Overview of submm Single Dish: From Observations to Useful Data

Observing with single dish telescopes at submillimetre wavelengths adds a number of challenges. The Earth's atmosphere not only absorbs the sky signal with varying amounts as a function of frequency and weather conditions, but it also emits a signal that is many orders of magnitude brighter than the astronomical signal one is interested in. Additional challenges come in the calibration and removal of certain instrumental effects. I will give an overview of present and planned submillimetre telescopes, instrument types, and observing strategies.