(Q58489890)

2

object named as

A. Finoguenov

0 references

Hans Böhringer

3

object named as

H. Böhringer

0 references

author name string

Y.-Y. Zhang

1

0 references

G. P. Smith

5

0 references

O. Czoske

6

0 references

G. Soucail

Astronomy and Astrophysics

7

0 references

language of work or name

English

0 references

publication date

5 March 2007

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published in

1 reference

SIMBAD

volume

467

1 reference

SIMBAD

issue

2

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page(s)

437–457

1 reference

The LX--T relation and intracluster gas fractions of X-ray clusters

SIMBAD

cites work

1 reference

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A CFH12k lensing survey of X-ray luminous galaxy clusters. I. Weak lensing methodology

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Determination of the Cosmic Distance Scale from Sunyaev‐Zel’dovich Effect andChandraX‐Ray Measurements of High‐Redshift Galaxy Clusters

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Strong‐Lensing Analysis of A1689 from Deep Advanced Camera Images

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Adaptive spatial binning of integral-field spectroscopic data using Voronoi tessellations

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VIMOS-IFU survey of z~0.2 massive galaxy clusters. I. Observations of the strong lensing cluster Abell 2667

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Mass Estimates of X-Ray Clusters

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Hubble Space TelescopeObservations of the Lensing Cluster Abell 2218

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A Wide-Field Hubble Space Telescope Study of the Cluster Cl 0024+1654 at z=0.4. II. The Cluster Mass Distribution

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A Probablez ∼ 7 Galaxy Strongly Lensed by the Rich Cluster A2218: Exploring the Dark Ages

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Properties of the Intracluster Medium in an Ensemble of Nearby Galaxy Clusters

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A Universal Density Profile from Hierarchical Clustering

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Measuring8with Cluster Lensing: Biases from Unrelaxed Clusters

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A Hubble Space Telescope lensing survey of X-ray luminous galaxy clusters - IV. Mass, structure and thermodynamics of cluster cores at z = 0.2

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Multiple-images in the cluster lens Abell 2218: Constraining the geometry of the Universe?

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The X‐Ray Luminosity–Mass Relation for Local Clusters of Galaxies

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ChandraSample of Nearby Relaxed Galaxy Clusters: Mass, Gas Fraction, and Mass‐Temperature Relation

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The baryon content of galaxy clusters: a challenge to cosmological orthodoxy

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The prevalence of cooling cores in clusters of galaxies atz≈ 0.15-0.4

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Temperature Profiles of Nearby Clusters of Galaxies

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The 2–8 keV cosmic X-ray background spectrum as observed with XMM-Newton

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Erratum: Properties of the X-ray-brightest Abell-type clusters of galaxies (XBACs) from ROSAT All-Sky Survey data -- I. The sample

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Cosmological Constraints from the Evolution of the Cluster Baryon Mass Function atz∼ 0.5

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