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Dissertations / Theses on the topic 'Sunyani'

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Published: 4 June 2025
Last updated: 1 August 2025

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1

Pius, A., and E. V. Shkarupa. "Environmental sanitation policy and solid waste management in Sunyani municipality." Thesis, Сумський державний університет, 2013. http://essuir.sumdu.edu.ua/handle/123456789/31698.

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Solid Waste management is one of the least recognized public policy issues in Ghana. Quite apart from the obvious physical unattractiveness of the business, waste management often competes with more pressing economic and social issues such as fiscal and trade matters, unemployment and poverty, education and health. Even within the domain of environmental sustainability, the management of waste has had to play second fiddle to more apparently manifest challenges such as land and coastal degradation, biodiversity loss, and climate change. Waste management, however, remains a major challenge for
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2

Kusi, Hinneh. "Managing junior secondary schools in Sunyani Municipality (Ghana) : the challenges for headteachers and their professional development needs." Thesis, University of Leicester, 2008. http://hdl.handle.net/2381/4099.

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The study investigated the challenges for Junior Secondary School headteachers (both male and female) in the Sunyani municipality of Ghana and their professional development needs. Ghana is a developing country in West Africa facing the challenge of improving educational provision at different levels. This was a qualitative study underpinned by interpretive philosophical thought. It employed a case study approach and collected data in two phases using semi-structured questionnaire and semi-structured interview. In the first phase, a questionnaire was distributed to all headteachers and Circuit
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3

Grainger, William Frank. "Using the Sunyaev-Zel'dovich effect." Thesis, University of Cambridge, 2001. https://www.repository.cam.ac.uk/handle/1810/251795.

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This work is concerned with the Sunyaev-Zel'dovich (S-Z) effect in clusters of galaxies and its use in cosmology. In Chapter 2, I consider possible causes of error in the determination of <I>H</I><SUB>0</SUB> from the uncertain geometry of clusters and complications such as lack of virialisation. From numerical simulations, I find that with 20 clusters, the resultant error is 8%. Chapter 3 details and tests a new maximum likelihood algorithm for the removal of contaminating radio sources. Two new estimates of <I>H</I><SUB>0</SUB> are presented, 78<SUP>+26</SUP><SUB>-20</SUB> dm s<SUP>-1</SUP>
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4

Hennig, Christina. "The galaxy population evolution of Sunyaev." Diss., Ludwig-Maximilians-Universität München, 2015. http://nbn-resolving.de/urn:nbn:de:bvb:19-184237.

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This thesis presents a study of the galaxy populations in massive galaxy clusters that have been selected via the Sunyaev - Zeldovich Effect from the South Pole Telescope. The clusters have multiband optical imaging data from the Dark Energy Survey (DES). Each cluster has a robust mass estimate and with the deep DES data they cover a redshift range between 0 and 1.1. This makes it an ideal cluster sample to study evolutionary trends of the galaxy populations with mass and redshift.
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5

Portsmouth, Jamie 1974. "Polarization in the Sunyaev-Zeldovich effect." Thesis, Massachusetts Institute of Technology, 2003. http://hdl.handle.net/1721.1/17016.

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Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2003.<br>Includes bibliographical references (p. 121-125).<br>This electronic version was submitted by the student author. The certified thesis is available in the Institute Archives and Special Collections.<br>A novel covariant formalism for the treatment of the transfer and Compton scattering of partially polarized light is presented. In this approach, the polarization state of a light beam is described by a tensor constructed from the time average of quadratic products of the electric field components in a local obse
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6

Geisbüsch, Jörn. "Cosmology with Sunyaev-Zelʼdovich cluster surveys". Thesis, University of Cambridge, 2007. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.613080.

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7

Jones, Michael Edward. "Aperture synthesis observations of the Sunyaev-Zel'dovich effect." Thesis, University of Cambridge, 1990. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.357766.

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8

Chen, Nan-chieh. "Menschsein als Dialog und Shūnyatā : eine transkulturelle Studie zur Schwerstbehindertenpädagogik /." Berlin ; Münster : Lit, 2007. http://deposit.d-nb.de/cgi-bin/dokserv?id=2956113&prov=M&dokv̲ar=1&doke̲xt=htm.

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9

Grainge, Keith. "Measuring the Hubble constant via the Sunyaev-Zel'dovich effect." Thesis, University of Cambridge, 1996. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.264501.

