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Toward a New Kind of Asteroseismic Grid Fitting

  • Authors: M. Gruberbauer, D. B. Guenther, and T. Kallinger

Gruberbauer, Guenther, & Kallinger 2012 The Astrophysical Journal 749 109.

  • Provider: AAS Journals

Caption: Figure 3.

Behavior of the beta prior for systematic offsets in an echelle diagram. The squares represent model frequencies, while the shaded "trails" indicate the prior probability density for varying Δ i . The left panel uses equal Δ max, whereas the right panel uses a power-law Δ max with exponent b = 4.9 (see Section 4.1). Note that the uniform prior is not shown, since it simply assigns a constant probability density.

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