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On the Normalization of the Cosmic Star Formation History

  • Authors: Andrew M. Hopkins and John F. Beacom

Hopkins & Beacom 2006 The Astrophysical Journal 651 142.

  • Provider: AAS Journals

Caption: Fig. 4.

Same as Fig. 2, but assuming a piecewise linear SFH model, assuming (a) SalA IMF and (b) BG IMF. As before, solid lines assume a ﹩\overline{\nu }_{e}﹩ temperature of ﹩T=4﹩ or 6 MeV, and dotted lines, ﹩T=8﹩ MeV.
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