X-ray to optical flux ratio: X/O 120. Typical Type I AGN: X/O 10 ... (very rare): X/O ~ 100. If an EXO it is much more X-ray bright than any detected ...
5-20 arcmin (about twice better than EGRET) Sensitivity: ... 3 sr, about 6 times EGRET's. sensitivity for a 1-year all sky survey 3 times better than EGRET ...
Wide gaps between some lobes in radio galaxies imply jets launched after mergers ... If jets are moderately conical, the standard analysis, which assumes =0, would ...
... inverted spectrum of the Extreme Intra-day Variable (IDV) Blazar PKS 0405-385 ... by the two radio lobes transform the bubble into a fat pancake, or superdisk ...
-quasar LS 5039. GRO J1823-12 (l/b: 17.5/-0.5) Summary. complicated source region ... exclude the quasar QSO 0241 622 as the source of ?-ray emission. ...
For several EGRET blazars, recent VLBI shows: vapp 25c (hence j 25) (Piner et al. 2006) ... Why deceleration in TeV blazars only (and not in EGRET blazars) ...