unbiased

a r X i v :a s t r o -p h /0511113v 2 21 F e

b 2006

Astron.Nachr./AN xxx(xxxx)x,xxx–xxx

Correspondence to:larry@e84c7e7e27284b73f242506d tributions from compact sources.At this point,we have sim-ply examined the residual large scale emission by eye,and identi?ed strong diffuse structures.In this examination,we ?nd a rich variety of sources,including extended radio galax-ies,previously known radio halos and relics,the occasional supernova remnant or HII region when we venture too close to the galactic plane,and new diffuse so