1 code implementation • 19 Dec 2019 • Stephen M. Feeney, Benjamin D. Wandelt, Melissa K. Ness
With this in mind, we introduce SSSpaNG: a data-driven Gaussian Process model of stellar spectra.
Solar and Stellar Astrophysics Astrophysics of Galaxies Instrumentation and Methods for Astrophysics
1 code implementation • 28 Nov 2018 • Daniel J. Mortlock, Stephen M. Feeney, Hiranya V. Peiris, Andrew R. Williamson, Samaya M. Nissanke
Gravitational wave (GW) observations of binary neutron star (BNS) mergers can be used to measure luminosity distances and hence, when coupled with estimates for the mergers' host redshifts, infer the Hubble constant, $H_0$.
Cosmology and Nongalactic Astrophysics
1 code implementation • 9 Feb 2018 • Stephen M. Feeney, Hiranya V. Peiris, Andrew R. Williamson, Samaya M. Nissanke, Daniel J. Mortlock, Justin Alsing, Dan Scolnic
The Hubble constant ($H_0$) estimated from the local Cepheid-supernova (SN) distance ladder is in 3-$\sigma$ tension with the value extrapolated from cosmic microwave background (CMB) data assuming the standard cosmological model.
Cosmology and Nongalactic Astrophysics
1 code implementation • 30 Jun 2017 • Stephen M. Feeney, Daniel J. Mortlock, Niccolò Dalmasso
Estimates of the Hubble constant, $H_0$, from the distance ladder and the cosmic microwave background (CMB) differ at the $\sim$3-$\sigma$ level, indicating a potential issue with the standard $\Lambda$CDM cosmology.
Cosmology and Nongalactic Astrophysics
