Table 2.
Open in new tab

Hubble constant measurements found with the dark sirens from the three LIGO/Virgo runs and the bright siren GW170817. All priors are flat in the range [20, 140]. The uncertainty from the flat prior is derived by assuming the same H0 maximum found in the analysis. Quoted uncertainties represent 68 per cent HDI around the maximum of the posterior. The ‘|$\sigma _{H_0}/\sigma _{\rm prior}$|’ column shows the 68 per cent CI from the posterior divided by 68 per cent CI of the prior width.

Event|$H_0\, \left(\rm {km\, s^{-1}\, Mpc^{-1}}\right)$||$\sigma _{H_0}\, \left(\rm {km s^{-1} Mpc^{-1}}\right)$||$\sigma _{H_0}/\sigma _{\rm prior}$|Reference
GW190924|$\_$|021846|$70.4^{+54.7}_{-15.1}$|34.985 %This work
GW200202|$\_$|154313|$51.2^{+61.6}_{-11.8}$|36.790 %This work
GW170817—bright|$68.8^{+17.30}_{-7.63}$|12.330 %Nicolaou et al. (2020)
GW190814|$78^{+57}_{-13}$|3586 %Palmese et al. (2020)
GW190924 + GW200202|$60.33^{+55.79}_{-13.61}$|34.785 %This work
GW190814 + GW170814|$77^{+41}_{-22}$|31.577 %Palmese et al. (2020)
8 dark sirens|$79.8^{+19.1}_{-12.4}$|15.839 %Palmese et al. (2023)
10 dark sirens|$76.00^{+17.64}_{-13.45}$|15.5538 %This work
Event|$H_0\, \left(\rm {km\, s^{-1}\, Mpc^{-1}}\right)$||$\sigma _{H_0}\, \left(\rm {km s^{-1} Mpc^{-1}}\right)$||$\sigma _{H_0}/\sigma _{\rm prior}$|Reference
GW190924|$\_$|021846|$70.4^{+54.7}_{-15.1}$|34.985 %This work
GW200202|$\_$|154313|$51.2^{+61.6}_{-11.8}$|36.790 %This work
GW170817—bright|$68.8^{+17.30}_{-7.63}$|12.330 %Nicolaou et al. (2020)
GW190814|$78^{+57}_{-13}$|3586 %Palmese et al. (2020)
GW190924 + GW200202|$60.33^{+55.79}_{-13.61}$|34.785 %This work
GW190814 + GW170814|$77^{+41}_{-22}$|31.577 %Palmese et al. (2020)
8 dark sirens|$79.8^{+19.1}_{-12.4}$|15.839 %Palmese et al. (2023)
10 dark sirens|$76.00^{+17.64}_{-13.45}$|15.5538 %This work
Table 2.
Open in new tab

Hubble constant measurements found with the dark sirens from the three LIGO/Virgo runs and the bright siren GW170817. All priors are flat in the range [20, 140]. The uncertainty from the flat prior is derived by assuming the same H0 maximum found in the analysis. Quoted uncertainties represent 68 per cent HDI around the maximum of the posterior. The ‘|$\sigma _{H_0}/\sigma _{\rm prior}$|’ column shows the 68 per cent CI from the posterior divided by 68 per cent CI of the prior width.

Event|$H_0\, \left(\rm {km\, s^{-1}\, Mpc^{-1}}\right)$||$\sigma _{H_0}\, \left(\rm {km s^{-1} Mpc^{-1}}\right)$||$\sigma _{H_0}/\sigma _{\rm prior}$|Reference
GW190924|$\_$|021846|$70.4^{+54.7}_{-15.1}$|34.985 %This work
GW200202|$\_$|154313|$51.2^{+61.6}_{-11.8}$|36.790 %This work
GW170817—bright|$68.8^{+17.30}_{-7.63}$|12.330 %Nicolaou et al. (2020)
GW190814|$78^{+57}_{-13}$|3586 %Palmese et al. (2020)
GW190924 + GW200202|$60.33^{+55.79}_{-13.61}$|34.785 %This work
GW190814 + GW170814|$77^{+41}_{-22}$|31.577 %Palmese et al. (2020)
8 dark sirens|$79.8^{+19.1}_{-12.4}$|15.839 %Palmese et al. (2023)
10 dark sirens|$76.00^{+17.64}_{-13.45}$|15.5538 %This work
Event|$H_0\, \left(\rm {km\, s^{-1}\, Mpc^{-1}}\right)$||$\sigma _{H_0}\, \left(\rm {km s^{-1} Mpc^{-1}}\right)$||$\sigma _{H_0}/\sigma _{\rm prior}$|Reference
GW190924|$\_$|021846|$70.4^{+54.7}_{-15.1}$|34.985 %This work
GW200202|$\_$|154313|$51.2^{+61.6}_{-11.8}$|36.790 %This work
GW170817—bright|$68.8^{+17.30}_{-7.63}$|12.330 %Nicolaou et al. (2020)
GW190814|$78^{+57}_{-13}$|3586 %Palmese et al. (2020)
GW190924 + GW200202|$60.33^{+55.79}_{-13.61}$|34.785 %This work
GW190814 + GW170814|$77^{+41}_{-22}$|31.577 %Palmese et al. (2020)
8 dark sirens|$79.8^{+19.1}_{-12.4}$|15.839 %Palmese et al. (2023)
10 dark sirens|$76.00^{+17.64}_{-13.45}$|15.5538 %This work
Close
This Feature Is Available To Subscribers Only

Sign In or Create an Account

Close

This PDF is available to Subscribers Only

View Article Abstract & Purchase Options

For full access to this pdf, sign in to an existing account, or purchase an annual subscription.

Close