A comprehensive catalog of dark matter halo models for SPARC galaxies
  We present rotation curve fits to 175 late-type galaxies from the Spitzer
Photometry & Accurate Rotation Curves (SPARC) database using seven dark matter
(DM) halo profiles: pseudo-isothermal (pISO), Burkert, Navarro-Frenk-White
(NFW), Einasto, Di Cintio (2014, DC14), coreNFW, and a new semi-empirical
profile named Lucky13. We marginalize over stellar mass-to-light ratio, galaxy
distance, disk inclination, halo concentration and halo mass (and an additional
shape parameter for Einasto) using a Markov Chain Monte Carlo method. We find
that cored halo models such as the DC14 and Burkert profiles generally provide
better fits to rotation curves than the cuspy NFW profile. The stellar
mass-halo mass relation from abundance matching is recovered by all halo
profiles once imposed as a Bayesian prior, whereas the halo mass-concentration
relation is not reproduced in detail by any halo model. We provide an extensive
set of figures as well as best-fit parameters in machine-readable tables to
facilitate model comparison and the exploration of DM halo properties.
