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S. S. Murray

9 ta ish

Center for Astrophysics Harvard & Smithsonian

AkademScholarda batafsil koʻrsatkichlar

  1. <i>Chandra</i>Sample of Nearby Relaxed Galaxy Clusters: Mass, Gas Fraction, and Mass‐Temperature Relation

    A. Vikhlinin, Andrey V. Kravtsov, W. Forman +4

    Maqola20064 iqtibos
    ABI

  2. Direct Constraints on the Dark Matter Self‐Interaction Cross Section from the Merging Galaxy Cluster 1E 0657−56

    Maxim Markevitch, Anthony H. Gonzalez, Douglas Clowe +5

    MaqolaOchiq kirish20043 iqtibos
    ABI

  3. An Overview of the Performance and Scientific Results from the<i>Chandra X‐Ray Observatory</i>

    Martin C. Weisskopf, Bert Brinkman, C. R. Canizares +3

    MaqolaOchiq kirish20023 iqtibos
    ABI

  4. COSMOLOGICAL CONSTRAINTS FROM SUNYAEV–ZEL'DOVICH-SELECTED CLUSTERS WITH X-RAY OBSERVATIONS IN THE FIRST 178 deg<sup>2</sup> OF THE SOUTH POLE TELESCOPE SURVEY

    B. A. Benson, T. de Haan, J. P. Dudley +77

    MaqolaOchiq kirish20133 iqtibos
    ABI

  5. OPTICAL SPECTROSCOPY AND VELOCITY DISPERSIONS OF GALAXY CLUSTERS FROM THE SPT-SZ SURVEY

    J. Ruel, G. Bazin, Matthew Bayliss +79

    MaqolaOchiq kirish20143 iqtibos
    ABI

  6. <i>CHANDRA</i>CLUSTER COSMOLOGY PROJECT. II. SAMPLES AND X-RAY DATA REDUCTION

    A. Vikhlinin, R. Burenin, H. Ebeling +8

    MaqolaOchiq kirish20093 iqtibos
    ABI

  7. MASS CALIBRATION AND COSMOLOGICAL ANALYSIS OF THE SPT-SZ GALAXY CLUSTER SAMPLE USING VELOCITY DISPERSION σ<sub><i>v</i></sub>AND X-RAY<i>Y</i><sub>X</sub>MEASUREMENTS

    S. Bocquet, A. Saro, J. J. Mohr +68

    MaqolaOchiq kirish20152 iqtibos
    ABI

  8. COSMOLOGICAL CONSTRAINTS FROM GALAXY CLUSTERS IN THE 2500 SQUARE-DEGREE SPT-SZ SURVEY

    T. de Haan, B. A. Benson, L. E. Bleem +74

    MaqolaOchiq kirish20162 iqtibos
    ABI

  9. THE GROWTH OF COOL CORES AND EVOLUTION OF COOLING PROPERTIES IN A SAMPLE OF 83 GALAXY CLUSTERS AT 0.3 &lt;<i>z</i>&lt; 1.2 SELECTED FROM THE SPT-SZ SURVEY

    M. McDonald, B. A. Benson, A. Vikhlinin +76

    MaqolaOchiq kirish20132 iqtibos
    ABI