AMICO galaxy clusters in KiDS-DR3: Measuring the splashback radius from weak gravitational lensing

Open Access

Table 4.

Adopted prior parameters for the DK14 model when modelling the cluster+lss data set is used to constrain the splashback radius.

log₁₀(M_200m/h⁻¹ M_⊙)	Gaussian ^(a)
c_200m	Gaussian ^(a)
r_t/R_200m	[0.8, 5]
b_e	[0.1, 4]
s_e	[0.5, 2]

Notes.

^(a)

As derived from the cluster data model.

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.