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distance modulus
noun
- astronomy a measure of the distance, r , of a celestial object too far away to show measurable parallax. It is given by m – M = 5 log( r /10), where m is its apparent magnitude (corrected for interstellar absorption) and M is its absolute magnitude
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Example Sentences
Examples have not been reviewed.
For our adopted distance modulus and foreground reddening, this implies that any source at the position of AT 2017gfo must have an absolute magnitude F606W > −5.8.
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