In the data files containing posterior samples, the masses are given directly in
the source frame, accounting for redshift by dividing the measured "redshifted" 
masses by (1+z). Here, we have taken the redshift z=0.0099 to be constant across 
all samples, equal to the geocentric redshift of NGC 4993 at the time of the event, 
based on the MUSE/VLT measurement.


Figure 1 data
-----

 * EoS-insensitive_posterior_samples.dat : posterior samples for source masses, 
   tidal deformabilities and derived radii for the two NSs, using the 
   EOS-insensitive relations method; Figure 1 shows 2-D joint posteriors of 
   dimensionless tidal deformabilities (Lambda1, Lambda2) (columns 3 and 4)

 * Parametrized-EoS_maxmass_posterior_samples.dat : posterior samples for source
   masses, tidal deformabilities and radii for the two NSs, using the 
   Parametrized-EOS method with the requirement that the EOS must support NS 
   masses of 1.97 M_\odot; Figure 1 shows 2-D joint posteriors of dimensionless 
   tidal deformabilities (Lambda1, Lambda2) (columns 3 and 4)

 * Parametrized-EoS_nomaxmass_posterior_samples.dat : posterior samples for 
   source masses, tidal deformabilities and radii for the two NSs, using the 
   Parametrized-EOS method without any requirement on the maximum mass supported
   by the EOS; Figure 1 shows 2-D joint posteriors of dimensionless tidal 
   deformabilities (Lambda1, Lambda2) (columns 3 and 4)


Figure 2 data
-----

 * Pressure_density_credible_levels.dat : symmetric 90% and 50% confidence 
   intervals of (log10) pressure as a function of (log10) density, using the 
   Parametrized-EOS method; both quantities are given in cgs units, density 
   in g/cm^3, pressure in dyn/cm^2


Figure 3 data
-----

 * EoS-insensitive_posterior_samples.dat : posterior samples for source masses, 
   tidal deformabilities and derived radii for the two NSs, using the 
   EOS-insensitive relations method; Figure 3 shows 2-D joint posteriors of 
   radii [km] and intrinsic masses [M_\odot] for each NS 
   (m1_source_frame_Msun, Radius1_km), (m2_source_frame_Msun, Radius2_km) (columns 1-5, 2-6)

 * Parametrized-EoS_maxmass_posterior_samples.dat : posterior samples for source
   masses, tidal deformabilities and radii for the two NSs, using the 
   Parametrized-EOS method with the requirement that the EOS must support NS 
   masses of 1.97 M_\odot; Figure 3 shows 2-D joint posteriors of 
   radii [km] and intrinsic masses [M_\odot] for each NS 
   (m1_source_frame_Msun, Radius1_km), (m2_source_frame_Msun, Radius2_km) (columns 1-5, 2-6)

 * Parametrized-EoS_nomaxmass_posterior_samples.dat : posterior samples for 
   source masses, tidal deformabilities and radii for the two NSs, using the 
   Parametrized-EOS method without any requirement on the maximum mass supported
   by the EOS; Figure 3 shows 2-D joint posteriors of radii [km] and intrinsic 
   masses [M_\odot] for each NS (m1_source_frame_Msun, Radius1_km),
   (m2_source_frame_Msun, Radius2_km) (columns 1-5, 2-6)