The Citing articles tool gives a list of articles citing the current article.CrossRef Cited-by Linking Program
Cited article:
P. Schuecker , H. Böhringer , C. A. Collins , L. Guzzo
A&A, 398 3 (2003) 867-877
Published online: 2003-01-28
This article has been cited by the following article(s):
155 articles | Pages:
The dependence of galaxy formation on cosmological parameters: can we distinguish between the WMAP1 and WMAP3 parameter sets?
Jie Wang, Gabriella De Lucia, Manfred G. Kitzbichler and Simon D. M. White384 (4) 1301 (2008)https://doi.org/10.1111/j.1365-2966.2007.12797.x
An Evolving Entropy Floor in the Intracluster Gas?
Wenjuan Fang and Zoltán Haiman680 (1) 200 (2008)https://doi.org/10.1086/587780
The representative XMM-Newton cluster structure survey (REXCESS) of an X-ray luminosity selected galaxy cluster sample
H. Böhringer, P. Schuecker, G. W. Pratt, et al. 469 (1) 363 (2007)https://doi.org/10.1051/0004-6361:20066740
Galaxy clusters in the CFHTLS
L. F. Olsen, C. Benoist, A. Cappi, et al. 461 (1) 81 (2007)https://doi.org/10.1051/0004-6361:20066088
The Virial Mass Function of Nearby SDSS Galaxy Clusters
Kenneth Rines, Antonaldo Diaferio and Priyamvada Natarajan657 (1) 183 (2007)https://doi.org/10.1086/510829
Scaling relations and mass calibration of the X-ray
luminous galaxy clusters at redshift ~0.2: XMM-Newton observations
Y.-Y. Zhang, A. Finoguenov, H. Böhringer, et al. 467 (2) 437 (2007)https://doi.org/10.1051/0004-6361:20066567
The
XMM‐Newton
Wide‐Field Survey in the COSMOS Field: Statistical Properties of Clusters of Galaxies
A. Finoguenov, L. Guzzo, G. Hasinger, et al. 172 (1) 182 (2007)https://doi.org/10.1086/516577
Statistics of X-ray observables for the cooling-core and non-cooling core galaxy clusters
Y. Chen, T. H. Reiprich, H. Böhringer, Y. Ikebe and Y.-Y. Zhang466 (3) 805 (2007)https://doi.org/10.1051/0004-6361:20066471
The 400 Square Degree
ROSAT
PSPC Galaxy Cluster Survey: Catalog and Statistical Calibration
R. A. Burenin, A. Vikhlinin, A. Hornstrup, et al. 172 (2) 561 (2007)https://doi.org/10.1086/519457
GaBoDS: The Garching-Bonn deep survey
M. Hetterscheidt, P. Simon, M. Schirmer, et al. 468 (3) 859 (2007)https://doi.org/10.1051/0004-6361:20065885
TheXMMCluster Survey: The Dynamical State of XMMXCS J2215.9−1738 atz= 1.457
Matt Hilton, Chris A. Collins, S. Adam Stanford, et al. 670 (2) 1000 (2007)https://doi.org/10.1086/522827
High-redshift Fanaroff-Riley type II radio sources: large-scale X-ray environment
E. Belsole, D. M. Worrall, M. J. Hardcastle and J. H. Croston381 (3) 1109 (2007)https://doi.org/10.1111/j.1365-2966.2007.12298.x
Cosmological Simulations of the Preheating Scenario for Galaxy Cluster Formation: Comparison to Analytic Models and Observations
Joshua D. Younger and Greg L. Bryan666 (2) 647 (2007)https://doi.org/10.1086/520619
Breaking Cosmological Degeneracies in Galaxy Cluster Surveys with a Physical Model of Cluster Structure
Joshua D. Younger, Zoltan Haiman, Greg L. Bryan and Sheng Wang653 (1) 27 (2006)https://doi.org/10.1086/508646
Galaxy groups in the 2dF Galaxy Redshift Survey: the number density of groups
V. R. Eke, Carlton M. Baugh, Shaun Cole, Carlos S. Frenk and Julio F. Navarro370 (3) 1147 (2006)https://doi.org/10.1111/j.1365-2966.2006.10568.x
Non-linear structure formation in cosmologies with early dark
energy
M. Bartelmann, M. Doran and C. Wetterich454 (1) 27 (2006)https://doi.org/10.1051/0004-6361:20053922
X-ray properties in massive galaxy clusters: XMM-Newton observations of the REFLEX-DXL sample
Y.-Y. Zhang, H. Böhringer, A. Finoguenov, et al. 456 (1) 55 (2006)https://doi.org/10.1051/0004-6361:20053650
The Sunyaev‐Zel'dovich Effect in CMB‐calibrated Theories Applied to the Cosmic Background Imager Anisotropy Power atl> 2000
J. R. Bond, C. R. Contaldi, U.‐L. Pen, et al. 626 (1) 12 (2005)https://doi.org/10.1086/429855
The First Cosmic Structures and Their Effects
