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Relevant bibliographies by topics / Millenium simulation / Dissertations / Theses

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Dissertations / Theses on the topic 'Millenium simulation'

Author: Grafiati

Published: 4 June 2021

Last updated: 16 February 2022

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1

Hilbert, Stefan Johannes. "Ray-Tracing through the Millennium Simulation." Diss., lmu, 2008. http://nbn-resolving.de/urn:nbn:de:bvb:19-85684.

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2

Kitzbichler, Manfred G. "Galaxy formation and evolution in the Millennium Simulation." Diss., lmu, 2008. http://nbn-resolving.de/urn:nbn:de:bvb:19-95401.

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3

Ramamonjisoa, Fidy Andriamanankasina. "Modelling radio galaxies in the Millennium simulation: SKA/MeerKAT sources and CMB contaminants." University of the Western Cape, 2010. http://hdl.handle.net/11394/2944.

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Magister Scientiae - MSc<br>We investigate the modelling of radio galaxies within a semi-analytic framework in the Millennium Simulation of the Virgo Consortium. The aim is to assess the radio sources contamination of Sunyaev-Zeldovich (SZ) signatures of clusters of galaxies in Cosmic Microwave Background (CMB) experiments. The modelling is also relevant to the Karoo Array Telescope (MeerKAT) and the Square Kilometre Array (SKA) science. The semi-analytical model consists of N-body simulation, the Millennium Run to trace the merger history of dark matter haloes within the Λ Cold Dark Matter (Λ

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4

Parsons, Luke A., Garrison R. Loope, Jonathan T. Overpeck, Toby R. Ault, Ronald Stouffer, and Julia E. Cole. "Temperature and Precipitation Variance in CMIP5 Simulations and Paleoclimate Records of the Last Millennium." AMER METEOROLOGICAL SOC, 2017. http://hdl.handle.net/10150/626270.

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Accurate assessments of future climate impacts require realistic simulation of interannual-century-scale temperature and precipitation variability. Here, well-constrained paleoclimate data and the latest generation of Earth system model data are used to evaluate the magnitude and spatial consistency of climate variance distributions across interannual to centennial frequencies. It is found that temperature variance generally increases with time scale in patterns that are spatially consistent among models, especially over the mid-and high-latitude oceans. However, precipitation is similar to wh

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5

Dondlinger, Mary Jo Warren Scott J. "The global village playground a qualitative case study of designing an ARG as a capstone learning experience /." [Denton, Tex.] : University of North Texas, 2009. http://digital.library.unt.edu/permalink/meta-dc-10995.

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6

Pyrina, Maria [Verfasser], and Eduardo [Akademischer Betreuer] Zorita. "North Atlantic Ocean decadal variability over the past millennium from climate model simulations and proxy based reconstructions / Maria Pyrina ; Betreuer: Eduardo Zorita." Hamburg : Staats- und Universitätsbibliothek Hamburg, 2017. http://d-nb.info/1136719946/34.

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7

Milkeraitis, Martha. "Optical galaxy cluster detection and weak gravitational lensing derived galaxy cluster mass functions : the development of a new algorithm and its application to the Millennium Simulation, CFHTLS-Deep, and CFHTLS-Wide surveys." Thesis, University of British Columbia, 2011. http://hdl.handle.net/2429/38130.

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Hierarchical structure formation and the λCDM model of the Universe reveal that large structures, such as galaxy clusters, form from the aggregation and merging of smaller structures over time. Exploring the morphologies and distribution of galaxy clusters enables the identification of processes that affect this growth, including the significant role of dark matter in structure formation. The particle constituting dark matter remains unknown and current experimental searches for it abound. Weak gravitational lensing (WL) is an observational astronomy technique that can successfully measure dar

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8

Dondlinger, Mary Jo. "The Global Village Playground: A qualitative case study of designing an ARG as a capstone learning experience." Thesis, University of North Texas, 2009. https://digital.library.unt.edu/ark:/67531/metadc10995/.

