Volume 518, July-August 2010
Herschel: the first science highlights
Article Number L18
Number of page(s) 5
Section Letters
Published online 16 July 2010

Online Material

\end{figure} Figure 4:

Left - Weak lensing mass maps (contours, spaced at 1$\sigma $ mass reconstruction error; Ok10; Okabe & Umetsu 2008) in order of decreasing cluster virial mass - top left-to-right: A 1835, A 1763, A 1689, A 2219; bottom: A 2390, A 1914, A 1758, Z 7160. Spectroscopically confirmed Herschel-detected members (selected as described in Sect. 4) are marked as filled red circles that scale logarithmically with $L_{\rm TIR}/L_K$. North is up and East is left, and the axis tick-marks are spaced at 1 $\mathrel {\rm arcmin}$ intervals. Right - Number density of galaxies relative to the mean number density of each population as a function of total projected cluster mass density. Positive correlation of the Herschel-detected cluster members with the mass distribution in/surrounding the clusters is detected at ${\sim }$5$\sigma $. The absence of red triangular data points at ${\Sigma}_{\rm mass} > 1000~{\mathrel{M_{\odot}}}~{\mathrel{\rm kpc}}^{-2}$ is because we do not find any non-BCG IR luminous cluster members at such high densities. The dip in the signal for cluster members at ${\sim}1250~{\mathrel{M_{\odot}}}~{\rm kpc}^{-2}$ is due to the incompleteness of our spectroscopic catalog in high density environments due to MMT/Hectospec fiber collisions.

Open with DEXTER

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.