Shemi, A. Mon. We thank E. Perlman for providing the radio flux of 1ES1853-379 prior to publication, and J. Lim and S. Johnston for forwarding the results of the Parkes pulsar search. The EUVE limiting flux was obtained through the Center for Extreme Ultraviolet Astrophysics' Skyflux request facility. The central region of the V-band image from the CTIO 0.9m. The radius of the HRI error circle is 1.5 arcsec.
North is up and east is to the left.
The gray scale has been stretched to bring up the fainter stars. We reduced the plate solution to the GSC reference frame by triangulating on HST guide stars in the field. Only star M was detected in our U-band image, to a limiting magnitude of 19.6 0.3. The best fit blackbody spectrum. The relatively poor suggests the formal uncertainties may be too small.