Inferring dark matter halo properties for H i-selected galaxies

We set constraints on the dark matter halo mass and concentration of ∼22 000 individual galaxies visible both in H I (from the ALFALFA survey) and optical light (from the Sloan Digital Sky Survey). This is achieved by combining two Bayesian models, one for the H I line width as a function of the ste...

תיאור מלא

מידע ביבליוגרפי
Main Authors: Yasin, T, Desmond, H, Devriendt, J, Slyz, A
פורמט: Journal article
שפה:English
יצא לאור: Oxford University Press 2023