  Recent observations with the dispersive X-ray spectrometers aboard Chandra
and Newton Observatory have begun to probe the properties of the X-ray
intergalactic medium (IGM) at small redshifts. Using large quantities (~950
ksec) of spectroscopic data acquired using the RGS aboard Newton Observatory,
we investigated the intervening material toward three low redshift, high
Galactic latitude AGNs with nominally featureless spectra: Mrk421, PKS2155-304
and 3C273. Each spectrum provides clear evidence for what appears to be a local
(z~0), highly ionized absorbing medium betrayed by the OVII 1s-2p resonance
transition feature seen at 21.6A (N[OVII] ~ 1E16 cm-2). Measurements are also
made for the Lyman alpha transition of the adjacent ionization state, (OVIII;
18.97A), which potentially constrains the absorber's temperature. Finally, in a
collisional equilibrium approximation, upper limits to diffuse emission
intensities place upper limits on the electron density (ne < 2E-4 cm-3), lower
limits on the scale length of the absorber (L > 140 kpc) and lower limits on
its mass (M > 5E10 M[sun]). Limits on the absorber's scale length and its
velocity distribution lead us to identify it with the Local Group.
