what methods of detection does it include?
The detector must be at least 1 km deep to suppress downward traveling muons, and are subject to an irreducible background of extraterrestric neutrinos interacting in the Earth's atmosphere.
Neutrino astronomy
 The detector must be at least 1 km deep to suppress downward traveling muons, and are subject to an irreducible background of extraterrestric neutrinos interacting in the Earth's atmosphere.
what area of science did the muslim world excel in Astronomy, mathematics, and medicine. what does the first one refer to? The natural science that studies celestial objects and phenomena. what is it further classified into? Observational, radio, Infrared, Optical , Ultraviolet, X-ray and Gamma-ray astronomy. what are the leading types of the second area? UNANSWERABLE are there any foundations associated with it? Yes, in nutrino astronomy, GALLEX or Gallium Experiment was a radiochemical neutrino detection experiment that ran between 1991 and 1997 at the Laboratori Nazionali del Gran Sasso (LNGS). what does the the kind of astronomy mean? It  is the branch of astronomy that observes astronomical objects with neutrino detectors in special observatories. what are it's applications? It is used for observing the cores of stars.
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Neutrino astronomy [SEP] Detection methods
Upward because no other known particle can traverse the entire Earth. The detector must be at least 1 km deep to suppress downward traveling muons, and are subject to an irreducible background of extraterrestric neutrinos interacting in the Earth's atmosphere. This background also provides a standard calibration source. Sources of radioactive isotopes must also be controlled as they produce energetic particles when they decay. The detectors consist of an array of photomultiplier tubes (PMTs) housed in transparent pressure spheres which are suspended in a large volume of water or ice. The PMTs record the arrival time and amplitude of the Cherenkov light emitted by muons or particle cascades.