Abstract
Following on the discussion of the properties of the near-infrared sky, we now describe the hardware suite required to successfully carry out observations in this wavelength range. This includes a brief illustration of the standard telescope concepts, a discussion on the various flavors of active and adaptive optics systems, an outline of how imagers, spectrographs, integral-field units and interferometers work, a description of the filter systems in the near-infrared, and a discussion of the detector technologies currently in use. The understanding of all these is imperative to properly prepare, execute, and reduce near-infrared observations. Finally, we comment on the upcoming 30m class telescopes and their instrumentation.
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Heidt, J. (2022). Hardware for Near-Infrared Observations—Adaptive Optics, Instrumentation, and Detectors. In: Astronomy in the Near-Infrared - Observing Strategies and Data Reduction Techniques. Astrophysics and Space Science Library, vol 467. Springer, Cham. https://doi.org/10.1007/978-3-030-98441-0_4
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