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We report on our Chandra Cycle 9 program to observe half of the 60(unobserved by Chandra) 3C radio sources at z<0.3 for 8 ksec each. Here we givethe basic data: the X-ray intensity of the nuclei and any features associatedwith radio structures such as hot spots and knots in jets. We have measuredfluxes in soft, medium and hard bands and are thus able to isolate sources withsignificant intrinsic column density. For the stronger nuclei, we have appliedthe standard spectral analysis which provides the best fit values of X-rayspectral index and column density. We find evidence for intrinsic absorptionexceeding a column density of 10^{22} cm^{-2} for one third of our sources.

Chandra Observations of 3C Radio Sources with z<0.3: Nuclei, Diffuse Emission, Jets and Hotspots