2002AJ....123..637D

We present optical and/or near-IR images of 128 ultra-steep-spectrum radio sources. Roughly half of the objects are identified in the optical images (R≲24), while in the near-IR images, more than 94% are detected at K≲22. The mean K magnitude is K{d1}=19.26 within a 2" diameter aperture. The distribution of R-K colors indicates that at least one-third of the objects observed have very red colors (R-K>5). The major axes of the identifications in the K band are preferentially oriented along the radio axes, with half of them having compact morphologies. The 22 sources with spectroscopic redshifts and K-band magnitudes follow the K-z relation found from previous radio samples, but with a larger scatter. We argue that this may be due to a dependence of K magnitude on the radio power, with the most luminous radio sources inhabiting the most massive host galaxies. We present a composite K-z diagram of radio-loud and radio-quiet galaxies, selected from the Hubble Deep Field (North) and the Hawaii surveys. Out to z≲1, the radio-loud galaxies trace the bright envelope of the radio quiet galaxies, while at z≳1, the radio-loud galaxies are ≳2 mag brighter. We argue that this is not due to a contribution from the active galactic nucleus or emission lines. This difference strongly suggests that radio galaxies pinpoint the most massive systems out to the highest known redshifts, probably as a result of the mutual correlation of the mass of the galaxy and the radio power on the mass of the central black hole.