Table 1 Summary of H0 results.

From: Measuring the Hubble constant with a sample of kilonovae

Kilonova

Kasen—0.25

Kasen—0.1

Bulla—0.25

Bulla—0.1

GW170817

\(7{5}_{-8}^{+9}\)

\(7{8}_{-8}^{+9}\)

\(7{5}_{-7}^{+7}\)

\(7{5}_{-6}^{+6}\)

GRB 060614

\(6{8}_{-16}^{+22}\)

\(6{6}_{-12}^{+13}\)

\(7{1}_{-20}^{+33}\)

\(6{6}_{-11}^{+16}\)

GRB 150101B

\(6{6}_{-20}^{+40}\)

\(7{6}_{-20}^{+39}\)

\(8{9}_{-33}^{+54}\)

\(9{6}_{-38}^{+51}\)

GRB 050709

\(7{8}_{-19}^{+29}\)

\(6{3}_{-11}^{+14}\)

\(6{2}_{-7}^{+9}\)

\(6{1}_{-6}^{+8}\)

GRB 160821B

\(6{4}_{-10}^{+11}\)

\(6{3}_{-9}^{+12}\)

\(6{2}_{-6}^{+8}\)

\(6{2}_{-6}^{+8}\)

Combined

\(71.{9}_{-5.5}^{+6.4}\)

\(73.{8}_{-5.8}^{+6.3}\)

\(69.{9}_{-3.7}^{+3.6}\)

\(71.{2}_{-3.1}^{+3.2}\)

  1. We use units of km s−1 Mpc−1. Individual rows refer to the GRB/GW observations and individual columns to the Kasen et al. and Bulla et al. model assuming a 0.25 and 0.1 mag systematic uncertainty. We note that the GRB individual H0 measurements use the SBF of the host galaxy NGC 499333 to pin the distance.