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- B8fd0ba12b852b87e588008003c81ce22 hasDbXref "https://en.wikipedia.org/wiki/Gamma_ray" @default.
- B8fd0ba12b852b87e588008003c81ce22 type Axiom @default.
- B8fd0ba12b852b87e588008003c81ce22 annotatedProperty comment @default.
- B8fd0ba12b852b87e588008003c81ce22 annotatedSource ENVO_01001218 @default.
- B8fd0ba12b852b87e588008003c81ce22 annotatedTarget "Ambiguity exists in the definition of gamma rays. As a rule of thumb, gamma rays have energies above 100 keV, frequencies above 10 exahertz, and wavelengths less than 10 picometers. However, regardless of the energy released, electromagnetic radiation from radioactive decay of atomic nuclei is referred to as "gamma rays". In astronomy, however, gamma rays are defined by their energy, and no production process needs to be specified." @default.