activity
19952022
most citedPlanck 2013 results. XVI. Cosmological parameters

6.6k citations · 28.1k across the 200 of their papers we have counts for

collaborators
Showing 2012 · astro-ph.COShow all

12 papers · 2 filters

astro-ph.CO2012★ 27 cited

Relative velocity of dark matter and barions in clusters of galaxies and measurements of their peculiar velocities

Klaus Dolag, Rashid Sunyaev

The increasing sensitivity of current experiments, which nowadays routinely measure the thermal SZ effect within galaxy clusters, provide the hope that peculiar velocities of indiv…

astro-ph.CO2012★ 35 cited

AGN and QSOs in the eROSITA All-Sky Survey -- Part I: Statistical properties

Alexander Kolodzig, Marat Gilfanov, Rashid Sunyaev +2

Context. The main element of the observing program of the Spectrum-Roentgen-Gamma orbital observatory is a four-year all-sky survey, in the course of which the entire sky will be s…

astro-ph.CO2012★ 40 cited

Bias from gas inhomogeneities in the pressure profiles as measured from X-ray and SZ observations

S. Khedekar, E. Churazov, A. Kravtsov +4

X-ray observations of galaxy clusters provide emission measure weighted spectra, arising from a range of density and temperature fluctuations in the intra-cluster medium (ICM). Thi…

astro-ph.CO2012★ 69 cited

Planck intermediate results. X. Physics of the hot gas in the Coma cluster

Planck Collaboration, P. A. R. Ade, N. Aghanim +207

We present an analysis of Planck satellite data on the Coma Cluster observed via the Sunyaev-Zeldovich effect. Planck is able, for the first time, to detect SZ emission up to r ~ 3…

astro-ph.CO2012★ 111 cited

Beyond y and μ: the shape of the CMB spectral distortions in the intermediate epoch, 1.5x10^4 < z < 2x10^5

Rishi Khatri, Rashid A. Sunyaev

We calculate numerical solutions and analytic approximations for the intermediate-type spectral distortions. Detection of a μ-type distortion (saturated comptonization) in the CMB…

astro-ph.CO2012★ 4 cited

Angular fluctuations in the CXB: Is Fe 6.4 keV line tomography of the large-scale structure feasible?

Gert Hütsi, Marat Gilfanov, Rashid Sunyaev

AGN are known to account for a major portion, if not all, of the cosmic X-ray background radiation. The dominant sharp spectral feature in their spectra is the 6.4 keV fluorescent…