Multi-messenger constraints on the neutron-star equation of state and the Hubble constant by T. Dietrich, M. W. Coughlin, P. T. H. Pang, M. Bulla, J. Heinzel, L. Issa, I. Tews, S. Antier
Data and code realease
The individual directories contain:
EOS
--> the chiral EFT EOSs used for our study
POSSIS_models
--> Kilonova spectral energy distributions from POSSIS used as input for gwemlightcurves
bilby_patches
--> all necessary code changes to redo our analysis with parallel_bilby
gwemlightcurve_intructions
--> instructions to use gewmlightcurves for our analysis
posterior_samples
--> all posterior samples from our individual analysis steps
hubble_constant
--> posterior samples on the Hubble constant estimate