K correction
K correction is a process for converting measurements of astronomical objects into their respective rest frames. The correction acts on that object's observed magnitude (or equivalently, its flux).
K correction is a process for converting measurements of astronomical objects into their respective rest frames. The correction acts on that object's observed magnitude (or equivalently, its flux).
K correction is a process for converting measurements of astronomical objects into their respective rest frames. The correction acts on that object's observed magnitude (or equivalently, its flux).
Source: Wikipedia "K correction" · CC BY-SA 4.0
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