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Baire one star function : ウィキペディア英語版
Baire one star function
Baire one star function is a term from real analysis. A function f: \mathbb \to \mathbb is in class Baire
* one, written f \in \mathbf^_, and is called a Baire one star function, if for each perfect set P \in \mathbb, there is an open interval I \in \mathbb, such that P \cap I is nonempty, and the restriction f |_ is continuous. The notion seems to have originated with B. Kerchheim in an article titled 'Baire one star functions' (Real Anal. Exch. 18 (1992/93), 385-399).
The terminology is actually due to Richard O'Malley, 'Baire
* 1, Darboux functions' Proc. Amer. Math. Soc. 60 (1976) 187-192. The concept itself (under a different name) goes back at least to 1951. See H. W. Ellis, 'Darboux properties and applications to nonabsolutely convergent integrals' Canad. Math. J., 3 (1951), 471-484, where the same concept is labelled as () (for generalized continuity).

==External links==

*(A paper which defines class Baire
* one
)

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