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We present a combined radio, optical, and X-ray study of the nearby LINERgalaxy NGC 1052. Data from a short (2.3 ksec) {\it CHANDRA} observation of NGC1052 reveal the presence of various jet-related X-ray emitting regions, abright compact core and unresolved knots in the jet structure as well as anextended emitting region inside the galaxy well aligned with the radiosynchrotron jet-emission. The spectrum of the extended X-ray emission can bestbe fitted with a thermal model with $kT = (0.4-0.5)$ keV, while the compactcore exhibits a very flat spectrum, best approximated by an absorbed power-lawwith $N_{\rm H} = (0.6-0.8) \times 10^{22} {\rm cm^{-2}}$. We compare the radiostructure to an optical ``structure map'' from a {\it Hubble Space Telescope}({\it HST}) observation and find a good positional correlation between theradio jet and the optical emission cone. Bright, compact knots in the jetstructure are visible in all three frequency bands whose spectrum isinconsistent with synchrotron emission.Comment: 8 pages, 5 figures (figure 2 in color), image resolution degraded wrt  journal version, needs aa.cls. Accepted for publication in A&

Jet emission in NGC 1052 at radio, optical, and X-ray frequencies