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Dark Matter in the Classical Dwarf Spheroidal Galaxies: A Robust Constraint on the Astrophysical Factor for γ-Ray Flux Calculations

  • Authors: M. G. Walker, C. Combet, J. A. Hinton, D. Maurin, and M. I. Wilkinson

Walker et al. 2011 The Astrophysical Journal Letters 733 L46.

  • Provider: AAS Journals

Caption: Figure 4.

Astrophysical factor as a function of the distance to the dSph. Filled circles, solid, and dashed error bars correspond, respectively, to the median value, 68%, and 95% CIs on (where α c is given in Table 1). Empty circles correspond to .

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