Table 2
EOS constraints obtained from our multi-messenger PEs.
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log10 P(2ρsat) | log10 P(4ρsat) |
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Notes. Starting from our agnostic prior set of 10 million EOS, we progressively added the information coming from PSR J0952+0607 (), PSR J0030+0451 and PSR J0740+6620 (NICER), and GW170817 (GW) and AT2017gfo (kN). We report the median and 90% credible intervals of the relevant EOS-dependent properties.
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