Zobrazeno 1 - 10
of 42
pro vyhledávání: '"E J Lloyd"'
Autor:
Scott T. Kay, Michael J. West, Peter A. Thomas, Nicola Mehrtens, P. Rooney, Martin Sahlén, Chris A. Collins, Kivanc Sabirli, Ben Hoyle, Craig D. Harrison, Andrew R. Liddle, E. J. Lloyd-Davies, Christopher J. Miller, C. J. Short, Pedro T. P. Viana, Julian A. Mayers, A. Kathy Romer, Robert C. Nichol, John P. Stott, Matt Hilton, Mark Hosmer, Spencer A. Stanford, Michael Davidson, Robert G. Mann
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 424:2086-2096
We measure the evolution of the X-ray luminosity-temperature (L_X-T) relation since z~1.5 using a sample of 211 serendipitously detected galaxy clusters with spectroscopic redshifts drawn from the XMM Cluster Survey first data release (XCS-DR1). This
Autor:
Martin Sahlén, Chris A. Collins, Craig D. Harrison, Scott T. Kay, E. J. Lloyd-Davies, P. J. Rooney, Matt Hilton, C. M. Booth, John P. Stott, A. Kathy Romer, Alastair C. Edge, Joop Schaye, N. Mehrtens, Ben Hoyle, Pedro T. P. Viana, Andrew R. Liddle, Christopher J. Miller, Ian G. McCarthy, Ryan C. Hickox
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 422:2213-2229
Using a sample of 123 X-ray clusters and groups drawn from the XMM-Cluster Survey first data release, we investigate the interplay between the brightest cluster galaxy (BCG), its black hole, and the intra-cluster/group medium (ICM). It appears that f
Autor:
Pedro T. P. Viana, António da Silva, Elsa P. R. G. Ramos, Andrew R. Liddle, E. J. Lloyd-Davies, A. Kathy Romer, Scott T. Kay, Chris A. Collins, Matt Hilton, Mark Hosmer, Ben Hoyle, Julian A. Mayers, Nicola Mehrtens, Christopher J. Miller, Martin Sahlén, S. Adam Stanford, John P. Stott
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 422:1007-1013
We present a list of 15 clusters of galaxies, serendipitously detected by the XMM Cluster Survey (XCS), that have a high probability of detection by the Planck satellite. Three of them already appear in the Planck Early Sunyaev-Zel'dovich (ESZ) catal
Autor:
Emma Kuwertz, John P. Stott, Christopher J. Miller, Ben Hoyle, Robert G. Mann, A. Kathy Romer, Mark Hosmer, Robert C. Nichol, Pedro T. P. Viana, Martin Sahlén, Chris A. Collins, Kivanc Sabirli, Craig D. Harrison, Peter E. Freeman, Michael Davidson, Nicola Mehrtens, Spencer A. Stanford, Andrew R. Liddle, Scott T. Kay, E. Naomi Dubois, Matt Hilton, Heather Campbell, E. J. Lloyd-Davies
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 418:14-53
The XMM Cluster Survey (XCS) is a serendipitous search for galaxy clusters using all publicly available data in the XMM-Newton Science Archive. Its main aims are to measure cosmological parameters and trace the evolution of X-ray scaling relations. I
Autor:
E. J. Lloyd-Davies, Christopher J. Miller, Scott T. Kay, Mark Hosmer, Matt Hilton, A. K. Romer, Michael Davidson, Pedro T. P. Viana, Diego Capozzi, Andrew R. Liddle, Robert C. Nichol, John P. Stott, Ben Hoyle, S. A. Stanford, Nicola Mehrtens, Martin Sahlén, Chris A. Collins
Publikováno v:
Stott, J P, Collins, C A, Sahlen, M, Hilton, M, Lloyd-Davies, E, Capozzi, D, Hosmer, M, Liddle, A R, Mehrtens, N, Miller, C J, Romer, A K, Stanford, S A, Viana, P T P, Davidson, M, Hoyle, B, Kay, S T & Nichol, B 2010, ' The XMM Cluster Survey: the build up of stellar mass in Brightest Cluster Galaxies at high redshift ', The Astrophysical Journal, vol. 718, no. 1, pp. 23-30 . https://doi.org/10.1088/0004-637X/718/1/23