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The Global Village Playground (GVP) was a capstone learning experience designed to address institutional assessment needs while providing an integrated, contextualized, and authentic learning experience for students. In the GVP, students work on simulated and real-world problems as a design team tasked with developing an alternate reality game that makes an impact on the United Nations Millennium Development Goals. The purpose of this study was to evaluate the effectiveness of the design of the GVP as a capstone experience. The research design follows a qualitative case study approach to gathe

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9

Ratsimbazafy, Ando Lalaina. "Luminous red galaxies in simulations." Thesis, 2010. http://hdl.handle.net/11394/3483.

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>Magister Scientiae - MSc<br>There have been a number of attempts to measure the expansion rate of the Universe using age-dating of Luminous Red Galaxies (LRGs).Assuming stars in LRGs form at the same time, age-dating of two populations of LRGs at different redshifts can provide an estimate of the time difference associated with the corresponding redshift interval (dt/dz). This gives a direct estimate of the Hubble parameter at the average redshift of the two populations. In this thesis, we explore the validity of the assumptions in this method using LRGs identified in the Millenium Simulation

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10

Hilbert, Stefan [Verfasser]. "Ray-tracing through the millennium simulation / Stefan Johannes Hilbert." 2008. http://d-nb.info/989450503/34.

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11

Opolot, Daniel Christopher. "Infrared-bright galaxies in the millennium simulation and Sunyaev Zeldovich effect contamination." Thesis, 2010. http://hdl.handle.net/11394/3451.

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>Magister Scientiae - MSc<br>Measuring the evolution of the abundance of galaxy clusters puts constraints on cosmological parameters like the cosmological density parameter m, σ8 and the dark energy equation of state parameter, w. Current observations that promise to give large cluster counts and their properties are those that rely on the Sunyaev-Zeldovich effect (SZE) from clusters. We study the contamination of the SZ signals from galaxy clusters by cluster infrared (IR) galaxies and particularly faint IR galaxies. We use the Millennium simulation database to extract galaxy clusters and ded

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12

Ramamonjisoa, Fidy. "Modelling radio galaxies in the Millennium simulation: SKA/MeerKAT sources and CMB contaminants." Thesis, 2010. http://etd.uwc.ac.za/index.php?module=etd&action=viewtitle&id=gen8Srv25Nme4_2091_1367481520.

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13

Kitzbichler, Manfred Georg [Verfasser]. "Galaxy formation and evolution in the millennium simulation / vorgelegt von Manfred Georg Kitzbichler." 2007. http://d-nb.info/993536816/34.

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14

Radovan, Mauricio. "Facial Modelling and animation trends in the new millennium : a survey." Diss., 2008. http://hdl.handle.net/10500/2765.

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M.Sc (Computer Science)<br>Facial modelling and animation is considered one of the most challenging areas in the animation world. Since Parke and Waters’s (1996) comprehensive book, no major work encompassing the entire field of facial animation has been published. This thesis covers Parke and Waters’s work, while also providing a survey of the developments in the field since 1996. The thesis describes, analyses, and compares (where applicable) the existing techniques and practices used to produce the facial animation. Where applicable, the related techniques are grouped in the same chapt

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15

Almeida, Ana Carolina Silva. "Simulated discounted cash flow valuation for a financial institution: Millennium BCP." Master's thesis, 2019. http://hdl.handle.net/10071/19539.

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Valuing a bank is not an easy challenge. The only similarities with the valuation of other companies are the different approaches and models that can be used to valuate both. That variety, frequently, leads to different outcomes and/or interpretations and, thus, there is not a consensual agreement between financial analysts. This report aims to valuate a financial institution using the discounted cash flow valuation model, known to be the most appropriate and used amongst the financial and academic community. Knowing the particularities of a financial institution bank, the purpose of this rep

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