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There should be discussion of the covariance of the solution. I think it's that if J is left-multiplied by the inverse of the input covariance, than <math>J^\top \Sigma^{-1} J</math> is the covariance of the output, or somesuch. [[User:BenFrantzDale|—Ben FrantzDale]] ([[User talk:BenFrantzDale|talk]]) 17:20, 26 October 2011 (UTC)
== External links modified ==
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*Added archive https://web.archive.org/web/20110723020836/http://trac.astrometry.net/wiki/PyLevmar to http://trac.astrometry.net/wiki/PyLevmar
*Added archive https://web.archive.org/web/20130722142233/http://www2.imm.dtu.dk/~hbni/Software/SMarquardt.m to http://www2.imm.dtu.dk/~hbni/Software/SMarquardt.m
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