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相关论文: Bias Minimisation in POTENT

200 篇论文

We present an improved POTENT method for reconstructing the velocity and mass density fields from radial peculiar velocities, test it with mock catalogs, and apply it to the Mark III Catalog. Method improvments: (a) inhomogeneous Malmquist…

天体物理学 · 物理学 2009-10-31 A. Dekel , A. Eldar , T. Kolatt , A. Yahil , J. A. Willick , S. M. Faber , S. Courteau , D. Burstein

In this paper we review the two main approaches to the problem of Malmquist bias which have been adopted in the cosmology literature, and show how these two formulations of the problem represent fundamentally different views of the nature…

天体物理学 · 物理学 2007-05-23 Martin A. Hendry , John F. L. Simmons , Andrew M. Newsam

Maps of the peculiar velocity field derived from distance relations are affected by Malmquist type bias and selection effects. Because of the large number of interdependent effects, they are in most cases difficult to treat analytically.…

We investigate the effect of using different distance estimators on the recovery of the peculiar velocity field of galaxies using Potent. An inappropriate choice of distance estimator will give rise to spurious flows. We discuss methods of…

天体物理学 · 物理学 2007-05-23 Andrew Newsam , John F. L. Simmons , Martin Hendry

Methods for inferring the velocity field from the peculiar velocity data are described and applied to old and newer data. Inhomogeneous Malmquist bias and ways to avoid it are discussed and utilized. We infer that these biases are probably…

天体物理学 · 物理学 2007-05-23 Albert Stebbins

Galaxy peculiar velocities are excellent cosmological probes provided that biases inherent to their measurements are contained before any study. This paper proposes a new algorithm based on an object point process model whose probability…

宇宙学与河外天体物理 · 物理学 2023-11-01 Jenny G. Sorce , Radu S. Stoica , Elmo Tempel

Cosmological implications of the observed large-scale peculiar velocities are reviewed, alone or combined with redshift surveys and CMB data. The latest version of the POTENT method for reconstructing the underlying three-dimensional…

天体物理学 · 物理学 2007-05-23 Avishai Dekel

The mass density field in the local universe, recovered by the POTENT method from peculiar velocities of $\sim$3000 galaxies, is compared with the density field of optically-selected galaxies. Both density fields are smoothed with a…

天体物理学 · 物理学 2015-06-24 M. J. Hudson , A. Dekel , S. Courteau , S. M. Faber , J. A. Willick

Galaxy distances and derived radial peculiar velocity catalogs constitute valuable datasets to study the dynamics of the Local Universe. However, such catalogs suffer from biases whose effects increase with the distance. Malmquist biases…

宇宙学与河外天体物理 · 物理学 2015-05-20 Jenny G. Sorce

We describe a new method of overcoming problems inherent in peculiar velocity surveys by using data compression as a filter with which to separate large-scale, linear flows from small-scale noise that biases the results systematically. We…

天体物理学 · 物理学 2007-05-23 Hume A Feldman , Richard Watkins , Adrian Melott , Will Chambers

We present a forward-modelled velocity field reconstruction algorithm that performs the reconstruction of the mass density field using only peculiar velocity data. Our method consistently accounts for the inhomogeneous Malmquist bias using…

宇宙学与河外天体物理 · 物理学 2023-03-01 Supranta S. Boruah , Guilhem Lavaux , Michael J. Hudson

Although Potent purports to use only radial velocities in reconstructing the potential velocity field of galaxies, the derivation of transverse components is implicit in the smoothing procedures adopted. Thus the possibility arises of using…

天体物理学 · 物理学 2007-05-23 J. F. L. Simmons , A. Newsam , M. A. Hendry

We study the implicit bias of generic optimization methods, such as mirror descent, natural gradient descent, and steepest descent with respect to different potentials and norms, when optimizing underdetermined linear regression or…

机器学习 · 统计学 2020-06-24 Suriya Gunasekar , Jason Lee , Daniel Soudry , Nathan Srebro

The large-scale dynamics of matter is inferred from the observed peculiar velocities of galaxies via the POTENT procedure. The smoothed fields of velocity and mass-density fluctuations are recovered from the current data of about 3000…

天体物理学 · 物理学 2007-05-23 Avishai Dekel

Although Potent purports to use only radial velocities in retrieving the potential velocity field of galaxies, the derivation of transverse components is implicit in the smoothing procedures. Thus the possibility of using nonradial line…

天体物理学 · 物理学 2007-05-23 John F. L. Simmons , Andrew Newsam , Martin Hendry

Given an irrotational (vorticity free) velocity field in real space, we prove that, in the distant observer limit and in the absence of multi-valued zones, the associated velocity field in redshift space is also irrotational. The proof does…

天体物理学 · 物理学 2009-10-31 Michal Chodorowski , Adi Nusser

In recent years, random matrices have come to play a major role in computational mathematics, but most of the classical areas of random matrix theory remain the province of experts. Over the last decade, with the advent of matrix…

概率论 · 数学 2015-01-08 Joel A. Tropp

The Monte Carlo Hamiltonian method developed recently allows to investigate ground state and low-lying excited states of a quantum system, using Monte Carlo algorithm with importance sampling. However, conventional MC algorithm has some…

高能物理 - 格点 · 物理学 2018-01-17 Xiang-Qian Luo , Xiao-Ni Cheng , Helmut Kroger

Analyses of peculiar velocity surveys face several challenges, including low signal--to--noise in individual velocity measurements and the presence of small--scale, nonlinear flows. This is the second in a series of papers in which we…

天体物理学 · 物理学 2009-11-07 Hume A. Feldman , Richard Watkins , Adrian L. Melott , Scott W. Chambers

We apply an iterative reconstruction method to galaxy mocks in redshift space obtained from $N$-body simulations. Comparing the two-point correlation functions for the reconstructed density field, we find that although the performance is…

宇宙学与河外天体物理 · 物理学 2019-06-26 Ryuichiro Hada , Daniel J. Eisenstein
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