| Abstract
| - We have conducted observations of the environment around the z=2.15 radio-loud quasar 1550-269 in search of distant galaxies associated either with it or the z=2.09 C iv absorber along its line of sight. Such objects will be distinguished by their red colours, R−K>4.5. We find five such objects in a 1.5 arcmin2 field around the quasar, with typical K′ magnitudes of ∼20.4 and no detected R-band emission. We also find a sixth object with K=19.6±0.3, and undetected at R, just two arcsec from the quasar. The nature of all these objects is currently unclear, and will remain so until we have determined their redshifts. We suggest that it is likely that they are associated with either the quasar or the C iv absorber, in which case their properties might be similar to those of the z=2.38 red Lyα emitting galaxies discovered by Francis et al. The small separation between the quasar and the brightest of our objects suggests that it may be the galaxy responsible for the C iv metal line absorption system. The closeness to the quasar and the red colour might have precluded similar objects from being uncovered in previous searches for emission from C iv and damped absorbers.
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