Benedetta Ciardi and Andrea Ferrara116 (3-4) 625 (2005)https://doi.org/10.1007/s11214-005-3592-0
Neutrino mass limit from galaxy cluster number density evolution
Tina Kahniashvili, Eckhard von Toerne, Natalia A. Arhipova and Bharat Ratra71 (12) 125009 (2005)https://doi.org/10.1103/PhysRevD.71.125009
Restframe I-band Hubble diagram for type Ia supernovae up
to redshift z $\mathsf{\sim}$ 0.5
S. Nobili, R. Amanullah, G. Garavini, et al. 437 (3) 789 (2005)https://doi.org/10.1051/0004-6361:20042463
Towards a precision cosmology from starburst galaxies atz> 2
E. R. Siegel, R. Guzmán, Jorge P. Gallego, M. Orduña López and P. Rodríguez Hidalgo356 (3) 1117 (2005)https://doi.org/10.1111/j.1365-2966.2004.08539.x
Temperature gradients in XMM-Newton
observed REFLEX-DXL galaxy clusters
at z $\mathsf{\sim 0.3}$
Y.-Y. Zhang, A. Finoguenov, H. Böhringer, et al. 413 (1) 49 (2004)https://doi.org/10.1051/0004-6361:20031531
Cosmological parameters from SDSS and WMAP
Max Tegmark, Michael A. Strauss, Michael R. Blanton, et al. 69 (10) 103501 (2004)https://doi.org/10.1103/PhysRevD.69.103501
Observability of gamma rays from neutralino annihilations in the Milky Way substructure
Savvas M. Koushiappas, Andrew R. Zentner and Terrence P. Walker69 (4) 043501 (2004)https://doi.org/10.1103/PhysRevD.69.043501
Constraining Amplitude and Slope of the Mass Fluctuation Spectrum Using a Cluster Baryon Mass Function
A. Voevodkin and A. Vikhlinin601 (2) 610 (2004)https://doi.org/10.1086/380818
Astrophysics in 2003
Virginia Trimble and Markus J. Aschwanden116 (817) 187 (2004)https://doi.org/10.1086/383241
X‐Ray Temperatures for the Extended Medium‐Sensitivity Survey High‐Redshift Cluster Sample: Constraints on Cosmology and the Dark Energy Equation of State
J. Patrick Henry609 (2) 603 (2004)https://doi.org/10.1086/421336
Halo model analysis of cluster statistics
Eduardo Rozo, Scott Dodelson and Joshua Frieman70 (8) 083008 (2004)https://doi.org/10.1103/PhysRevD.70.083008
Multiwavelength Cosmology
Steven W. Allenhttps://doi.org/10.1007/0-306-48570-2_50
The Dark Side of the Halo Occupation Distribution
Andrey V. Kravtsov, Andreas A. Berlind, Risa H. Wechsler, et al. 609 (1) 35 (2004)https://doi.org/10.1086/420959
Constraining the evolution of dark energy with a combination of galaxy cluster observables
Sheng Wang, Justin Khoury, Zoltán Haiman and Morgan May70 (12) 123008 (2004)https://doi.org/10.1103/PhysRevD.70.123008
The X-ray luminosity-velocity dispersion relation in the REFLEX cluster survey
A. Ortiz-Gil, L. Guzzo, P. Schuecker, H. Böhringer and C. A. Collins348 (1) 325 (2004)https://doi.org/10.1111/j.1365-2966.2004.07371.x
The ROSAT-ESO Flux Limited X-ray (REFLEX) Galaxy cluster survey
H. Böhringer, P. Schuecker, L. Guzzo, et al. 425 (1) 367 (2004)https://doi.org/10.1051/0004-6361:20034484
The case for dynamical dark energy revisited
Ujjaini Alam, Varun Sahni and A A Starobinsky2004 (06) 008 (2004)https://doi.org/10.1088/1475-7516/2004/06/008
Detection of X-ray clusters of galaxies by matching
RASS photons and SDSS galaxies within GAVO
P. Schuecker, H. Böhringer and W. Voges420 (1) 61 (2004)https://doi.org/10.1051/0004-6361:20035597
CMB-cluster lensing
Scott Dodelson70 (2) 023009 (2004)https://doi.org/10.1103/PhysRevD.70.023009
The Brera Multi-scale Wavelet HRI Cluster Survey
A. Moretti, L. Guzzo, S. Campana, et al. 428 (1) 21 (2004)https://doi.org/10.1051/0004-6361:20041326
Galaxy clustering and dark energy
Dipak Munshi, Cristiano Porciani and Yun Wang349 (1) 281 (2004)https://doi.org/10.1111/j.1365-2966.2004.07498.x
Last stand before WMAP: Cosmological parameters from lensing, CMB, and galaxy clustering
Xiaomin Wang, Max Tegmark, Bhuvnesh Jain and Matias Zaldarriaga68 (12) (2003)https://doi.org/10.1103/PhysRevD.68.123001
Halo Substructure and the Power Spectrum
Andrew R. Zentner and James S. Bullock598 (1) 49 (2003)https://doi.org/10.1086/378797
A new prescription for protogalactic feedback and outflows: where have all the baryons gone?
