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Paper detail

A right and left truncated gamma distribution with application to the stars

The gamma density function is usually defined in interval between zero and infinity. This paper introduces an upper and a lower boundary to this distribution. The parameters which characterize the truncated gamma distribution are evaluated. A statistical test is performed on two samples of stars. A comparison with the lognormal and the four power law distribution is made.

preprint2014arXivOpen access
L. Zaninetti
astro-ph.IMastro-ph.SR
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L. Zaninetti

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