The nearby ( z = 0.03015 ) cluster of galaxies Abell 2199 was observed by Suzaku 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 the center to peripheries by a factor of \sim 2 , while the oxygen abundance tends to be flat .
The temperature within 12 ^ { \prime } ( \sim 430 kpc ) is \sim 4 keV , and the 0.5–10 keV X-ray luminosity integrated up to 30 ^ { \prime } is ( 2.9 \pm 0.1 ) \times 10 ^ { 44 } erg s ^ { -1 } , in agreement with previous XMM-Newton measurements .
Above this thermal emission , no significant excess was found either in the XIS range below \sim 1 keV , or in the HXD-PIN range above \sim 15 keV .
The 90 % -confidence upper limit on the emission measure of an assumed 0.2 keV warm gas is ( 3.7–7.5 ) \times 10 ^ { 62 } cm ^ { -3 } arcmin ^ { -2 } , which is 3.7–7.6 times tighter than the detection reported with XMM-Newton .
The 90 % -confidence upper 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 this upper limit does not reject the possible 2.1 \sigma detection by the BeppoSAX PDS , it is a factor of 2.1 tighter than that of the PDS if both are considered upper limits .
The non-detection of the hard excess can be reconciled with the upper limit on diffuse radio emission , without invoking the very low magnetic fields ( < 0.073 \mu G ) which were suggested previously .