  We present mid- and far-IR photometry of the high-redshift (z=4.69) dusty
quasar BR1202-0725. The quasar was detected in the near-IR, at a flux level
(0.7+/-0.2 mJy) consistent with an average Radio-Quiet Quasar at it's redshift.
Only upper limits for the emission were obtained in the far-IR. These upper
limits, when combined with data from ground-based telescopes, are the first
direct evidence for a turn-over in the far-IR emission and hence confirm that a
black-body dominates the SED at FIR wavelengths. This black-body is most
probably cool dust, constrained to have a temperature below 80K, for a beta of
1.5.