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10

Schammel, Michel Philippe. "Blind Sunyaev-Zel'dovich survey with the Arcminute Microkelvin Imager." Thesis, University of Cambridge, 2013. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.648243.

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11

Holanda, Rodrigo Fernandes Lira de. "O efeito Sunyaev-Zel\'dovich: teoria e aplicações cosmológicas." Universidade de São Paulo, 2011. http://www.teses.usp.br/teses/disponiveis/14/14131/tde-13092011-135337/.

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O efeito Sunyaev-Zel\'dovich (ESZ) é uma das mais promissoras técnicas de investigação cosmológica envolvendo os aglomerados de galáxias e a radiação cósmica de fundo (RCF). Tal efeito é uma modificação no espectro planckiano da RCF devido à interação dos fótons com os elétrons energéticos que permeiam o meio intra-aglomerado. Nesta tese de doutorado, vinculamos alguns parâmetros cosmológicos e investigamos a estrutura dos aglomerados de galáxias. Para tal, consideramos amostras de aglomerados para os quais existem medidas conjuntas do ESZ e do brilho em Raios-X. Duas amostras são consi
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12

Taburet, Nicolas. "L'effet Sunyaev-Zel'dovich dans l'analyse du fond diffus cosmologique." Paris 11, 2010. http://www.theses.fr/2010PA112322.

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Une nouvelle génération de relevés mesure actuellement les anisotropies du fond diffus cosmologique (FDC) aux petites échelles angulaires et va permettre de tester plus avant le modèle standard de la cosmologie. A ces petites échelles les anisotropies primaires sont dominées par celles, secondaires, dues à l'effet Sunyaev-Zel'dovich (SZ) des amas de galaxies. La signature spectrale caractéristique de l'effet SZ permet de construire des catalogues d'amas et d'en soustraire la contribution au FDC primaire. Cependant les résidus SZ des amas non résolus sont susceptibles de biaiser l'estimation de
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13

Edgington, Samantha Faye Lange Andrew E. "A galaxy cluster survey using the Sunyaev Zel'dovich effect /." Diss., Pasadena, Calif. : California Institute of Technology, 2004. http://resolver.caltech.edu/CaltechETD:etd-09272003-154928.

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14

Di, Mascolo Luca [Verfasser], and Rashid [Akademischer Betreuer] Sunyaev. "Probing the intracluster medium at high angular resolution via radio-interferometric measurements of the Sunyaev-Zeldovich effect / Luca Di Mascolo ; Betreuer: Rashid Sunyaev." München : Universitätsbibliothek der Ludwig-Maximilians-Universität, 2020. http://d-nb.info/1214593356/34.

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15

Staniszewski, Zachary K. "First Galaxy Clusters Discovered Via the Sunyaev Zel-D'ovich Effect /." Cleveland, Ohio : Case Western Reserve University, 2010. http://rave.ohiolink.edu/etdc/view?acc_num=case1271698482.

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Thesis (Doctor of Philosophy)--Case Western Reserve University, 2010<br>Department of Physics Title from PDF (viewed on 2010-05-25) Includes abstract Includes bibliographical references and appendices Available online via the OhioLINK ETD Center
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16

Lyskova, Natalya [Verfasser], and Rashid [Akademischer Betreuer] Sunyaev. "Mass determination of elliptical galaxies / Natalya Lyskova. Betreuer: Rashid Sunyaev." München : Universitätsbibliothek der Ludwig-Maximilians-Universität, 2014. http://d-nb.info/1050648129/34.

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17

Kennedy, James 1983. "The APEX-SZ experiment : observations of the Sunyaev Zel'dovich effect." Thesis, McGill University, 2008. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=116109.

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The Sunyaev Zel'dovich effect (SZE) is a secondary distortion of the cosmic microwave background (CMB) spectrum produced by galaxy clusters that allows for measurements of intra-cluster gas properties. Current experiments are using large arrays of multiplexed transition-edge sensor bolometers to achieve the sensitivities required for SZE cluster surveys and targeted cluster SZE observations. This thesis describes the APEX-SZ experiment, the first instrument to produce scientific results from observations with such an array. The scientific motivation for the APEX-SZ experiment is discussed, fol
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18

Cunha, da Silva António José. "The Sunyaev-Zel'dovich effect : predictions from hydrodynamical N-body simulations." Thesis, University of Sussex, 2002. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.247972.

