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The VIRUS-dE Survey. I. Stars in Dwarf Elliptical Galaxies—3D Dynamics and Radially Resolved Stellar Initial Mass Functions

  • Authors: Mathias Lipka, Jens Thomas, Roberto Saglia, Ralf Bender, Maximilian Fabricius, Gary J. Hill, Matthias Kluge, Martin Landriau, Ximena Mazzalay, Eva Noyola, Taniya Parikh, Jan Snigula

Mathias Lipka et al 2024 The Astrophysical Journal 976 .

  • Provider: AAS Journals

Caption: Figure 23.

Comparison of an optimized LOSVD model parameterized by a Gauss–Hermite series (left) and a nonparametric description (right) for the same Voronoi Bin of VCC 200 (S/N = 26). Both are broadly consistent with one another. In the case of this specific Voronoi Bin, the Gauss–Hermite representation is slightly preferred by AIC p . The error suppression by a Gauss–Hermite parameterization at high velocities is substantial, which is why we readjusted the errors as described in Section 2.2.

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