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

An erroneous interpretation of the hydrodynamical results led to an incorrectdetermination of the fallback masses in Ugliano et al. (2012), which also (on asmaller level) affects the neutron star masses provided in that paper. Thisproblem was already addressed and corrected in the follow-up works by Ertl etal. (2015) and Sukhbold et al. (2015). Therefore, the reader is advised to usethe new data of the latter two publications. In the remaining text of thisErratum we present the differences of the old and new fallback results indetail and explain the origin of the mistake in the original analysis byUgliano et al. (2012).

Erratum: Progenitor-explosion connection and remnant birth masses for neutrino-driven supernovae of iron-core progenitors (2012, ApJ, 757, 69)