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19

Runyan, Marcus Christian Lange Andrew E. "A search for galaxy clusters using the Sunyaev-Zel'dovich effect /." Diss., Pasadena, Calif. : California Institute of Technology, 2003. http://resolver.caltech.edu/CaltechETD:etd-05292003-125239.

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20

Shimwell, Timothy William. "Blind and pointed Sunyaev-Zel'dovich observations with the Arcminute Microkelvin Imager." Thesis, University of Cambridge, 2011. https://www.repository.cam.ac.uk/handle/1810/241039.

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In this thesis I discuss my work on the Arcminute Microkelvin Imager (AMI). I focus on the detection of Sunyaev-Zel'dovich (SZ) signatures at 14-18GHz. Once the background science and operation of the instrument are described I proceed to present my contribution to the calibration of AMI, including: primary beam measurements; refinements to the known antenna geometry and flagging geostationary satellite interference. This is followed by an outline of the software that I have developed to subtract sources from visibilities, concatenate data from multiple observations, simulate data, and perform
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21

Zenteno, Alfredo. "Galaxy populations in galaxy clusters selected by the Sunyaev-Zeldovich Effect." Diss., Ludwig-Maximilians-Universität München, 2014. http://nbn-resolving.de/urn:nbn:de:bvb:19-170507.

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We present a study of the galaxy populations in massive galaxy clusters selected by their Sunyaev–Zel’dovich Effect (SZE) signatures. Selection via the SZE is approximately mass- limited where the mass limit varies only slightly with redshift, making it an ideal selection method for studying the evolution of the galaxy content of clusters. We begin by introducing the SZE, the South Pole Telescope (SPT), and the larger research project in which this Thesis is embedded. We then present the core galaxy population studies of this Thesis. In Chapter 3, we present the first large-scale follow-up of
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22

Horner, Piers Francis. "1.1mm Bolocam observations of the Sunyaev Zel'dovich increment in Abell 1835." Thesis, Cardiff University, 2010. http://orca.cf.ac.uk/55186/.

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Over recent years, there has been an increasing level of interest in the cosmological significance of observations of the Sunyaev Zel'dovich (SZ) effect in galaxy clusters. Al though the SZ effect has been known about for around fifty years, observations of it have only become mainstream recently. The SZ effect refers to the redistribution of energy of Cosmic Microwave Background (CMB) photons due to inverse Compton scattering off populations of free electrons, most commonly in galaxy clusters. The SZ acts as an artificial 'emitter' or 'absorber' along the line of sight to a cluster once other
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23

Mecoli, Davide. "Processi di scattering e applicazioni astrofisiche." Bachelor's thesis, Alma Mater Studiorum - Università di Bologna, 2017. http://amslaurea.unibo.it/14771/.

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L'elaborato contiene la descrizione fisica dei processi di scattering Thomson, Compton e Compton inverso. Sono trattati i fenomeni di Comptonizzazione, Synchrotron Self Compton, Catastrofe Compton ed Effetto Sunyaev-Zeldovich nel panorama astrofisico. Nell'elaborato sono inclusi due articoli scientifici pubblicati in "The Astronomical Journal", in particolare l'effetto Sunyaev-Zeldovich impiegato per la determinazione della Costante di Hubble.
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24

Hancock, Stephen. "Detections of structure in the cosmic microwave background." Thesis, University of Cambridge, 1994. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.338307.

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25

Soraisam, Monika Devi [Verfasser], and Rashid [Akademischer Betreuer] Sunyaev. "Novae : a theoretical and observational study / Monika Devi Soraisam. Betreuer: Rashid Sunyaev." München : Universitätsbibliothek der Ludwig-Maximilians-Universität, 2016. http://d-nb.info/1102897213/34.

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26

Mineo, Stefano [Verfasser], and Rashid [Akademischer Betreuer] Sunyaev. "X-ray emission from star-forming galaxies / Stefano Mineo. Betreuer: Rashid Sunyaev." München : Universitätsbibliothek der Ludwig-Maximilians-Universität, 2011. http://d-nb.info/1015500900/34.

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27

Chen, Hailiang [Verfasser], and Rashid [Akademischer Betreuer] Sunyaev. "Modelling accreting white dwarf populations in galaxies / Hailiang Chen. Betreuer: Rashid Sunyaev." München : Universitätsbibliothek der Ludwig-Maximilians-Universität, 2016. http://d-nb.info/1113534583/34.

