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Relevant bibliographies by topics / Galaxy clustering, large-scale structure of Universe

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Academic literature on the topic 'Galaxy clustering, large-scale structure of Universe'

Author: Grafiati

Published: 24 April 2022

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Journal articles on the topic "Galaxy clustering, large-scale structure of Universe"

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Diaferio, Antonaldo. "Ab Initio Formation of Galaxies, Groups and Large-Scale Structure." International Astronomical Union Colloquium 174 (2000): 434–44. http://dx.doi.org/10.1017/s0252921100055421.

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AbstractFor the first time, the combination of semi-analytic modelling of galaxy formation and N-body simulations of cosmic structure formation enables us to model, at the same time, both the photometric and the clustering properties of galaxies. Two Cold Dark Matter Universes provide a reasonable fit to the observed properties of galaxies, groups and clusters, including luminosities, colours, density and velocity biases. We show how the properties of galaxies and groups on small scales are inextricably connected with the global properties of the Universe.

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Heymans, Catherine, and Gong-Bo Zhao. "Large-scale structure probes of modified gravity." International Journal of Modern Physics D 27, no. 15 (2018): 1848005. http://dx.doi.org/10.1142/s021827181848005x.

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Observations of the evolution of large-scale structures in the Universe provides unique tools to confront Einstein’s theory of General Relativity on cosmological scales. We review weak gravitational lensing and galaxy clustering studies, discussing how these can be used in combination in order to constrain a range of different modified gravity theories. We argue that in order to maximise the future information gain from these probes, theoretical effort will be required in order to model the impact of beyond-Einstein gravity in the nonlinear regime of structure formation.

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FANG, LI ZHI. "QUASAR CLUSTERING AND ITS COSMOLOGICAL IMPLICATION." International Journal of Modern Physics A 04, no. 14 (1989): 3477–502. http://dx.doi.org/10.1142/s0217751x89001394.

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The clusterings of quasars and absorption line clouds have been analyzed from the viewpoint of the structure formation of the universe. It was found that the features of quasar clustering are quite different from those of galaxies. These results have already given several meaningful constraints on the structure formation, as follows: (a) quasar clustering is much weaker than in galaxies; (b) large scale structures, such as superclusters, should probably be formed after the epoch z~2; (c) the amplitude of the total density inhomogeneity seems to be less than that of galaxy distribution by at le

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Collins, C. A. "Galaxy Clustering in the Southern Hemisphere." International Astronomical Union Colloquium 148 (1995): 510–21. http://dx.doi.org/10.1017/s0252921100022454.

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AbstractIn this paper some of the major results from the COSMOS and APM digitised galaxy surveys are presented. The main motivation behind these catalogues was to study large-scale structure in the universe. We begin by outlining the importance of such studies to cosmology and discussing the early results from the visually compiled galaxy catalogues. The impact of the digitised catalogues is demonstrated by focussing on three key areas of research; the galaxy-galaxy two-point angular correlation function, the cluster-cluster spatial correlation function, and galaxy number counts.

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Tsaprazi, Eleni, Jens Jasche, Ariel Goobar, et al. "The large-scale environment of thermonuclear and core-collapse supernovae." Monthly Notices of the Royal Astronomical Society 510, no. 1 (2021): 366–72. http://dx.doi.org/10.1093/mnras/stab3525.

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ABSTRACT The new generation of wide-field time-domain surveys has made it feasible to study the clustering of supernova (SN) host galaxies in the large-scale structure (LSS) for the first time. We investigate the LSS environment of SN populations, using 106 dark matter density realisations with a resolution of ∼3.8 Mpc, constrained by the 2M+ + galaxy survey. We limit our analysis to redshift z &lt; 0.036, using samples of 498 thermonuclear and 782 core-collapse SNe from the Zwicky Transient Facility’s Bright Transient Survey and Census of the Local Universe catalogues. We detect clusterin

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Bond, J. Richard. "Structure Constraints from Large Angle CMB Anisotropies." Highlights of Astronomy 9 (1992): 319–21. http://dx.doi.org/10.1017/s1539299600009126.

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Constraints on models of cosmic structure formation that can be drawn from current limits on large angle microwave background anisotropies are now competitive with those from recent small and intermediate angle experiments and are relatively insensitive to the reheating history of the Universe. Here I give limits on Gaussian scale invariant adiabatic fluctuations and describe the role that the large angle results play in constraining models with enhanced large distance galaxy clustering power inferred from correlation function measurements is described.

