For fixed , a large positive root must lie close to a pole of the tangent function: away from its poles, cannot balance the unbounded right side. Label the adjacent poles by and write . The Taylor series of gives
Seek the asymptotic expansion . The coefficients of and give
Thus the large roots near tangent poles satisfy
The first correction already supplies the requested dependence on . For the root approaches the pole from below; for it approaches from above. This labels roots by their nearby poles, avoiding an irrelevant finite shift in the enumeration of positive roots.
No positivity restriction on is required. The expansion requires fixed and , so the displacement is small. It is not uniform as . At the roots are exactly , a different leading sequence; these cannot be recovered by setting in the pole expansion. If varies with , its size must be checked against the small-displacement and successive-term conditions rather than using the fixed-parameter remainder blindly.
Watson's lemma applies to Laplace-type endpoint integrals such as as , when has a local algebraic expansion with and suitable integrability or exponential-growth control away from the endpoint. Each term contributes . The exponential selects a neighborhood of .
Laplace method instead treats by locating the dominant maxima of a real phase . A smooth nondegenerate interior maximum produces a neighborhood governed by a Gaussian function of width ; endpoint or degenerate maxima require their corresponding local scaling. Contributions away from a strict dominant maximum must be smaller. These methods overlap after suitable changes of variable, but their usual starting forms emphasize an endpoint amplitude expansion and an exponential maximum, respectively.
For the Gamma function, put . Then
The phase has its unique maximum at , with value and second derivative . Set . Near this maximum,
Combining the amplitude and exponential expansions in Laplace method gives
Localization near justifies extending the limits for the Gaussian integral; the distant endpoint is not being expanded uniformly by this local series. Odd terms integrate to zero. The moments of the Gaussian integral satisfy , , , so the relative correction is
The two terms of the Stirling formula, obtained by the Stirling correction by Gaussian moments, are therefore

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