K band (infrared)

In infrared astronomy, the K band is an atmospheric transmission window centered on 2.2 μm (in the near-infrared 136 THz range).

[1][2] HgCdTe-based detectors are typically preferred for observing in this band.

[3] Photometric systems used in astronomy are sets of filters or detectors that have well-defined windows of absorption, based around a central peak detection frequency and where the edges of the detection window are typically reported where sensitivity drops below 50% of peak.

Various organizations have defined systems with various peak frequencies and cutoffs in the K band, including K′, and KS, and Kdark.

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