Erratum: Particle Dark Matter constraints: the effect of Galactic uncertainties (Journal of Cosmology and Astroparticle Physics DOI: 10.1088/1475-7516/2017/02/007)

This erratum corrects the following mistakes in our paper Particle Dark Matter Constraints: the Effect of Galactic Uncertainties: values of the stellar mass of the Milky Way (MW) in column 4 of table 1, values of the total MW mass quoted in text, and a typo when referring to the value of the total MW as quoted in the Sagittarius stream paper [1]. Here we provide a correct version of table 1 (stellar mass of the MW corrected, column 4), and replace the final, corrected version of the text (original lines below table 1 in page 5). No other element of the paper has changed, and conclusions are unaffected. 1.1 Changes: When varying Galactic parameters, we obtain the total mass of the MW within 50 kpc to be in the range M(< 50 ) = (1.2-22.9) × 1011MȮ. The lower limit is in agreement with previous determinations [1, 11-14], while the larger MW masses we obtain can not be directly compared, as the adopted Galactic Parameters are different than ours. When varying baryonic morphology, the minimum/maximum values obtain are M(< 50 kpc) = 4.36+0.11-0.10 × 1011 MȮ and M(< 50 kpc) = 7.0±0.3 × 1011MȮ. The former value for the variation of morphology is in good agreement with mass estimate from kinematics of globular clusters, satellite galaxies and halo stars [11, 12, 14, 15]. There is, however, a discrepancy at the 1 σ level with the independent determination in [1], that used the Sagittarius stream, and is slightly smaller than the other cited determinations. All our results are in agreement at the 1 σ level with the recent estimate of the dynamical mass [16] within the region of the Galactic bulge, as in the analysis presented in [17]. (Table Presented).