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Crab (unit)

A Crab is a standard astrophotometrical unit for measurement of the intensity of astrophysical X-ray sources. One Crab is defined as the intensity of the Crab Nebula at the corresponding X-ray photon energy.

The Crab Nebula, and the Crab Pulsar within it, is an intense space X-ray source. It is used as a standard candle in the calibration procedure of X-ray instruments in space. However, because of the Crab Nebula's variable intensity at different X-ray energies, conversion of the Crab to another units depends on the X-ray energy range of interest.

In the photon energy range from 2 to 10 keV, 1 Crab equals 2.4 · 10<sup>−8</sup> erg cm<sup>−2</sup> s<sup>−1</sup> = 15 keV cm<sup>−2</sup> s<sup>−1</sup> = 2.4 · 10<sup>−11</sup> W m<sup>−2</sup>. For energies greater than ~30 keV, the Crab Nebula becomes unsuitable for calibration purposes, as its flux can no longer be characterized by a single coherent model.

The unit mCrab, or milliCrab, is sometimes used instead of the Crab.

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