Photometric mass and mass decomposition in early-type lens galaxies

Free Access

Table 6:

The 1 $\sigma$ confidence intervals of the mass in the form of dark matter.
	Sal, BC/Sal, M	Cha, BC/Kro, M
$M_{{\rm D}}[(R_{{\rm Ein}}/R_{{\rm e}}) \le 0.2]~(M_{*})$	[0.04,0.22]	[0.18,0.43]
$M_{{\rm D}}[(R_{{\rm Ein}}/R_{{\rm e}}) \le 0.6]~(M_{*})$	[0.19,0.31]	[0.58,0.70]
$M_{{\rm D}}[(R_{{\rm Ein}}/R_{{\rm e}}) \le 1.0]~(M_{*})$	[0.20,0.41]	[0.63,1.12]

Notes: in each aperture, the lower and upper limits of the intervals are chosen as the smallest and the largest values predicted, at 1 $\sigma$ confidence level, by the best-fit power-law and pseudo-Jaffe models. These values are given in units of the luminous mass, that is determined by adopting a Salpeter (left) or Chabrier/Kroupa (right) IMF.

Source LaTeX | All tables | In the text

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.