Classifier Instance:

Anchor text: Herschel Space Observatory
Target Entity: Herschel_Space_Observatory
Preceding Context: While bolometers can be used to measure radiation of any frequency, for most wavelength ranges there are other methods of detection that are more sensitive. For submillimeter wavelengths (from around 200 µm to 1 mm wavelength, also known as the far-infrared or terahertz), bolometers are among the most sensitive available detectors, and are therefore used for astronomy at these wavelengths. To achieve the best sensitivity, they must be cooled down to a fraction of a degree above absolute zero (typically from 50 millikelvins to 300 mK). Notable examples of bolometers employed in submillimeter astronomy include the
Succeeding Context: , the Atacama Large Millimeter Array (ALMA), the James Clerk Maxwell Telescope, and the Stratospheric Observatory for Infrared Astronomy (SOFIA).
Paragraph Title: Applications in astronomy
Source Page: Bolometer

Ground Truth Types:

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