English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

such that Ms(t) and rs(t) are related by a power law with coefficient γ. The quoted values of γ in the figure are correct. The curves shown in the figure are not affected, nor are any other figures in the article. A corrected version of Fig. 4 is shown in Fig. 1. In the discussion of the results from the Milky-Way like Aquarius dark matter haloes we mentioned that the similarly defined growth rate ac of Mvir(t) (see Wechsler et al. 2002) was in the range 0.1 to 0.2 for these haloes, which was below the 68% scatter of the median given by Wechsler et al. in their Fig. 8. With the correction above, we now find ac in the range ≈0.2 to 0.4, which is still mostly below the median but within the 68% scatter. The authors would like to thank Raphael Errani for pointing out this error.

A new fitting-function to describe the time evolution of a galaxy’s gravitational potential(Corrigendum)