Fully stripped? The dynamics of dark and luminous matter in the massive cluster collision MACSJ0553.4-3342
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[1] D. Wittman,et al. The Mismeasure of Mergers: Revised Limits on Self-interacting Dark Matter in Merging Galaxy Clusters , 2017, The Astrophysical Journal.
[2] S. Randall,et al. MULTI-WAVELENGTH OBSERVATIONS OF THE DISSOCIATIVE MERGER IN THE GALAXY CLUSTER CIZA J0107.7+5408 , 2016, 1604.03551.
[3] K. Nandra,et al. Second ROSAT all-sky survey (2RXS) source catalogue , 2016, 1609.09244.
[4] M. Markevitch,et al. THE MERGING GALAXY CLUSTER A520—A BROKEN-UP COOL CORE, A DARK SUBCLUSTER, AND AN X-RAY CHANNEL , 2016, 1603.05232.
[5] H. Ebeling,et al. Jellyfish: the origin and distribution of extreme ram-pressure stripping events in massive galaxy clusters , 2015, 1511.00033.
[6] S. Molendi,et al. The evolution of the spatially-resolved metal abundance in galaxy clusters up to z=1.4 , 2015, 1504.02107.
[7] David Harvey,et al. The nongravitational interactions of dark matter in colliding galaxy clusters , 2015, Science.
[8] O. Fèvre,et al. The galaxy luminosity function at z ≃ 6 and evidence for rapid evolution in the bright end from z ≃ 7 to 5 , 2014, 1411.2976.
[9] J. Kneib,et al. Mass and magnification maps for the Hubble Space Telescope Frontier Fields clusters: implications for high-redshift studies , 2014 .
[10] R. Massey,et al. Hubble Frontier Fields: a high-precision strong-lensing analysis of the massive galaxy cluster Abell 2744 using ∼180 multiple images , 2014, 1409.8663.
[11] R. Bouwens,et al. FIRST FRONTIER FIELD CONSTRAINTS ON THE COSMIC STAR FORMATION RATE DENSITY AT z ∼ 10—THE IMPACT OF LENSING SHEAR ON COMPLETENESS OF HIGH-REDSHIFT GALAXY SAMPLES , 2014, 1409.1228.
[12] J. Kneib,et al. NEW CONSTRAINTS ON THE FAINT END OF THE UV LUMINOSITY FUNCTION AT z ∼ 7–8 USING THE GRAVITATIONAL LENSING OF THE HUBBLE FRONTIER FIELDS CLUSTER A2744 , 2014, 1409.0512.
[13] S. Paltani,et al. The stripping of a galaxy group diving into the massive cluster A2142 , 2014, 1408.1394.
[14] Y. Rephaeli,et al. Evolution of the gas mass fraction in galaxy clusters , 2014, 1406.3709.
[15] A. Edge,et al. JELLYFISH: EVIDENCE OF EXTREME RAM-PRESSURE STRIPPING IN MASSIVE GALAXY CLUSTERS , 2013, 1312.6135.
[16] J. Richard,et al. An X-ray/optical study of the geometry and dynamics of MACS J0140.0−0555, a massive post-collision cluster merger , 2012, 1207.6235.
[17] A. Edge,et al. Discovery of radio haloes and double relics in distant MACS galaxy clusters: clues to the efficiency of particle acceleration , 2012, 1206.6102.
[18] W. Couch,et al. SHOCKING TAILS IN THE MAJOR MERGER ABELL 2744 , 2012, 1204.1052.
[19] A. Connolly,et al. THE DEEP2 GALAXY REDSHIFT SURVEY: DESIGN, OBSERVATIONS, DATA REDUCTION, AND REDSHIFTS , 2012, 1203.3192.
[20] Jean-Paul Kneib,et al. Cluster lenses , 2012, 1202.0185.
[21] A. Mann,et al. X-ray–optical classification of cluster mergers and the evolution of the cluster merger fraction , 2011, 1111.2396.
[22] Christine Jones,et al. THE UNIVERSAL GAS MASS FRACTION IN CLUSTERS OF GALAXIES , 2011, 1109.5067.
[23] J. Kneib,et al. Strong lensing by a node of the cosmic web The core of MACS J0717.5+3745 at z=0.55 , 2011, 1109.3301.
[24] D. Masters,et al. SpecPro: An Interactive IDL Program for Viewing and Analyzing Astronomical Spectra , 2011, 1103.3222.
[25] J. Rhodes,et al. Creation of cosmic structure in the complex galaxy cluster merger Abell 2744 , 2011, 1103.2772.
[26] A. Edge,et al. The X-ray brightest clusters of galaxies from the Massive Cluster Survey , 2010, 1004.4683.
[27] J. Kneib,et al. LoCuSS: first results from strong-lensing analysis of 20 massive galaxy clusters at z= 0.2 , 2009, 0911.3302.
[28] S. Borgani,et al. The cluster gas mass fraction as a cosmological probe: a revised study , 2009, 0904.2740.
