Evidence against cuspy dark matter haloes in large galaxies

@article{Rodrigues2017EvidenceAC,
  title={Evidence against cuspy dark matter haloes in large galaxies},
  author={Davi C. Rodrigues and Antonino del Popolo and Valerio Marra and Paulo L. C. de Oliveira},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2017},
  volume={470},
  pages={2410-2426}
}
We develop and apply new techniques in order to uncover galaxy rotation curves (RC) systematics. Considering that an ideal dark matter (DM) profile should yield RCs that have no bias towards any particular radius, we find that the Burkert DM profile satisfies the test, while the Navarro-Frenk-While (NFW) profile has a tendency of better fitting the region between one and two disc scale lengths than the inner disc scale length region. Our sample indicates that this behaviour happens to more than… Expand

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