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de la Torre, Sylvain. "Probing the accelerating Universe with redshift-space distortions in VIPERS." Proceedings of the International Astronomical Union 11, S308 (2014): 617–22. http://dx.doi.org/10.1017/s1743921316010693.

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AbstractWe present the first measurement of the growth rate of structure at z=0.8. It has been obtained from the redshift-space distortions observed in the galaxy clustering pattern in the VIMOS Public Redshift survey (VIPERS) first data release. VIPERS is a large galaxy redshift survey probing the large-scale structure at 0.5 < z < 1.2 with an unprecedented accuracy. This measurement represents a new reference in the distant Universe, which has been poorly explored until now. We obtain σ8 = 0.47 ± 0.08 at z = 0.8 that is consistent with the predictions of standard cosmological models ba

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McLean, B. J., H. Böhringer, R. Burg, R. Giacconi, J. P. Huchra, and W. Voges. "Optical Identification of Rosat All-Sky Survey Galaxy Cluster Candidates." Symposium - International Astronomical Union 161 (1994): 653–57. http://dx.doi.org/10.1017/s0074180900048294.

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Clusters of galaxies are used to study large scale structure and evolution in the universe. The luminosity functions of clusters can be used to investigate their evolutionary effects while their spatial and angular correlation functions are a measure of large-scale clustering. There are, however, many problems with the traditional cluster catalogues that were derived by visual inspection of plate material. The widely used Abell catalogue (Abell 1958) has been shown to have significant problems in homogeneity and completeness (Postman et al. 1986).

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Boyle, BJ. "The Clustering and Evolution of QSOs." Australian Journal of Physics 43, no. 2 (1990): 251. http://dx.doi.org/10.1071/ph900251.

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Recent advances in instrumentation, particularly at the Anglo-Australian Telescope, have greatly increased the number of quaSi-stellar objects (QSOs) identified at faint magnitudes (B> 20 mag) and high redshifts (z> 2.2). As a result, significant progress has been made in the study of QSO clustering and evolution in the last two to three years. This paper reviews the results obtained and discusses their relevance to models of galaxy formation and the large-scale structure of the universe.

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Shao, Xiaoyun, Zhoujian Cao, Xilong Fan, and Shichao Wu. "Probing the Large-scale Structure of the Universe Through Gravitational Wave Observations." Research in Astronomy and Astrophysics 22, no. 1 (2022): 015006. http://dx.doi.org/10.1088/1674-4527/ac32b4.

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Abstract The improvements in the sensitivity of the gravitational wave (GW) network enable the detection of several large redshift GW sources by third-generation GW detectors. These advancements provide an independent method to probe the large-scale structure of the universe by using the clustering of the binary black holes (BBHs). The black hole catalogs are complementary to the galaxy catalogs because of large redshifts of GW events, which may imply that BBHs are a better choice than galaxies to probe the large-scale structure of the universe and cosmic evolution over a large redshift range.

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Dissertations / Theses on the topic "Galaxy clustering, large-scale structure of Universe"

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Baugh, Carlton Martin. "Statistical analysis of large scale structure in the universe." Thesis, University of Oxford, 1994. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.259779.

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Kwan, J., C. Sánchez, J. Clampitt, et al. "Cosmology from large-scale galaxy clustering and galaxy–galaxy lensing with Dark Energy Survey Science Verification data." OXFORD UNIV PRESS, 2017. http://hdl.handle.net/10150/623270.

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We present cosmological constraints from the Dark Energy Survey (DES) using a combined analysis of angular clustering of red galaxies and their cross-correlation with weak gravitational lensing of background galaxies. We use a 139 deg(2) contiguous patch of DES data from the Science Verification (SV) period of observations. Using large-scale measurements, we constrain the matter density of the Universe as Omega(m) = 0.31 +/- 0.09 and the clustering amplitude of the matter power spectrum as sigma(8) = 0.74 +/- 0.13 after marginalizing over seven nuisance parameters and three additional cosmolog

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Wibking, Benjamin Douglas. "Cosmic structure formation on small scales: From non-linear galaxy clustering to the interstellar medium." The Ohio State University, 2019. http://rave.ohiolink.edu/etdc/view?acc_num=osu1561556033289855.

