Search Results - "Maughan, B. J"

Self-similar scaling and evolution in the galaxy cluster X-ray luminosity-temperature relation by Maughan, B. J., Giles, P. A., Randall, S. W., Jones, C., Forman, W. R.

“…We investigate the form and evolution of the X-ray luminosity-temperature (L X-kT) relation of a sample of 114 galaxy clusters observed with Chandra at 0.1 < z…”
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Chandra measurements of a complete sample of X-ray luminous galaxy clusters: the luminosity–mass relation by Giles, P A, Maughan, B J, Dahle, H, Bonamente, M, Landry, D, Jones, C, Joy, M, Murray, S S, van der Pyl, N

“…We present the results of work involving a statistically complete sample of 34 galaxy clusters, in the redshift range 0.15 = z = 0.3 observed with Chandra. We…”
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The X-ray luminosity–temperature relation of a complete sample of low-mass galaxy clusters by Zou, S., Maughan, B. J., Giles, P. A., Vikhlinin, A., Pacaud, F., Burenin, R., Hornstrup, A.

“…We present Chandra observations of 23 galaxy groups and low-mass galaxy clusters at 0.03 < z < 0.15 with a median temperature of ${\sim }2{{\rm keV}}$ . The…”
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The X-ray properties of weak-lensing-selected galaxy clusters by Giles, P A, Maughan, B J, Hamana, T, Miyazaki, S, Birkinshaw, M, Ellis, R S, Massey, R

“…We present the results of an X-ray follow-up campaign targeting 10 weak-lensing (WL)-selected galaxy clusters from a Subaru WL survey. Archival Chandra data…”
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The evolution of the cluster X-ray scaling relations in the Wide Angle ROSAT Pointed Survey sample at 0.6 < z < 1.0 by Maughan, B. J., Jones, L. R., Ebeling, H., Scharf, C.

“…The X-ray properties of a sample of 11 high-redshift (0.6 < z < 1.0) clusters observed with Chandra and/or XMM-Newton are used to investigate the evolution of…”
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Separating the BL Lac and cluster X-ray emissions in Abell 689 withChandra by Giles, P A, Maughan, B J, Birkinshaw, M, Worrall, D M, Lancaster, K

“…ABSTRACT We present the results of aChandra observation of the galaxy cluster Abell 689 (z = 0.279). Abell 689 is one of the most luminous clusters detected in…”
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The LX-YX Relation: Using Galaxy Cluster X-Ray Luminosity as a Robust, Low-Scatter Mass Proxy by Maughan, B. J

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The WARPS Survey - VIII. Evolution of the galaxy cluster X-ray Luminosity Function by Koens, L. A., Maughan, B. J., Jones, L. R., Ebeling, H., Horner, D. J., Perlman, E. S., Phillipps, S., Scharf, C. A.

“…We present measurements of the galaxy cluster X-ray Luminosity Function (XLF) from the Wide Angle ROSAT Pointed Survey (WARPS) and quantify its evolution…”
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Deep XMM-Newton and Chandra Observations of Cl J1226.9+3332: A Detailed X-Ray Mass Analysis of a z = 0.89 Galaxy Cluster by Maughan, B. J, Jones, C, Jones, L. R, Van Speybroeck, L

“…Deep XMM-Newton and Chandra observations of Cl J1226.9+3332 at z = 0.89 have enabled the most detailed X-ray mass analysis of any such high-redshift galaxy…”
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PICACS: self-consistent modelling of galaxy cluster scaling relations by Maughan, B. J.

“…In this paper, we introduce Physically motivated, Internally Consistent Analysis of Cluster Scaling (PICACS), a detailed model of scaling relations between…”
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The L X ‐ Y X Relation: Using Galaxy Cluster X‐Ray Luminosity as a Robust, Low‐Scatter Mass Proxy by Maughan, B. J.

