Extended Data Fig. 1: Comparison of the galaxy properties between different methods for dwarf galaxies in LITTLE THINGS.
From: Further evidence for a population of dark-matter-deficient dwarf galaxies
a, Comparison of the rH i using our method with that obtained using tilted-ring method by LITTLE THINGS team. b, Comparison of the VH i using our method with that obtained using tilted-ring method by LITTLE THINGS team. c, Comparison of the dynamical mass estimated using our method with those derived using the tilted-ring method. Black and grey dots are measurements based on w20 and w50, respectively.
