activity
20142026
most citedThe XXL Survey: I. Scientific motivations - XMM-Newton observing plan - Follow-up observations and simulation programme

272 citations · 1.5k across the 26 of their papers we have counts for

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Showing 2015Show all

7 papers · 1 filter

astro-ph.GA2015★ 17 cited

The XXL Survey X: K-band luminosity - weak-lensing mass relation for groups and clusters of galaxies

F. Ziparo, G. P. Smith, S. L. Mulroy +15

We present the K-band luminosity-halo mass relation, , for a subsample of 20 of the 100 brightest clusters in the XXL Survey observed with WIRCam at the Canad…

astro-ph.CO2015★ 272 cited

The XXL Survey: I. Scientific motivations - XMM-Newton observing plan - Follow-up observations and simulation programme

M. Pierre, F. Pacaud, C. Adami +89

We present the XXL Survey, the largest XMM programme totaling some 6.9 Ms to date and involving an international consortium of roughly 100 members. The XXL Survey covers two extrag…

astro-ph.CO2015★ 143 cited

The XXL Survey. II. The bright cluster sample: catalogue and luminosity function

F. Pacaud, N. Clerc, P. A. Giles +40

Context. The XXL Survey is the largest survey carried out by the XMM-Newton satellite and covers a total area of 50 square degrees distributed over two fields. It primarily aims at…

astro-ph.CO2015★ 89 cited

The XXL Survey IV. Mass-temperature relation of the bright cluster sample

Maggie Lieu, Graham P. Smith, Paul A. Giles +18

The XXL survey is the largest survey carried out by XMM-Newton. Covering an area of 50deg, the survey contains galaxy clusters out to a redshift 2 and to an X-r…

astro-ph.CO2015★ 102 cited

The XXL Survey III. Luminosity-temperature relation of the Bright Cluster Sample

P. A. Giles, B. J. Maughan, F. Pacaud +13

The XXL Survey is the largest homogeneous survey carried out with XMM-Newton. Covering an area of 50 deg, the survey contains several hundred galaxy clusters out to a redshif…

astro-ph.CO2015★ 116 cited

The XXL Survey. XIII. Baryon content of the bright cluster sample

D. Eckert, S. Ettori, J. Coupon +20

Traditionally, galaxy clusters have been expected to retain all the material accreted since their formation epoch. For this reason, their matter content should be representative of…

astro-ph.CO2015★ 121 cited

LoCuSS: Testing hydrostatic equilibrium in galaxy clusters

G. P. Smith, P. Mazzotta, N. Okabe +17

We test the assumption of hydrostatic equilibrium in an X-ray luminosity selected sample of 50 galaxy clusters at from the Local Cluster Substructure Survey (LoCuSS).…