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20022006
most citedMass-temperature relation of galaxy clusters: implications from the observed luminosity-temperature relation and X-ray temperature function

48 citations · 100 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph2006★ 38 cited

Radial profile and log-normal fluctuations of intra-cluster medium as an origin of systematic bias of spectroscopic temperature

Hajime Kawahara, Yasushi Suto, Tetsu Kitayama +4

The origin of the recently reported systematic bias in the spectroscopic temperature of galaxy clusters is investigated using cosmological hydrodynamical simulations. We find that…

astro-ph2006★ 3 cited

Systematic bias in the estimate of cluster mass and the fluctuation amplitude from cluster abundance statistics

Mamoru Shimizu, Tetsu Kitayama, Shin Sasaki +1

We revisit the estimate of the mass fluctuation amplitude, sigma_8, from the observational X-ray cluster abundance. In particular, we examine the effect of the systematic differenc…

astro-ph2003★ 5 cited

Monte-Carlo Modeling of Non-Gravitational Heating Processes in Galaxy Clusters

Mamoru Shimizu, Tetsu Kitayama, Shin Sasaki +1

We consider non-gravitational heating effects on galaxy clusters on the basis of the Monte-Carlo modeling of merging trees of dark matter halos combined with the thermal evolution…

astro-ph2002★ 48 cited

Mass-temperature relation of galaxy clusters: implications from the observed luminosity-temperature relation and X-ray temperature function

Mamoru Shimizu, Tetsu Kitayama, Shin Sasaki +1

We derive constraints on the mass-temperature relation of galaxy clusters from their observed luminosity-temperature relation and X-ray temperature function. Adopting the isotherma…

astro-ph2002★ 6 cited

Reliability of merger tree realizations of dark halos in the Monte-Carlo modeling of galaxy formation

Mamoru Shimizu, Tetsu Kitayama, Shin Sasaki +1

We examine the reliability of the merger trees generated for the Monte-Carlo modeling of galaxy formation. In particular we focus on the cold gas fraction predicted from the merger…