Table 2.
Future number of kilonovae detected with GW and optical counterparts vs. the expected fractional constraint attainable on H0.
BNS mergers | 1 | 5 | 10 |
---|---|---|---|
![]() |
3% | 1.4% | 1.0% |
Notes. All mergers are assumed to be uniformly distributed within an observable volume with a distance of 150 Mpc, with identical intrinsic luminosities and peculiar velocity uncertainties as AT2017gfo.
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