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28

Allison, J. R. "Observations of the Sunyaev-Zel'dovich effect using the Cosmic Background Imager 2." Thesis, University of Oxford, 2010. http://ora.ox.ac.uk/objects/uuid:c6b10ecf-3b50-4c2a-9ee1-0fe8dd93e580.

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This thesis describes the analysis of pointed thermal Sunyaev-Zel'dovich (SZ) effect data from observations using the Cosmic Background Imager 2 (CBI2). CBI2 is an upgrade to the original Cosmic Background Imager, with antennas that have twice the effective collecting area, and hence provide greater sensitivity on longer baselines. Observations of the thermal SZ effect constrain the line-of-sight integrated gas pressure within clusters of galaxies and, when combined with X-ray data, provide an excellent tool for deriving the physical properties of these large structures. The CBI2 SZ data combi
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29

Puisieux, Sarah. "Etude des effets Sunyaev-Zel'dovitch cinétique et relativiste dans les données Planck." Phd thesis, Université Paris-Diderot - Paris VII, 2013. http://tel.archives-ouvertes.fr/tel-01019928.

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Les effets Sunyaev-Zel'dovitch (SZ) correspondent à la diffusion inverse-Compton des photons du fond diffus cosmologique sur le gaz des amas de galaxies. Ce travail a visé à étudier l'ensemble des aspects des effets SZ cinétique et relativiste dans les données Planck. Pour ce faire, nous avons développé des filtres adaptés, conçus spécialement pour la détection des effets SZ. Ces filtres nous ont permis d'utiliser l'ensemble des longueurs d'onde de l'expérience de façon optimale. L'effet SZ cinétique est proportionnel à la vitesse radiale particulière des amas de galaxies. Nous avons donc pu é
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30

Hurier, Guillaume. "Etude des amas de galaxies avec l'expérience PLANCK, via l'effet Sunyaev-Zel'dovich." Phd thesis, Université de Grenoble, 2012. http://tel.archives-ouvertes.fr/tel-00849126.

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Cette thèse se focalise sur l'étude des amas de galaxies, via l'effet Sunyaev-Zel'dovich (tSZ), qui consiste en l'interaction de ces même amas avec le fond diffus cosmologique. Pour ce faire j'ai utilisé les données expérimentale de l'instrument HFI du satellite PLANCK. Cette thèse ce découpe en trois parties majeures, (1) L'analyse et le traitement des données en temps, des données brut jusqu'au cartes du ciel, ce focalisant tout particulièrement sur les effets systématiques. (2) Le développement de méthode de séparation de sources, permettant la construction de cartes par émission astrophysi
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31

Trevisan, Marina. "Estudo da possibilidade de observação do efeito sunyaev-zel'Dovich nos mapas WMAP." Instituto Nacional de Pesquisas Espaciais, 2007. http://urlib.net/sid.inpe.br/mtc-m17@80/2007/07.02.16.42.

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Observações do efeito Sunyaev-Zeldovich (SZ) são de grande interesse em estudos de cosmologia e para o mapeamento das grandes estruturas do universo. Este efeito corresponde a uma pequena distorção no espectro da Radiação Cósmica de Fundo (RCF) causado por espalhamento Compton inverso dos fótons da RCF por elétrons presentes no gás em aglomerados de galáxias e é independente do redshift do aglomerado. Neste trabalho são apresentados a metodologia desenvolvida e os resultados da observação do efeito SZ nos mapas das bandas Q (41 GHz), V (61 GHz) eW(94 GHz) do satélite Wilkinson Microwave Anisot
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32

Adam, R., I. Bartalucci, G. W. Pratt, et al. "Mapping the kinetic Sunyaev-Zel’dovich effect toward MACS J0717.5+3745 with NIKA." EDP SCIENCES S A, 2017. http://hdl.handle.net/10150/623249.

