Stochastic gravitational wave backgrounds
N Christensen - Reports on Progress in Physics, 2018 - iopscience.iop.org
A stochastic background of gravitational waves could be created by the superposition of a
large number of independent sources. The physical processes occurring at the earliest …
large number of independent sources. The physical processes occurring at the earliest …
Cosmic microwave background anisotropies
W Hu, S Dodelson - Annual Review of Astronomy and …, 2002 - annualreviews.org
▪ Abstract Cosmic microwave background (CMB) temperature anisotropies have and will
continue to revolutionize our understanding of cosmology. The recent discovery of the …
continue to revolutionize our understanding of cosmology. The recent discovery of the …
First-year Wilkinson Microwave Anisotropy Probe (WMAP)* observations: determination of cosmological parameters
ABSTRACT WMAP precision data enable accurate testing of cosmological models. We find
that the emerging standard model of cosmology, a flat Λ-dominated universe seeded by a …
that the emerging standard model of cosmology, a flat Λ-dominated universe seeded by a …
Three-year Wilkinson Microwave Anisotropy Probe (WMAP) observations: implications for cosmology
A simple cosmological model with only six parameters (matter density, Ω mh 2, baryon
density, Ω bh 2, Hubble constant, H 0, amplitude of fluctuations, σ 8, optical depth, τ, and a …
density, Ω bh 2, Hubble constant, H 0, amplitude of fluctuations, σ 8, optical depth, τ, and a …
Detection of the baryon acoustic peak in the large-scale correlation function of SDSS luminous red galaxies
We present the large-scale correlation function measured from a spectroscopic sample of
46,748 luminous red galaxies from the Sloan Digital Sky Survey. The survey region covers …
46,748 luminous red galaxies from the Sloan Digital Sky Survey. The survey region covers …
Cosmological parameters from CMB and other data: A Monte Carlo approach
A Lewis, S Bridle - Physical Review D, 2002 - APS
We present a fast Markov chain Monte Carlo exploration of cosmological parameter space.
We perform a joint analysis of results from recent cosmic microwave background (CMB) …
We perform a joint analysis of results from recent cosmic microwave background (CMB) …
New Hubble space telescope discoveries of type Ia supernovae at z≥ 1: narrowing constraints on the early behavior of dark energy
AG Riess, LG Strolger, S Casertano… - The Astrophysical …, 2007 - iopscience.iop.org
We have discovered 21 new Type Ia supernovae (SNe Ia) with the Hubble Space Telescope
(HST) and have used them to trace the history of cosmic expansion over the last 10 billion yr …
(HST) and have used them to trace the history of cosmic expansion over the last 10 billion yr …
Constraints on the equation of state of dark energy and the Hubble constant from stellar ages and the cosmic microwave background
We place constraints on the redshift-averaged, effective value of the equation of state of dark
energy, w, using only the absolute ages of Galactic stars and the observed position of the …
energy, w, using only the absolute ages of Galactic stars and the observed position of the …
First-year Wilkinson microwave anisotropy probe (wmap)* observations: parameter estimation methodology
We describe our methodology for comparing the Wilkinson Microwave Anisotropy Probe
(WMAP) measurements of the cosmic microwave background (CMB) and other …
(WMAP) measurements of the cosmic microwave background (CMB) and other …
Quantifying the uncertainty in the orbits of extrasolar planets
EB Ford - The Astronomical Journal, 2005 - iopscience.iop.org
Precise radial velocity measurements have led to the discovery of∼ 100 extrasolar
planetary systems. We investigate the uncertainty in the orbital solutions that have been …
planetary systems. We investigate the uncertainty in the orbital solutions that have been …