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Rezaie, Mehdi. "Robust Measurements of the Large-Scale Clustering of Galaxy Survey Data." Ohio University / OhioLINK, 2009. http://rave.ohiolink.edu/etdc/view?acc_num=ohiou1626320867298365.

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Rezaie, Mehdi. "Robust Measurements of the Large-Scale Clustering of Galaxy Survey Data." Ohio University / OhioLINK, 2021. http://rave.ohiolink.edu/etdc/view?acc_num=ohiou1626320867298365.

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Hoffmann, Kai Delf. "Cosmology with galaxy clustering." Doctoral thesis, Universitat Autònoma de Barcelona, 2015. http://hdl.handle.net/10803/297700.

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Per constrènyer models cosmològics mitjançant el creixement de les fluctuacions a gran escala de la matèria és cabdal entendre com les galàxies que observem tracen el camp de densitat de tot el conjunt de matèria. La relació entre el camp de densitat de matèria i el de galàxies s'acostuma a aproximar amb una expansió de segon ordre de la funció anomenada bias. La llibertat en els paràmetres d'aquesta funció redueix la informació cosmològica que es pot extreure de les observacions. En aquesta tesi estudiem dos mètodes per determinar els paràmetres del bias independentment del creixement. L'anàl

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Durkalec, Anna. "Properties and evolution of galaxy clustering at 2." Thesis, Aix-Marseille, 2014. http://www.theses.fr/2014AIXM4758/document.

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Cette thèse porte sur l'étude des propriétés et l'évolution de regroupement de galaxies pour les galaxies de la gamme de 22. Je ai pu mesurer la distribution spatiale d'une population générale de galaxie à redshift z~3 pour la première fois avec une grande précision. Je ai quantifié le regroupement de galaxie en estimation et la modélisation de la fonction de corrélation projetée (espace réel) à deux points, pour une population générale de 3022 galaxies. Je ai prolongé les mesures de regroupement à la luminosité et des sous-échantillons de masse sélectionné stellaires. Mes résultats montrent q

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Eggemeier, Alexander. "Challenges and prospects of probing galaxy clustering with three-point statistics." Thesis, University of Sussex, 2018. http://sro.sussex.ac.uk/id/eprint/80679/.

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In this work we explore three-point statistics applied to the large-scale structure in our Universe. Three-point statistics, such as the bispectrum, encode information not accessible via the standard analysis method-the power spectrum-and thus provide the potential for greatly improving current constraints on cosmological parameters. They also present us with additional challenges, and we focus on two of these arising from a measurement as well as modelling point of view. The first challenge we address is the covariance matrix of the bispectrum, as its precise estimate is required when perform

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Hatton, Stephen John. "Probing the large-scale structure of the Universe with future galaxy redshift surveys." Thesis, Durham University, 1999. http://etheses.dur.ac.uk/4494/.

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Several projects are currently underway to obtain large galaxy redshift surveys over the course of the next decade. The aim of this thesis is to study how well the resultant three-dimensional maps of the galaxy distribution will be able to constrain the various parameters of the standard Big Bang cosmology. The work is driven by the need to deal with data of far better quality than has previously been available. Systematic biases in the treatment of existing datasets have been dwarfed by random errors due to the small size of the sample, but this will not be the case with the wealth of data th

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More, James G. "The large scale structure of the universe in pancake models of galaxy formation." Thesis, University of Edinburgh, 1989. http://hdl.handle.net/1842/28659.

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This thesis investigates the evolution of characteristic structures in neutrino or adiabatic baryon-dominated models of galaxy formation. We discuss the collapse of protocluster or protosupercluster clouds in terms of the behaviour of non-rotating, homogeneous triaxial ellipsoids, predicting that galaxies should populate filamentary or quasi-spherical structures rather than the generic flat structures (pancakes). Secondly we have designed a numerical code which allows us to do fast cosmological hydrodynamics. We investigate the effect of explosions on the standard pancake picture for galaxy fo

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Books on the topic "Galaxy clustering, large-scale structure of Universe"

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S, Maurogordato, ed. Clustering in the universe: Proceedings of the XXXth Rencontres de Moriond, Les Arcs, Savoie, France, March 11-18, 1995. Editions Frontières, 1995.

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Peebles, P. J. E. The Large-Scale Structure of the Universe. Princeton University Press, 2020. http://dx.doi.org/10.23943/princeton/9780691209838.001.0001.

