Strong lensing time-delay cosmography in the 2020s
T Treu, SH Suyu, PJ Marshall - The Astronomy and Astrophysics Review, 2022 - Springer
Multiply imaged time-variable sources can be used to measure absolute distances as a
function of redshifts and thus determine cosmological parameters, chiefly the Hubble …
function of redshifts and thus determine cosmological parameters, chiefly the Hubble …
Strong lensing by galaxies
T Treu - Annual Review of Astronomy and Astrophysics, 2010 - annualreviews.org
Strong lensing is a powerful tool to address three major astrophysical issues: understanding
the spatial distribution of mass at kiloparsec and subkiloparsec scale, where baryons and …
the spatial distribution of mass at kiloparsec and subkiloparsec scale, where baryons and …
Simulating cosmic structure formation with the gadget-4 code
Numerical methods have become a powerful tool for research in astrophysics, but their utility
depends critically on the availability of suitable simulation codes. This calls for continuous …
depends critically on the availability of suitable simulation codes. This calls for continuous …
H0LiCOW – V. New COSMOGRAIL time delays of HE 0435−1223: H0 to 3.8 per cent precision from strong lensing in a flat ΛCDM model
We present a new measurement of the Hubble Constant H 0 and other cosmological
parameters based on the joint analysis of three multiply imaged quasar systems with …
parameters based on the joint analysis of three multiply imaged quasar systems with …
Five-year wilkinson microwave anisotropy probe* observations: likelihoods and parameters from the Wmap data
This paper focuses on cosmological constraints derived from analysis of WMAP data alone.
A simple ΛCDM cosmological model fits the five-year WMAP temperature and polarization …
A simple ΛCDM cosmological model fits the five-year WMAP temperature and polarization …
A comprehensive analysis of uncertainties affecting the stellar mass–halo mass relation for 0< z< 4
PS Behroozi, C Conroy… - The Astrophysical …, 2010 - iopscience.iop.org
We conduct a comprehensive analysis of the relationship between central galaxies and their
host dark matter halos, as characterized by the stellar mass–halo mass (SM–HM) relation …
host dark matter halos, as characterized by the stellar mass–halo mass (SM–HM) relation …
H0LiCOW – I. H0 Lenses in COSMOGRAIL's Wellspring: program overview
Strong gravitational lens systems with time delays between the multiple images allow
measurements of time-delay distances, which are primarily sensitive to the Hubble constant …
measurements of time-delay distances, which are primarily sensitive to the Hubble constant …
The dark matter of gravitational lensing
We review progress in understanding dark matter by astrophysics, and particularly via the
effect of gravitational lensing. Evidences from many different directions now all imply that five …
effect of gravitational lensing. Evidences from many different directions now all imply that five …
Dissecting the gravitational lens B1608+ 656. II. Precision measurements of the Hubble constant, spatial curvature, and the dark energy equation of state
SH Suyu, PJ Marshall, MW Auger… - The Astrophysical …, 2010 - iopscience.iop.org
Strong gravitational lens systems with measured time delays between the multiple images
provide a method for measuring the" time-delay distance" to the lens, and thus the Hubble …
provide a method for measuring the" time-delay distance" to the lens, and thus the Hubble …
Two accurate time-delay distances from strong lensing: Implications for cosmology
SH Suyu, MW Auger, S Hilbert… - The Astrophysical …, 2013 - iopscience.iop.org
Strong gravitational lenses with measured time delays between the multiple images and
models of the lens mass distribution allow a one-step determination of the time-delay …
models of the lens mass distribution allow a one-step determination of the time-delay …