Results 171 to 180 of about 11,925 (196)

Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Resolving the hot and ionized Universe through the Sunyaev-Zeldovich effect. [PDF]

open access: yesOpen Res Eur
Di Mascolo L   +25 more
europepmc   +1 more source

The Hubble Constant. [PDF]

open access: yesLiving Rev Relativ, 2007
Jackson N.
europepmc   +1 more source

Gravitational Lensing in Astronomy. [PDF]

open access: yesLiving Rev Relativ, 1998
Wambsganss J.
europepmc   +1 more source

Photometric redshift uncertainties in weak gravitational lensing shear analysis: models and marginalization

open access: yesMonthly Notices of the Royal Astronomical Society, 2022
ABSTRACT Recovering credible cosmological parameter constraints in a weak lensing shear analysis requires an accurate model that can be used to marginalize over nuisance parameters describing potential sources of systematic uncertainty, such as the uncertainties on the sample redshift distribution n(z).
Tianqing Zhang   +2 more
exaly   +3 more sources

im3shape: a maximum likelihood galaxy shear measurement code for cosmic gravitational lensing [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2013
We present and describe im3shape, a new publicly available galaxy shape measurement code for weak gravitational lensing shear. im3shape performs a maximum likelihood fit of a bulge-plus-disc galaxy model to noisy images, incorporating an applied point spread function.
Joe Zuntz   +2 more
exaly   +3 more sources

Strong gravitational lensing’s ‘external shear’ is not shear [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society
ABSTRACT The distribution of mass in galaxy-scale strong gravitational lenses is often modelled as an elliptical power-law plus ‘external shear’, which notionally accounts for neighbouring galaxies and cosmic shear along our line of sight.
Amy Etherington   +2 more
exaly   +6 more sources

Weak gravitational lensing shear measurement with FPFS: analytical mitigation of noise bias and selection bias [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2022
ABSTRACT Dedicated ‘Stage IV’ observatories will soon observe the entire extragalactic sky, to measure the ‘cosmic shear’ distortion of galaxy shapes by weak gravitational lensing. To measure the apparent shapes of those galaxies, we present an improved version of the Fourier Power Function Shapelets (FPFS) shear measurement method. This
Xiangchong Li, Yin Li, Richard J Massey
exaly   +5 more sources

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