“…We use a sample of 115 galaxy clusters at 0.1 < z < 1.3 observed with Chandra ACIS-I to investigate the relation between luminosity and Y(x (the product of gas…”
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Testing the galaxy cluster mass–observable relations at z=1 with XMM–Newton and Chandra observations of XLSSJ022403.9−041328 by Maughan, B. J., Jones, L. R., Pierre, M., Andreon, S., Birkinshaw, M., Bremer, M. N., Pacaud, F., Ponman, T. J., Valtchanov, I., Willis, J.

“…We present an analysis of deep XMM–Newton and Chandra observations of the z= 1.05 galaxy cluster XLSSJ022403.9−041328 (hereafter XLSSC 029), detected in the…”
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A systematic comparison of galaxy cluster temperatures measured with NuSTAR and Chandra by Wallbank, A N, Maughan, B J, Gastaldello, F, Potter, C, Wik, D R

“…ABSTRACT Temperature measurements of galaxy clusters are used to determine their masses, which in turn are used to determine cosmological parameters. However,…”
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An XMM–Newton observation of the massive, relaxed galaxy cluster ClJ1226.9+3332 at z= 0.89 by Maughan, B. J., Jones, L. R., Ebeling, H., Scharf, C.

“…A detailed X-ray analysis of an XMM–Newton observation of the high-redshift (z= 0.89) galaxy cluster ClJ1226.9+3332 is presented. After careful consideration…”
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SUNYAEV-ZEL'DOVICH-MEASURED PRESSURE PROFILES FROM THE BOLOCAM X-RAY/SZ GALAXY CLUSTER SAMPLE by Sayers, J, Czakon, N G, Mantz, A, Golwala, S R, Ameglio, S, Downes, T P, Koch, P M, Lin, K-Y, Maughan, B J, Molnar, S M

“…We describe Sunyaev-Zel'dovich (SZ) effect measurements and analysis of the intracluster medium (ICM) pressure profiles of a set of 45 massive galaxy clusters…”
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The XXL Survey – XLVIII. X-ray follow-up of distant XXL clusters: masses, scaling relations, and AGN contamination by Duffy, R T, Logan, C H A, Maughan, B J, Eckert, D, Birkinshaw, M, Clerc, N, Ettori, S, Gastaldello, F, Koulouridis, E, Pierre, M, Ricci, M, Sereno, M, Valtchanov, I, Willis, J P

“…ABSTRACT We use deep follow-up XMM–Newton observations of six clusters discovered in the XXL Survey at z > 1 to gain robust measurements of their X-ray…”
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The XXL Survey. XLII. The LX − σ v relation of galaxy groups and clusters detected in the XXL and GAMA surveys by Giles, P A, Robotham, A, Ramos-Ceja, M E, Maughan, B J, Sereno, M, McGee, S, Phillipps, S, Iovino, A, Turner, D J, Adami, C, Brough, S, Chiappetti, L, Driver, S P, Evrard, A E, Farahi, A, Gastaldello, F, Holwerda, B W, Hopkins, A M, Koulouridis, E, Pacaud, F, Pierre, M, Pimbblet, K A

“…ABSTRACT The XXL Survey is the largest homogeneous survey carried out with XMM-Newton. Covering an area of 50 deg2, the survey contains several hundred galaxy…”
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Chandra X-Ray Analysis of the Massive High-Redshift Galaxy Clusters Cl J1113.1–2615 and Cl J0152.7–1357 by Maughan, B. J, Jones, L. R, Ebeling, H, Perlman, E, Rosati, P, Frye, C, Mullis, C. R

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XMM-Newton Observes Cl J0152.7–1357: A Massive Galaxy Cluster Forming at Merger Crossroads at z = 0.83 by Maughan, B. J, Ellis, S. C, Jones, L. R, Mason, K. O, Córdova, F. A, Priedhorsky, W

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Separating the BL Lac and cluster X-ray emissions in Abell 689 with Chandra by Giles, P. A., Maughan, B. J., Birkinshaw, M., Worrall, D. M., Lancaster, K.

“…We present the results of a Chandra observation of the galaxy cluster Abell 689 (z = 0.279). Abell 689 is one of the most luminous clusters detected in the…”
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