[29] H. Ebeling,et al. AN X-RAY/OPTICAL STUDY OF THE COMPLEX DYNAMICS OF THE CORE OF THE MASSIVE INTERMEDIATE-REDSHIFT CLUSTER MACSJ0717.5+3745 , 2009, 0901.4783.
[30] J. Kneib,et al. Keck spectroscopic survey of strongly lensed galaxies in Abell 1703: further evidence of a relaxed, unimodal cluster , 2009, 0901.0427.
[31] Edinburgh,et al. Revealing the Properties of Dark Matter in the Merging Cluster MACS J0025.4–1222 , 2008, 0806.2320.
[32] M. Donahue,et al. Hα Tail, Intracluster H II Regions, and Star Formation: ESO 137-001 in Abell 3627 , 2007, 0706.1220.
[33] IoA,et al. Improved constraints on dark energy from Chandra X-ray observations of the largest relaxed galaxy clusters , 2007, 0706.0033.
[34] J. Kneib,et al. A Bayesian approach to strong lensing modelling of galaxy clusters , 2007, 0706.0048.
[35] Anthony H. Gonzalez,et al. Constraints on the Self-Interaction Cross Section of Dark Matter from Numerical Simulations of the Merging Galaxy Cluster 1E 0657–56 , 2007, 0704.0261.
[36] A. Edge,et al. A Complete Sample of 12 Very X-Ray Luminous Galaxy Clusters at z > 0.5 , 2007, astro-ph/0703394.
[37] J. Kneib,et al. The strong transformation of spiral galaxies infalling into massive clusters at z≈ 0.2 , 2007, astro-ph/0703012.
[38] L. Moscardini,et al. Virial Scaling of Massive Dark Matter Halos: Why Clusters Prefer a High Normalization Cosmology , 2007, astro-ph/0702241.
[39] Alexey Vikhlinin,et al. Shocks and cold fronts in galaxy clusters , 2007, astro-ph/0701821.
[40] D. Clowe,et al. A Direct Empirical Proof of the Existence of Dark Matter , 2006, astro-ph/0608407.
[41] J. Sanders. Contour binning: a new technique for spatially-resolved X-ray spectroscopy applied to Cassiopeia A , 2006, astro-ph/0606528.
[42] M. Markevitch,et al. SUBMITTED TO APJ Preprint typeset using LATEX style emulateapj v. 11/27/05 THE ORIGIN OF COLD FRONTS IN THE CORES OF RELAXED GALAXY CLUSTERS , 2006 .
[43] H. Ebeling,et al. Asmooth: a simple and efficient algorithm for adaptive kernel smoothing of two-dimensional imaging data , 2006, astro-ph/0601306.
[44] M. Markevitch,et al. Absolute Measurement of the Unresolved Cosmic X-Ray Background in the 0.5-8 keV Band with Chandra , 2005, astro-ph/0512542.
[45] C. Jones,et al. ERRATUM: “CHANDRA SAMPLE OF NEARBY RELAXED GALAXY CLUSTERS: MASS, GAS FRACTION, AND MASS–TEMPERATURE RELATION” (2006, ApJ, 640, 691) , 2005, astro-ph/0507092.
[46] W. B. Burton,et al. The Leiden/Argentine/Bonn (LAB) Survey of Galactic HI - Final data release of the combined LDS and IAR surveys with improved stray-radiation corrections , 2005, astro-ph/0504140.
[47] D. Clowe,et al. Direct constraints on the dark matter self-interaction cross-section from the merging galaxy cluster 1E0657-56 , 2003, astro-ph/0309303.
[48] G. Bruzual,et al. Stellar population synthesis at the resolution of 2003 , 2003, astro-ph/0309134.
[49] N. Aghanim,et al. The X-ray surface brightness profiles of hot galaxy clusters up to $\vec z$ ~ 0.8: Evidence for self-similarity and constraints on $\Omega_\mathsf{0}$ , 2002 .
[50] R. S. Warwick,et al. X-ray background measurements with XMM-Newton EPIC , 2002, astro-ph/0204147.
[51] Orsay,et al. The X-ray surface brightness profiles of hot galaxy clusters up to z~0.8: evidence for self-similarity and constraints on Omega_0 , 2001, astro-ph/0110428.
[52] A. Edge,et al. MACS: A Quest for the Most Massive Galaxy Clusters in the Universe , 2000, astro-ph/0009101.
[53] E. Bertin,et al. SExtractor: Software for source extraction , 1996 .
[54] I. Smail,et al. Hubble Space Telescope Observations of the Lensing Cluster Abell 2218 , 1995, astro-ph/9511015.
[55] Alan M. Watson,et al. The On-Orbit Performance of WFPC2 , 1994 .
[56] Y. Mellier,et al. The Dark Matter Distribution in MS 2137-23 from the Modeling of the Multiple Arc Systems , 1993 .
[57] T. Beers,et al. Measures of location and scale for velocities in clusters of galaxies. A robust approach , 1990 .
[58] S. Snowden,et al. Deconstructing the Spectrum of the Soft X-Ray Background , 2000 .