Free Access

  

Table 3:

Model parameters inferred from the lensing analysis.
\begin{displaymath}\begin{tabular}[c]{lr@{$~\pm~$}lr@{$~\pm~$}lr@{$~\pm~$}lr@{$~...
...n{2}{c}{[--2.4]}&\\
\noalign{\smallskip }
\hline
\end{tabular}\end{displaymath}

Notes. For each model, the first line specifies the mass components accounted by the cluster-sized halo, parameterized as a NFW distribution.``All'' refers to a mass model (DM+baryons) with a single NFW component. The other models may have additional components either for the gas or the galactic halos. The BCG is either scaled as the other galaxies (``All galaxies'') or embedded in the cluster-zised halo (halos ``with BCG''). The ICM is either modelled apart or embedded in the cluster-sized halo (``Halo with ICM''). The orientation angle $\theta_\epsilon$ is measured north over east and $r_{\rm sP}$ ( $r_{\rm cP}$) is the projected length scale (core radius) for the NFW ($\beta $) profile. Parameters in squared brackets were kept fixed in the lensing analysis. Convergences are normalised to the E system source redshift.


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.