Fig. 2.
Comparison of Chandra and VLA images of NGC 1052. The left and right panels show the Chandra images over 0.5−1 and 1−2 keV, respectively (see also Fig. 1). The superposed contours are from the VLA 1.4 GHz observation from 2002. Contour levels are 3σ (−1, 1, 2, 4, 8…256), where σ = 0.09 mJy beam−1, the image root mean square noise.
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