Open Access
Table A.1
Summary of the parameters used to describe the GW signal of BNS in this paper, together with the prior range used when sampling from the posterior probability.
| Parameter | Description | Units | Prior range |
|---|---|---|---|
| m1 | detector–frame primary mass | M⊙ | (0, +∞) |
| m2 | detector–frame secondary mass | M⊙ | (0, m1] |
| dL | luminosity distance | Gpc | (0, +∞) |
| θ, ϕ | polar and azimutal sky angles | rad | [0, π], [0, 2π] |
| ι | inclination angle w.r.t. orbital angular momentum | rad | [0, π] |
| ψ | polarization angle | rad | [0, π] |
| tc | time of coalescence GMST | day | [0, 1] |
| Φc | phase at coalescence | rad | [0, 2π] |
| χi,z | spin component of object i = {1, 2} along axis z | – | [−1, 1] |
| Λi | adimensional tidal deformability of object i = {1, 2} | – | [0, +∞) |
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