THE SPECTRAL ENERGY-DISTRIBUTION OF THE Z=3 QUASAR - HS-1946+7658

For the bright z = 3.02 radio-quiet quasar, HS 1946+7658, we have obta ined radio to X-ray data within the past year: 5 GHz and 1415 MHz data from the VLA; IR photometry at J, H, K, L' (3.4 mu m) and N; IR spect roscopy; UBVRI photometry; optical spectrophotometry and high-resoluti on spectra; and an X-ray spectrum from the ROSAT PSPC. The spectral en ergy distribution (SEC) constructed from these data is compared to the mean SED for a set of low-redshift quasars, and while they appear gen erally similar, there are several differences. In relation to the low- redshift mean, the SED of HS 1946+7658 shows (1) only an upper limit a t 10 mu m (a rest wavelength of 2.5 mu m) indicating that HS 1946+7658 does not have a strong near-IR excess such as hot dust would produce; (2) relatively weak Fe II and Balmer continuum emission at similar to 3000 Angstrom; and (3) a steeper turndown shortward of Ly alpha, even after correction for the Ly alpha forest absorption lines.