J. Silk343 (1) 249 (2003)https://doi.org/10.1046/j.1365-8711.2003.06674.x
The Mass, Baryonic Fraction, and X‐Ray Temperature of the Luminous, High‐Redshift Cluster of Galaxies MS 0451.6−0305
Megan Donahue, Jessica A. Gaskin, Sandeep K. Patel, et al. 598 (1) 190 (2003)https://doi.org/10.1086/378688
Measuring $\mathsf{\Omega_{m}}$ using clusters evolution
A. Del Popolo408 (1) 43 (2003)https://doi.org/10.1051/0004-6361:20030954
Cosmological constraints from the cluster contribution to the power spectrum of the soft X-ray background. New evidence for a low sigma8 ?
J. M. Diego, W. Sliwa, J. Silk and X. Barcons344 (3) 951 (2003)https://doi.org/10.1046/j.1365-8711.2003.06884.x
Median Statistics and the Mass Density of the Universe
Gang Chen and Bharat Ratra115 (811) 1143 (2003)https://doi.org/10.1086/377112
First‐Year
Wilkinson Microwave Anisotropy Probe
(
WMAP
) Observations: Determination of Cosmological Parameters
D. N. Spergel, L. Verde, H. V. Peiris, et al. 148 (1) 175 (2003)https://doi.org/10.1086/377226
On determining the cluster abundance normalization
E. Pierpaoli, S. Borgani, D. Scott and M. White342 (1) 163 (2003)https://doi.org/10.1046/j.1365-8711.2003.06525.x
Observational constraints on general relativistic energy
conditions, cosmic matter density and dark energy from X-ray
clusters of galaxies and type-Ia supernovae
P. Schuecker, R. R. Caldwell, H. Böhringer, et al. 402 (1) 53 (2003)https://doi.org/10.1051/0004-6361:20030197
Cosmological constraints from the local X-ray luminosity function of the most X-ray-luminous galaxy clusters
S. W. Allen, R. W. Schmidt, A. C. Fabian and H. Ebeling342 (1) 287 (2003)https://doi.org/10.1046/j.1365-8711.2003.06550.x
Constraining the cosmological parameters with the gas mass fraction
in local and $\mathsf{{\vec z}>0.7}$ galaxy clusters
S. Ettori, P. Tozzi and P. Rosati398 (3) 879 (2003)https://doi.org/10.1051/0004-6361:20021706
A preference for a non-zero neutrino mass from cosmological data
S. W. Allen, R. W. Schmidt and S. L. Bridle346 (2) 593 (2003)https://doi.org/10.1046/j.1365-2966.2003.07022.x
Improvements in theM‐TRelation, Mass Function, and Measured Value of \documentclass{aastex} \usepackage{amsbsy} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{bm} \usepackage{mathrsfs} \usepackage{pifont} \usepackage{stmaryrd} \usepackage{textcomp} \usepackage{portland,xspace} \usepackage{amsmath,amsxtra} \usepackage[OT2,OT1]{fontenc} \newcommand\cyr{ \renewcommand\rmdefault{wncyr} \renewcommand\sfdefault{wncyss} \renewcommand\encodingdefault{OT2} \normalfont \selectfont} \DeclareTextFontCommand{\textcyr}{\cyr} \pagestyle{empty} \DeclareMathSizes{10}{9}{7}{6} \begin{document} \landscape $\Omega _{m}$ \end{document} through Cluster Evolution
A. Del Popolo599 (2) 723 (2003)https://doi.org/10.1086/379542
Measuring
8
with Cluster Lensing: Biases from Unrelaxed Clusters
Graham P. Smith, Alastair C. Edge, Vincent R. Eke, et al. 590 (2) L79 (2003)https://doi.org/10.1086/376747
Halo Properties in Models with Dynamical Dark Energy
A. Klypin, A. V. Macciò, R. Mainini and S. A. Bonometto599 (1) 31 (2003)https://doi.org/10.1086/379237
Pages:
101 to 155 of 155 articles
and 
from cluster abundance and large-scale clustering