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Baire one star function

From Wikipedia, the free encyclopedia

A Baire one star function is a type of function studied in real analysis. A function is in class Baire* one, written , and is called a Baire one star function if, for each perfect set , there is an open interval , such that is nonempty, and the restriction is continuous. The notion seems to have originated with B. Kirchheim 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 [CG] (for generalized continuity).

References

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  • Maliszewski, Aleksander (1998), "On the averages of Darboux functions", Transactions of the American Mathematical Society, 350 (7): 2833–2846, doi:10.1090/S0002-9947-98-02267-3