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31: 5.17 Barnes’ G -Function (Double Gamma Function)
β–ΊFor error bounds and an exponentially-improved extension, see Nemes (2014a). …
32: Bibliography V
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  • A. L. Van Buren and J. E. Boisvert (2004) Improved calculation of prolate spheroidal radial functions of the second kind and their first derivatives. Quart. Appl. Math. 62 (3), pp. 493–507.
  • 33: 11.11 Asymptotic Expansions of Anger–Weber Functions
    β–ΊFor sharp error bounds and exponentially-improved extensions, see Nemes (2018). … β–ΊThe later references also contain exponentially-improved extensions of (11.11.8) and (11.11.10). …
    34: 9.7 Asymptotic Expansions
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    §9.7(v) Exponentially-Improved Expansions
    35: 10.74 Methods of Computation
    β–ΊFurthermore, the attainable accuracy can be increased substantially by use of the exponentially-improved expansions given in §10.17(v), even more so by application of the hyperasymptotic expansions to be found in the references in that subsection. …
    36: 13.29 Methods of Computation
    β–ΊHowever, this accuracy can be increased considerably by use of the exponentially-improved forms of expansion supplied by the combination of (13.7.10) and (13.7.11), or by use of the hyperasymptotic expansions given in Olde Daalhuis and Olver (1995a). …
    37: 19.14 Reduction of General Elliptic Integrals
    β–ΊIt then improves the classical method by first applying Hermite reduction to (19.2.3) to arrive at integrands without multiple poles and uses implicit full partial-fraction decomposition and implicit root finding to minimize computing with algebraic extensions. …
    38: 25.14 Lerch’s Transcendent
    β–Ί
    25.14.6 Ξ¦ ⁑ ( z , s , a ) = 1 2 ⁒ a s + 0 z x ( a + x ) s ⁒ d x 2 ⁒ 0 sin ⁑ ( x ⁒ ln ⁑ z s ⁒ arctan ⁑ ( x / a ) ) ( a 2 + x 2 ) s / 2 ⁒ ( e 2 ⁒ Ο€ ⁒ x 1 ) ⁒ d x , ⁑ a > 0 if | z | < 1 ; ⁑ s > 1 , ⁑ a > 0 if | z | = 1 .
    39: 30.16 Methods of Computation
    β–ΊApproximations to eigenvalues can be improved by using the continued-fraction equations from §30.3(iii) and §30.8; see Bouwkamp (1947) and Meixner and Schäfke (1954, §3.93). …
    40: 22.19 Physical Applications
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    22.19.6 x ⁑ ( t ) = a ⁒ cn ⁑ ( t ⁒ 1 + 2 ⁒ η , k ) .