We present deep J and Ks band photometry of 20 high redshift galaxy clusters between z=0.8-1.5, 19 of which are observed with the MOIRCS instrument on the Subaru Telescope. By using near-infrared light as a proxy for stellar mass we find the surprisi
Autor:
Jimmy A. Irwin, Jifeng Liu, E. J. Lloyd-Davies, Joel N. Bregman, Patrick Seitzer, Catherine Espaillat
Publikováno v:
The Astrophysical Journal. 621:L17-L20
Quasi-periodic oscillations and X-ray spectroscopy are powerful probes of black hole masses and accretion disks, and here we apply these diagnostics to an ultraluminous X-ray source (ULX) in the spiral galaxy NGC628 (M74). This object was observed fo
Autor:
M. Lueker, Chao-Lin Kuo, Christian L. Reichardt, M. C. Runyan, Percy Gomez, Kivanc Sabirli, E. J. Lloyd-Davies, M. D. Daub, W. L. Holzapfel, Christopher Cantalupo, L. E. Valkonen, Andrew E. Lange, J. Ruhl, A. K. Romer, Tomás Verdugo, J. H. Goldstein, J. B. Peterson
We present the first in-depth analysis of the massive cluster AS1063. This is one of the hottest X-ray clusters discovered to date and is undergoing a major merging event. The average temperature of the hot intracluster medium has been measured, usin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c44894a05b1fbe09f5111aef51990387
https://resolver.caltech.edu/CaltechAUTHORS:20120928-151230862
https://resolver.caltech.edu/CaltechAUTHORS:20120928-151230862
Autor:
E. J. Lloyd-Davies, A. Kathy Romer, Martin Sahlén, Chris A. Collins, Craig D. Harrison, John P. Stott, S. Adam Stanford, Nicola Mehrtens, Christopher J. Miller, Diego Capozzi, Andrew R. Liddle, Pedro T. P. Viana, Matt Hilton, Ben Hoyle, Paul James Deadman, Joseph W. Richards
This paper presents both the result of a search for fossil systems (FSs) within the XMM Cluster Survey and the Sloan Digital Sky Survey and the results of a study of the stellar mass assembly and stellar populations of their fossil galaxies. In total
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::851128072c89c1e8d1b7d6473dad9c34
Autor:
Christopher J. Miller, Martin Sahlén, Chris A. Collins, Kivanc Sabirli, S. Adam Stanford, Michael J. West, Robert C. Nichol, E. J. Lloyd-Davies, Robert G. Mann, A. Kathy Romer, Mark Hosmer, Matt Hilton, Andrew R. Liddle, Pedro T. P. Viana, Nicola Mehrtens, Peter E. Freeman, Scott T. Kay, Ben Hoyle, Michael Davidson
We forecast the constraints on the values of sigma_8, Omega_m, and cluster scaling relation parameters which we expect to obtain from the XMM Cluster Survey (XCS). We assume a flat Lambda-CDM Universe and perform a Monte Carlo Markov Chain analysis o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fa0e9bbd564817905c071782da7b73b1
http://sro.sussex.ac.uk/id/eprint/22613/1/MNRAS-2009-Lewis-471-6.pdf
http://sro.sussex.ac.uk/id/eprint/22613/1/MNRAS-2009-Lewis-471-6.pdf
At least 50% of the baryons in the local universe are undetected and predicted to be in a hot dilute phase (1E5-1E7 K) in low and moderate overdensity environments. We searched for the predicted diffuse faint emission through shadowing observations w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d608fe7bdb6a2c2ab61dbd3a155339bd
http://arxiv.org/abs/0907.0275
http://arxiv.org/abs/0907.0275