G. W. P. S. D. CEA-Saclay

Astronomy and Astrophysics · 2005–2007

A researcher in the Science corpus: 2 papers; trusts 4 researchers and is trusted by 5 researchers here, as inferred from the citation graph.

Subfields

Whom G. W. P. S. D. CEA-Saclay trusts overall

Their strongest outbound trust, strongest first, inferred from their citations.

  1. G. Mark Voit
  2. M. Arnaud
  3. E. Pointecouteau
  4. G. Pratt

Who trusts G. W. P. S. D. CEA-Saclay overall

  1. G. Pratt
  2. M. Arnaud
  3. H. Böhringer
  4. R. Piffaretti
  5. Judith Croston
  6. A. Vikhlinin
  7. Y.-Y. Zhang

Papers from G. W. P. S. D. CEA-Saclay's perspective

Ordered by how strongly the researchers G. W. P. S. D. CEA-Saclay trusts endorse each paper. Same corpus, a different order for every researcher.

  1. ERRATUM: “CHANDRA SAMPLE OF NEARBY RELAXED GALAXY CLUSTERS: MASS, GAS FRACTION, AND MASS–TEMPERATURE RELATION” (2006, ApJ, 640, 691)
  2. Tracing cosmic evolution with clusters of galaxies
  3. The X‐ray virial relations for relaxed lensing clusters observed with Chandra
  4. The mass profile of A1413 observed with XMM-Newton: Implications for the M-T relation
  5. X‐ray properties of galaxy clusters and groups from a cosmological hydrodynamical simulation
  6. Comparing the temperatures of galaxy clusters from hydrodynamical N-body simulations to Chandra and XMM-Newton observations
  7. Chandra Temperature Profiles for a Sample of Nearby Relaxed Galaxy Clusters
  8. The structural and scaling properties of nearby galaxy clusters. II. The M-T relation
  9. The structural and scaling properties of nearby galaxy clusters. I. The universal mass profile
  10. Details of the mass-temperature relation for clusters of galaxies

Their papers