Hubble constant and nuclear equation of state from kilonova spectro-photometric light curves

Open Access

Fig. 23.

Hubble constant determination with prior distribution from GW190425 comparing results for run3 EoS DD2 (red) and run10 EoS LS220 (orange), assuming GW190425-KN at 100 Mpc redshift 0.022 and 1 h exposure time. This figure follows the same panel structure than Figs. 21 and 22.

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.