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Recently much attention has been paid to the discovery of Hubble's law: the linear relation between the rate of recession of the distant galaxies and distance to them. Though we now mention several names associated with this law instead of…

物理学史与哲学 · 物理学 2015-06-19 Ari Belenkiy

Galton's family heights data has been a preeminent historical dataset in regression analysis, on which the original model and basic results have survived the close scrutiny of statisticians for 125 years. However by revisiting Galton's…

应用统计 · 统计学 2015-08-13 Hao Han , Yeming Ma , Wei Zhu

Hubble's name is associated closely with the idea of an expanding universe as he discovered the relation between the recession velocity and distances of galaxies. Hubble also did a lot of pioneering work on the distribution of galaxies in…

科普物理 · 物理学 2009-04-20 J. S. Bagla

After a brief introduction to the sixteenth and seventeenth century views of the Universe and the nineteenth century paradox of Olbers, we start the history of the cosmic expansion with Hubble's epochal discovery of the recession velocities…

天体物理学 · 物理学 2008-02-15 Matts Roos

A large luminosity--linewidth template sample is now available, improved absorption corrections have been derived, and there are a statistically significant number of galaxies with well determined distances to supply the zero point. A…

天体物理学 · 物理学 2016-01-27 R. Brent Tully

When linear regression generates a relationship between a (dependent) scalar response and one or multiple independent variables, various datasets providing distinct graphical trends can develop resembling relationships based on the same…

统计方法学 · 统计学 2021-08-27 Albert S. Kim

This is the first paper presenting our long-term project aimed at studying the nature of bulges through the analysis of their stellar population gradients. We present deep spectroscopic observations along the minor axis and the data…

天体物理学 · 物理学 2009-11-13 J. Gorgas , P. Jablonka , P. Goudfrooij

An important part of cosmological model fitting relies on correlating distance indicators of objects (for example type Ia supernovae) with their redshift, often illustrated on a Hubble diagram. Comparing the observed correlation with a…

宇宙学与河外天体物理 · 物理学 2019-07-22 Julian Adamek , Chris Clarkson , Louis Coates , Ruth Durrer , Martin Kunz

This paper considers the two-dataset problem, where data are collected from two potentially different populations sharing common aspects. This problem arises when data are collected by two different types of researchers or from two…

统计方法学 · 统计学 2022-09-27 Steven N. MacEachern , Koji Miyawaki

Linear regression is common in astronomical analyses. I discuss a Bayesian hierarchical modeling of data with heteroscedastic and possibly correlated measurement errors and intrinsic scatter. The method fully accounts for time evolution.…

天体物理仪器与方法 · 物理学 2015-10-12 Mauro Sereno

The effect of curvature on the results of fractal analyses of the galaxy distribution is investigated. We show that, if the universe satisfies the criteria of a wide class of parabolic homogeneous models, the observers measuring the fractal…

天体物理学 · 物理学 2009-10-31 Marie-Noëlle Célérier , Reuben Thieberger

The linearity of the Hubble relationship (i.e. between m and z) has been tested for galaxies and supernovea for low redshifts. We have studied this relationship for quasars for data taken from Veron Cetti Catalogue(2003).The data from Veron…

天体物理学 · 物理学 2007-05-23 Sisir Roy , Dhrubajit Datta , Malabika Roy , Menas Kafatos

In general-relativistic cosmological models, the expansion history, matter content, and geometry are closely intertwined. In this brief paper, we clarify the distinction between the effects of geometry and expansion history on the…

天体物理学 · 物理学 2009-11-10 Robert R. Caldwell , Marc Kamionkowski

The correlation between the luminosities and rotation velocities of galaxies can be used to estimate distances to late-type galaxies. It is an appropriate moment to re-evaluate this method given the great deal of new information available.…

天体物理学 · 物理学 2014-10-13 R. Brent Tully , M. J. Pierce

The supernova (SN) Hubble diagram residual contains valuable information on both the present matter power spectrum and its growth history. In this paper we show that this information can be retrieved with precision by combining both…

宇宙学与河外天体物理 · 物理学 2016-05-10 Tiago Castro , Miguel Quartin , Sandra Benitez-Herrera

The purpose of this paper is twofold. On a technical side, we propose an extension of the Hausdorff distance from metric spaces to spaces equipped with asymmetric distance measures. Specifically, we focus on the family of Bregman…

机器学习 · 计算机科学 2025-04-11 Tuyen Pham , Hana Dal Poz Kouřimská , Hubert Wagner

We use comparisons between the shapes of gravitational lens galaxies and models for their mass distributions to derive statistical constraints on the alignment of the mass distribution relative to the observed lens galaxy and on the…

天体物理学 · 物理学 2017-08-23 C. S. Kochanek

Since the pioneering work by Koenker and Bassett (1978), quantile regression models and its applications have become increasingly popular and important for research in many areas. In this paper, a random effects ordinal quantile regression…

统计计算 · 统计学 2016-03-02 Rahim Alhamzawi

The generalised linear model (GLM) is a very important tool for analysing real data in biology, sociology, agriculture, engineering and many other application domain where the relationship between the response and explanatory variables may…

统计方法学 · 统计学 2016-07-04 Abhik Ghosh , Ayanendranath Basu

The morphology of a galaxy has been shown to encode the evolutionary history and correlates strongly with physical properties such as stellar mass, star formation rates and past merger events. While the majority of galaxies in the local…

星系天体物理 · 物理学 2023-02-23 Clár-Bríd Tohill , Steven Bamford , Christopher Conselice
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