DISCOVERY OF A Z=2.76 DUSTY RADIO GALAXY

We report the discovery of a z = 2.76 radio galaxy, MG 1019+0535, with an unusual spectrum. Ly alpha, which usually dominates the spectra of high-redshift radio galaxies, is very weak, and the strongest lines i n the spectrum are C IV lambda 1549 and He II lambda 1640. We speculat e that dust is responsible for attenuating the Ly alpha line. This obj ect provides more evidence for dust formation at early epochs. The opt ical counterpart of the compact radio source has a double morphology w hich is orthogonal to the radio source axis and most likely due to the superposition of two distinct objects which may or may not be physica lly related. There is only one detected line from the brighter compone nt (B) which is close in observed wavelength to the redshifted He II l ambda 1640 line from the z = 2.76 galaxy (A). We discuss whether B is at the same redshift as A or whether it is a foreground galaxy at z = 0.66. We also report the serendipitous discovery of a very red (R-K > 7) field object.