We present ROSAT PSPC observations of the similar to 500 Myr old Coma
Berenices cluster. The X-ray survey in Coma consists of a) a raster sc
an of short duration PSPC pointings, b) ROSAT All-Sky Survey data, and
c) a 16 ksec deep PSPC pointing. The raster scan and the survey data
were merged together covering an area of about 36 square degrees, whil
e the deep pointing was analyzed separately. No major differences were
found between the two datasets. Our ROSAT observations indicate that
Coma is much more similar in its X-ray properties to the coeval Hyades
than to the also coeval Praesepe cluster. As in the Hyades, almost al
l late-F and G stars were detected, also showing a comparable range in
X-ray luminosity. X-ray luminosity distribution functions (XLDFs) for
solar-type members are in close agreement with those of the Hyades, c
onfirming that the majority of Praesepe's members are less luminous th
an what one would expect for stars of their age. The Coma Berenices cl
uster is known for its apparent deficit of low mass stars of spectral
type K and later. We present 12 new possible low-mass Coma candidates,
identified through this X-ray survey.