcox, H, Bacon, D, Nichol, RC, Rooney, PJ, Terukina, A, Romer, AK, Koyama, K, Zhao, G-B, Hood, R, Mann, RG, Hilton, M, Manolopoulou, M, Sahlen, M, Collins, CA, Liddle, AR, Mayers, JA, Mehrtens, N, Miller, CJ, Stott, JP & Viana, PTP 2015, 'The XMM Cluster Survey: Testing chameleon gravity using the profiles of clusters', Monthly Notices of the Royal Astronomical Society, vol. 452, no. 2, pp. 1171-1183. https://doi.org/10.1093/mnras/stv1366

APA

Wilcox, H., Bacon, D., Nichol, R. C., Rooney, P. J., Terukina, A., Romer, A. K., Koyama, K., Zhao, G-B., Hood, R., Mann, R. G., Hilton, M., Manolopoulou, M., Sahlen, M., Collins, C. A., Liddle, A. R., Mayers, J. A., Mehrtens, N., Miller, C. J., Stott, J. P., & Viana, P. T. P. (2015). The XMM Cluster Survey: Testing chameleon gravity using the profiles of clusters. Monthly Notices of the Royal Astronomical Society, 452(2), 1171-1183. https://doi.org/10.1093/mnras/stv1366

Vancouver

Wilcox H, Bacon D, Nichol RC, Rooney PJ, Terukina A, Romer AK et al. The XMM Cluster Survey: Testing chameleon gravity using the profiles of clusters. Monthly Notices of the Royal Astronomical Society. 2015 Jul 14;452(2):1171-1183. doi: 10.1093/mnras/stv1366

Author

Wilcox, Harry ; Bacon, David ; Nichol, Robert C. et al. / The XMM Cluster Survey : Testing chameleon gravity using the profiles of clusters. In: Monthly Notices of the Royal Astronomical Society. 2015 ; Vol. 452, No. 2. pp. 1171-1183.

Bibtex

@article{d197ee6cca7440eea991797aa3af71a0,
title = "The XMM Cluster Survey: Testing chameleon gravity using the profiles of clusters",
abstract = "The chameleon gravity model postulates the existence of a scalar field that couples with matter to mediate a fifth force. If it exists, this fifth force would influence the hot X-ray emitting gas filling the potential wells of galaxy clusters. However, it would not influence the clusters' weak lensing signal. Therefore, by comparing X-ray and weak lensing profiles, one can place upper limits on the strength of a fifth force. This technique has been attempted before using a single, nearby cluster (Coma, $z=0.02$). Here we apply the technique to the stacked profiles of 58 clusters at higher redshifts ($0.1z",
keywords = "astro-ph.CO",
author = "Harry Wilcox and David Bacon and Nichol, {Robert C.} and Rooney, {Philip J.} and Ayumu Terukina and Romer, {A. Kathy} and Kazuya Koyama and Gong-Bo Zhao and Ross Hood and Mann, {Robert G.} and Matt Hilton and Maria Manolopoulou and Martin Sahlen and Collins, {Chris A.} and Liddle, {Andrew R.} and Mayers, {Julian A.} and Nicola Mehrtens and Miller, {Christopher J.} and Stott, {John P.} and Viana, {Pedro T. P.}",
note = "14 pages, 7 figures",
year = "2015",
month = jul,
day = "14",
doi = "10.1093/mnras/stv1366",
language = "English",
volume = "452",
pages = "1171--1183",
journal = "Monthly Notices of the Royal Astronomical Society",
issn = "0035-8711",
publisher = "OXFORD UNIV PRESS",
number = "2",

}

RIS

TY - JOUR

T1 - The XMM Cluster Survey

T2 - Testing chameleon gravity using the profiles of clusters

AU - Wilcox, Harry

AU - Bacon, David

AU - Nichol, Robert C.

AU - Rooney, Philip J.

AU - Terukina, Ayumu

AU - Romer, A. Kathy

AU - Koyama, Kazuya

AU - Zhao, Gong-Bo

AU - Hood, Ross

AU - Mann, Robert G.

AU - Hilton, Matt

AU - Manolopoulou, Maria

AU - Sahlen, Martin

AU - Collins, Chris A.

AU - Liddle, Andrew R.

AU - Mayers, Julian A.

AU - Mehrtens, Nicola

AU - Miller, Christopher J.

AU - Stott, John P.

AU - Viana, Pedro T. P.

N1 - 14 pages, 7 figures

PY - 2015/7/14

Y1 - 2015/7/14

N2 - The chameleon gravity model postulates the existence of a scalar field that couples with matter to mediate a fifth force. If it exists, this fifth force would influence the hot X-ray emitting gas filling the potential wells of galaxy clusters. However, it would not influence the clusters' weak lensing signal. Therefore, by comparing X-ray and weak lensing profiles, one can place upper limits on the strength of a fifth force. This technique has been attempted before using a single, nearby cluster (Coma, $z=0.02$). Here we apply the technique to the stacked profiles of 58 clusters at higher redshifts ($0.1z

AB - The chameleon gravity model postulates the existence of a scalar field that couples with matter to mediate a fifth force. If it exists, this fifth force would influence the hot X-ray emitting gas filling the potential wells of galaxy clusters. However, it would not influence the clusters' weak lensing signal. Therefore, by comparing X-ray and weak lensing profiles, one can place upper limits on the strength of a fifth force. This technique has been attempted before using a single, nearby cluster (Coma, $z=0.02$). Here we apply the technique to the stacked profiles of 58 clusters at higher redshifts ($0.1z

KW - astro-ph.CO

U2 - 10.1093/mnras/stv1366

DO - 10.1093/mnras/stv1366

M3 - Journal article

VL - 452

SP - 1171

EP - 1183

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 2

ER -