A novel method of measuring cosmological distances using broad-line regions of quasars
arXiv:2005.10458 · doi:10.1016/j.scib.2020.04.038
Abstract
The absolute distance scale measurements in cosmology have always been an important mission. In particular, in recent years, the Hubble constant tension between the measurements from early and late universe has become a new crisis for cosmology, which calls for new, independent absolute cosmological distance measurements. Recently, a result of measuring the parallax distance to 3C 273 through spectroastrometry and reverberation mapping was reported. We comment on this novel method in this News & Views paper.
3 pages; News & Views, published online in Science Bulletin
References in corpus (3)
Cited by in corpus (11)
- The Gravitational-Wave Physics II: Progress
- Forecast for cosmological parameter estimation with gravitational-wave standard sirens from the LISA-Taiji network
- The Taiji-TianQin-LISA network: Precisely measuring the Hubble constant using both bright and dark sirens
- Synergy between CSST galaxy survey and gravitational-wave observation: Inferring the Hubble constant from dark standard sirens
- Prospects for measuring the Hubble constant and dark energy using gravitational-wave dark sirens with neutron star tidal deformation
- Impacts of gravitational-wave standard siren observations from Einstein Telescope and Cosmic Explorer on weighing neutrinos in interacting dark energy models
- Prospects for probing the interaction between dark energy and dark matter using gravitational-wave dark sirens with neutron star tidal deformation
- Joint constraints on cosmological parameters using future multi-band gravitational wave standard siren observations
- A comprehensive forecast for cosmological parameter estimation using joint observations of gravitational waves and short -ray bursts
- Standard siren cosmology in the era of the 2.5-generation ground-based gravitational wave detectors: bright and dark sirens of LIGO Voyager and NEMO
- Multi-messenger standard-siren cosmology for third-generation gravitational-wave detectors: forecasts considering observations of gamma-ray bursts and kilonovae