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/

Zendy Open

Presents the pdf analysis as premium feature

PDF Analysis

Insights

Presents the summarisation as premium feature

Summarisation

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the zaia usage as premium feature

ZAIA

Zendy Tools

Zendy Plus

Presents the access of premium content as premium feature

Premium Content

Accurate and densely populated BVRcIc lightcurves of supernovae SN 2011fe inM101, SN 2012aw in M95 and SN 2012cg in NGC 4424 are presented and discussed.The SN 2011fe lightcurve spans a total range of 342 days, from 17 days pre- to325 days post-maximum. The observations of both SN 2012aw and SN 2012cg werestopped by solar conjunction, when the objects were still bright. Thelightcurve for SN 2012aw covers 92 days, that of SN 2012cg spans 44 days. Timeand brightness of maxima are measured, and from the lightcurve shapes anddecline rates the absolute magnitudes are obtained, and the derived distancesare compared to that of the parent galaxies. The color evolution and thebolometric lightcurves are evaluated in comparison with those of other wellobserved supernovae, showing no significant deviations.

BVRI lightcurves of supernovae SN 2011fe in M101, SN 2012aw in M95, and SN 2012cg in NGC 4424