Source	Epoch	Contour PostScript	Colour PostScript	Colour GIF
1404+286 (OQ +208, Mrk 668) Galaxy z= 0.07690 V= 16.0 Notes (from the published papers): From global observations at 6 cm, OQ 208 has been described by Stanghellini et al. (1997) and others as a compact double, characteristic of GHz peaked spectrum sources. Our higher resolution observations at 2 cm, however, show a weak core located between two larger more complex components, suggesting that this source is a CSO. Comparison with the Stanghellini 6 cm image suggests that the central component has an inverted spectrum.	04/1995 12/1995 05/1996 10/1996 09/1997 03/1998 10/1998 07/1999 12/2000 01/2001	PS PS PS PS PS PS PS PS PS PS	PS PS PS PS PS PS PS PS PS PS	GIF GIF GIF GIF GIF GIF GIF GIF GIF GIF

ros@mpifr-bonn.mpg.de