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Peculiar velocities are the motions of galaxies due to the gravitational influence of large-scale structure, and thus are an important cosmological probe of the underlying matter density field. In recent years the number of surveys designed…

宇宙学与河外天体物理 · 物理学 2025-02-19 Ryan J. Turner

In recent years, significant progress has been made in building new galaxy clusters samples, at low and high redshifts, from wide-area surveys, particularly exploiting the Sunyaev--Zel'dovich (SZ) effect. A large effort is underway to…

A new component of the Universe which leads to an accelerated cosmic expansion is found from the measurements of distances to high-redshift type Ia supernovae. We describe the method and the results obtained from the observations of distant…

天体物理学 · 物理学 2007-05-23 Bruno Leibundgut , Gertrud Contardo , Patrick Woudt , Jason Spyromilio

We extend the general relativistic description of galaxy clustering developed in Yoo, Fitzpatrick, and Zaldarriaga (2009). For the first time we provide a fully general relativistic description of the observed matter power spectrum and the…

宇宙学与河外天体物理 · 物理学 2014-11-21 Jaiyul Yoo

The expansion of the universe causes spacetime curvature, distinguishing between distances measured along and transverse to the line of sight. The ratio of these distances, e.g. the cosmic shear distortion of a sphere defined by…

天体物理学 · 物理学 2009-11-07 Eric V. Linder

Cosmology in the near future promises a measurement of the sum of neutrino masses, a fundamental Standard Model parameter, as well as substantially-improved constraints on the dark energy. We use the shape of the BOSS redshift-space galaxy…

宇宙学与河外天体物理 · 物理学 2019-07-09 Amol Upadhye

In this manuscript I review the mathematics and physics that underpins recent work using the clustering of galaxies to derive cosmological model constraints. I start by describing the basic concepts, and gradually move on to some of the…

天体物理学 · 物理学 2009-07-28 Will J. Percival

Modified gravity theories may provide an alternative to dark energy to explain cosmic acceleration. We argue that the observational program developed to test dark energy needs to be augmented to capture new tests of gravity on astrophysical…

宇宙学与河外天体物理 · 物理学 2015-05-27 Bhuvnesh Jain

Our knowledge of the Galaxy is being revolutionised by a series of photometric, spectroscopic and astrometric surveys. Already an enormous body of data is available from completed surveys, and data of ever increasing quality and richness…

星系天体物理 · 物理学 2015-05-27 James Binney

The discovery of cosmic acceleration has stimulated theorists to consider dark energy or modifications to Einstein's General Relativity as possible explanations. The last decade has seen advances in theories that go beyond smooth dark…

Euclid will observe 15 000 deg$^2$ of the darkest sky, in regions free of contamination by light from our Galaxy and our Solar System. Three "Euclid Deep Fields" surveys covering around 40 deg$^2$ in total will extend the scientific scope…

宇宙学与河外天体物理 · 物理学 2022-11-17 Isaac Tutusaus , Jenny G. Sorce , Antonino Troja

The results from the Supernova Cosmology Project indicate a relation between cosmic distance and redshift that corresponds to an accelerating Universe, and, as a consequence, the presence of an energy component with negative pressure. This…

天体物理学 · 物理学 2007-05-23 Daniel Enstrom , Sverker Fredriksson , Johan Hansson

Over the last decade, cosmological observations have attained a level of precision which allows for detailed comparison with theoretical predictions. In this paper, we briefly review some studies of the current and prospected constraints…

科普物理 · 物理学 2007-05-23 Monique Signore , Denis Puy

We focus on uncertainties in supernova measurements, in particular of individual magnitudes and redshifts, to review to what extent supernovae measurements of the expansion history of the universe are likely to allow us to constrain a…

天体物理学 · 物理学 2011-05-12 Lawrence M. Krauss , Katherine Jones-Smith , Dragan Huterer

Eigenmode analysis is one of the most promising methods of analyzing large data sets in ongoing and near-future galaxy surveys. In such analyses, a fast evaluation of the correlation matrix in arbitrary cosmological models is crucial. The…

天体物理学 · 物理学 2009-11-10 Takahiko Matsubara , Alexander S. Szalay , Adrian C. Pope

Looking ahead to the next decade and imagining the landscape of astronomy in 2020, it is clear that astronomical surveys, large and small, plus extensive follow-up projects, will be a great engine of progress in our profession. Surveys have…

宇宙学与河外天体物理 · 物理学 2009-04-20 Steven T. Myers

Estimating galaxy redshifts is crucial for constraining key physical quantities like those in the equation of state of dark energy. Modern telescopes such as the James Webb Space Telescope, the Euclid Space Telescope, and the NASA Nancy…

天体物理仪器与方法 · 物理学 2026-03-27 Alexander Kuhn , Bonnabelle Zabelle , Sara Algeri , Galin L. Jones , Claudia Scarlata

This paper reviews statistical methods recently developed to reconstruct and analyze dark matter mass maps from weak lensing observations. The field of weak lensing is motivated by the observations made in the last decades showing that the…

宇宙学与河外天体物理 · 物理学 2015-05-14 S. Pires , J. -L. Starck , A. Refregier

The recent measurement of the gravitational redshifts of galaxies in galaxy clusters by Wojtak et al. has opened a new observational window on dark matter and modified gravity. By stacking clusters this determination effectively used the…

宇宙学与河外天体物理 · 物理学 2015-06-15 Rupert A. C. Croft

We demonstrate that observations lacking reliable redshift information, such as photometric and radio continuum surveys, can produce robust measurements of cosmological parameters when empowered by clustering-based redshift estimation. This…

宇宙学与河外天体物理 · 物理学 2017-05-10 Ely D. Kovetz , Alvise Raccanelli , Mubdi Rahman