activity
19982001
most citedRelativistic Corrections to the Sunyaev-Zel'dovich Effect for Clusters of Galaxies. IV. Analytic fitting formula for the Numerical Results

61 citations · 129 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph2001★ 4 cited

Nonrelativistic Electron-Electron Thermal Bremsstrahlung Gaunt Factor

Naoki Itoh, Youhei Kawana, Satoshi Nozawa

With the launch of the Chandra X-Ray Observatory and XMM-Newton, X-ray astronomy has entered an era of precision science. The precision observational data taken by these satellites…

astro-ph2000

Relativistic Corrections to the Sunyaev-Zel'dovich Effect for Clusters of Galaxies. V. Precision Analytic Fitting Formula for the Crossover Frequency Region

Naoki Itoh, Youhei Kawana, Satoshi Nozawa

We have succeeded in obtaining a precision analytic fitting formula for the exact numerical results of the relativistic corrections to the thermal Sunyaev-Zeldovich effect for clus…

astro-ph2000★ 32 cited

Relativistic Corrections to the Sunyaev-Zel'dovich Effect for Clusters of Galaxies. V. Multiple Scattering

Naoki Itoh, Youhei Kawana, Satoshi Nozawa +1

We extend the formalism for the calculation of the relativistic corrections to the Sunyaev-Zel'dovich effect for clusters of galaxies and include the multiple scattering effects. W…

astro-ph2000★ 61 cited

Relativistic Corrections to the Sunyaev-Zel'dovich Effect for Clusters of Galaxies. IV. Analytic fitting formula for the Numerical Results

Satoshi Nozawa, Naoki Itoh, Youhei Kawana +1

We present an accurate analytic fitting formula for the numerical results for the relativistic corrections to the thermal Sunyaev-Zel'dovich effect for clusters of galaxies. The nu…

astro-ph1998★ 32 cited

Relativistic Corrections to the Sunyaev-Zel'dovich Effect for Clusters of Galaxies. III. Polarization Effect

Naoki Itoh, Satoshi Nozawa, Yasuharu Kohyama

We extend the formalism of the relativistic thermal and kinematic Sunyaev-Zel'dovich effects and include the polarization of the cosmic microwave background photons. We consider th…