Relativistic corrections to Sunyaev-Zeldovich effect (Itoh+, 2004)

Details Relativistic corrections to Sunyaev-Zeldovich effect (Itoh+, 2004) Relativistic corrections to Sunyaev-Zeldovich effect (Itoh+, 2004)

Apr 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ycat..34170827i&link_type=abstract

VizieR On-line Data Catalog: J/A+A/417/827. Originally published in: 2004A&A...417..827I

Physics

Clusters: Galaxy, Models

Scientific paper

These tables contain numerical values for the distortion of the spectral intensity {Delta}I/y defined by the equation {Delta}I/y = 1/y * X3/(eX-1) * {Delta}n(X)/n0(X) = X3/(eX-1)*F({theta}e,X) The spectral intensity is the function of two variables X and {theta}e. Here X={omega}/kB*T0, {omega} being the photon angular frequency and kB*T0 being the thermal energy of CMB photons, and {theta}e=kB*Te/me*c2, kB*Te being the thermal energy of the electrons and me*c2 being the electron rest energy (T0 is the temperature of the cosmic microwave background radiation). In these tables, the range for X is taken as 0(1 data file).

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