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An instant landmark on its publication, this book remains the essential introduction to this vital area of research. Written by one of the world's most esteemed theoretical cosmologists, it provides an invaluable historical introduction to the subject, and an enduring overview of key methods, statistical measures, and techniques for dealing with cosmic evolution. With characteristic clarity and insight, the author focuses on the largest known structures — galaxy clusters — weighing the empirical evidence of the nature of clustering and the theories of how it evolves in an expanding universe. A

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Book chapters on the topic "Galaxy clustering, large-scale structure of Universe"

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Shanks, T., D. Hale-Sutton, and B. J. Boyle. "Observations of Galaxy and QSO Clustering." In Large Scale Structures of the Universe. Springer Netherlands, 1988. http://dx.doi.org/10.1007/978-94-009-2995-1_50.

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Schramm, David N. "Galaxy Formation, Dark Matter and Large Scale Structure." In Dark Matter in the Universe. Springer Netherlands, 1990. http://dx.doi.org/10.1007/978-94-009-1940-2_1.

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Parker, Q. A., H. T. MacGillivray, and S. M. Beard. "Tracing Large-Scale Structure with Galaxy Objective-Prism Spectra." In Large Scale Structures of the Universe. Springer Netherlands, 1988. http://dx.doi.org/10.1007/978-94-009-2995-1_80.

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Shaver, P. A. "Quasar Clustering and the Evolution of Structure." In Large Scale Structures of the Universe. Springer Netherlands, 1988. http://dx.doi.org/10.1007/978-94-009-2995-1_49.

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Lambas, D. G., E. J. Groth, and P. J. E. Peebles. "Statistics of Galaxy Orientations: Morphology and the Large Scale Structure." In Large Scale Structures of the Universe. Springer Netherlands, 1988. http://dx.doi.org/10.1007/978-94-009-2995-1_102.

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Schramm, David N. "The Consistency Problems of Large Scale Structure, Dark Matter, and Galaxy Formation." In Gauge Theory and the Early Universe. Springer Netherlands, 1988. http://dx.doi.org/10.1007/978-94-009-3059-9_9.

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Peebles, P. J. E. "Homogeneity and Clustering." In The Large-Scale Structure of the Universe. Princeton University Press, 2020. http://dx.doi.org/10.23943/princeton/9780691209838.003.0001.

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This chapter traces the history of the development of ideas on the large-scale structure of the universe. Modern discussions of the nature of the large-scale matter distribution can be traced back to three central ideas. In 1917, Albert Einstein argued that a closed homogeneous world model fits very well into general relativity theory and the requirements of Mach's principle. In 1926, Edwin Hubble showed that the large-scale distribution of galaxies is close to uniform with no indication of an edge or boundary. In 1927, Georges Lemaître showed that the uniform distribution of galaxies fits very well with the pattern of galaxy redshifts. The chapter then assesses several questions. The first is whether the universe really is homogeneous. Could the homogeneity of the universe have been deduced ahead of time from general principles? Or might it be a useful guide to new principles? It also asks how clustering evolves in an expanding universe, what its origin is, and what this reveals about the nature of the universe.

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Peebles, P. J. E. "Dynamics and Statistics." In The Large-Scale Structure of the Universe. Princeton University Press, 2020. http://dx.doi.org/10.23943/princeton/9780691209838.003.0004.

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This chapter studies how the n-point correlation functions have proved useful not only as descriptive statistics but also as dynamic variables in the Newtonian theory of the evolution of clustering. It generalizes the functions to mass correlation functions in position and momentum, and derives the BBGKY hierarchy of equations for their evolution. This yields a new way to analyze the evolution of mass clustering in an expanding universe. Of course, the main interest in the approach comes from the thought that the observed galaxy correlation functions may yield useful approximations to the mass correlation functions, so the observations may provide boundary values for the dynamical theory of evolution of the mass correlation functions. The test will be whether one can find a consistent theory for the joint distributions in galaxy positions and velocities.

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"GALAXY MOTIONS AND CLUSTERING." In Cosmological Inflation and Large-Scale Structure. Cambridge University Press, 2000. http://dx.doi.org/10.1017/cbo9781139175180.011.

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"HOMOGENEITY AND CLUSTERING." In The Large-Scale Structure of the Universe. Princeton University Press, 2020. http://dx.doi.org/10.2307/j.ctvxrpz4n.5.

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