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The nearby ($z=0.03015$) cluster of galaxies Abell~2199 was observed bySuzaku in X-rays, with five pointings for $\sim 20$ ks each. From the XIS data,the temperature and metal abundance profiles were derived out to $\sim 700$ kpc(0.4 times virial radius). Both these quantities decrease gradually from thecenter to peripheries by a factor of $\sim 2$, while the oxygen abundance tendsto be flat. The temperature within 12' ($\sim 430$ kpc) is $\sim 4$ keV, andthe 0.5--10 keV X-ray luminosity integrated up to 30' is $(2.9 \pm 0.1) \times10^{44}$ erg s$^{-1}$, in agreement with previous XMM-Newton measurements.Above this thermal emission, no significant excess was found either in the XISrange below $\sim 1$ keV, or in the HXD-PIN range above $\sim 15$ keV. The90%-confidence upper limit on the emission measure of an assumed 0.2 keV warmgas is (3.7--7.5) $\times 10^{62}$ cm$^{-3}$ arcmin$^{-2}$, which is 3.7--7.6times tighter than the detection reported with XMM-Newton. The 90%-confidenceupper limit on the 20--80 keV luminosity of any power law component is $1.8\times 10^{43}$ erg s$^{-1}$, assuming a photon index of 2.0. Although thisupper limit does not reject the possible 2.1$\sigma$ detection by the BeppoSAXPDS, it is a factor of 2.1 tighter than that of the PDS if both are consideredupper limits. The non-detection of the hard excess can be reconciled with theupper limit on diffuse radio emission, without invoking the very low magneticfields ($< 0.073 \mu$G) which were suggested previously.

Suzaku Constraints on the Soft and Hard Excess Emissions from Abell 2199