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Measurement of the gas velocity distribution in galaxy clusters provides insight into the physics of mergers, through which large scale structures form in the Universe. Velocity estimates within the intracluster medium (ICM) can be obtained via the Sunyaev-Zel'dovich (SZ) effect, but its observation is challenging both in term of sensitivity requirement and control of systematic effects, including the removal of contaminants. In this paper we report resolved observations, at 150 and 260 GHz, of the SZ effect toward the triple merger MACS J0717.5 + 3745 (z = 0.55), using data obtained with the
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33

Ip, Lai-Kwan Regin. "Vision of sunyata-wu (void) : towards a processual perspective of social work /." [St. Lucia, Qld.], 2001. http://www.library.uq.edu.au/pdfserve.php?image=thesisabs/absthe16155.pdf.

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34

Puisieux, Sarah. "Etude de l'effet Sunyaev-Zel'dovich cinétique et relativiste dans les données Planck." Paris 7, 2013. http://www.theses.fr/2013PA077232.

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Les effets Sunyaev-Zel'dovitch (SZ) correspondent à la diffusion inverse-Compton des photons du fond diffus cosmologique sur le gaz des amas de galaxies. Ce travail a visé à étudier l'ensemble des aspects des effets SZ cinétique et relativiste dans les données Planck. Pour ce faire, nous avons développé des filtres adaptés, conçus spécialement pour la détection des effets SZ. Ces filtres nous ont permis d'utiliser l'ensemble des longueurs d'onde de l'expérience de façon optimale. L'effet SZ cinétique est proportionnel à la vitesse radiale particulière des amas de galaxies. Nous avons donc pu é
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35

Contreras, Radovic Cristian. "La teoria del big bang y la doctrina de Nagarjuna: el vacío o sunyata como síntesis ontológica de todo cuanto existe." Doctoral thesis, Universitat Autònoma de Barcelona, 2004. http://hdl.handle.net/10803/5162.

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Mi tesis doctoral investiga la Teoría del Big Bang sobre el origen del universo y su relación con la doctrina del sabio filósofo budista, Nagarjuna (India s.II-III), fundador de la Vía Media o Camino Medio del budismo, según su obra genuina titulada Mûla-mâdhyamaka-kârik_, un texto decididamente auténtico, opus magna de este autor conforme la tradición india, china y tibetana, prueba indiscutible de la historicidad de su figura. Nagarjuna, uno de los cuatro soles que iluminan al mundo desde sus cuatro direcciones, maestro espiritual de Oriente y Occidente, fue el creador de la escuela budista
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36

Enriquez, Karen Bautista. "Interrupting the conversation on kenosis and sunyata: Buddhist and Christian women in search of the relational self." Thesis, Boston College, 2011. http://hdl.handle.net/2345/bc-ir:104404.

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Thesis advisor: John Makransky<br>The purpose of this dissertation is to contribute to Christian theological anthropology by bringing in the "interruption" of another religious tradition, Buddhism, in order to see how key Buddhist doctrines such as emptiness and practices of meditation may inform aspects of the Christian feminist discussions of kenosis in the spiritual life, and the search for a relational self. It also seeks to enhance Buddhist-Christian dialogue by bringing the "interruption" of feminist voices from both the Buddhist and Christian traditions into conversation with each other
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Tanimura, Hideki. "Probing the large-scale structure of the Universe with the Sunyaev-Zel'dovich Effect." Thesis, University of British Columbia, 2017. http://hdl.handle.net/2429/63189.

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The Sunyaev-Zeldovich (SZ) effect is a spectral distortion in the Cosmic Microwave Background (CMB), due to up-scattering of CMB photons by high energy electrons in clusters of galaxies or any cosmic structure. The Planck satellite mission has measured the spectral distortion with great sensitivity and has produced a full-sky SZ (y) map, which can be used to trace the large-scale structure of the Universe. In this dissertation, I construct the average SZ (y) profile of ∼ 65,000 Luminous Red Galaxies (LRGs) from the Sloan Digital Sky Survey Data Release 7 (SDSS/DR7) using the Planck y map and
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Komarov, Sergey [Verfasser], and Rashid [Akademischer Betreuer] Sunyaev. "Thermal conduction in hot gas of galaxy clusters / Sergey Komarov ; Betreuer: Rashid Sunyaev." München : Universitätsbibliothek der Ludwig-Maximilians-Universität, 2016. http://d-nb.info/1114068209/34.

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39

Chase, Simon Timothy. "A millimetre-wavelength search for the Sunyaev-Zeldovich effect in clusters of galaxies." Thesis, Imperial College London, 1985. http://hdl.handle.net/10044/1/37656.

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40

Soergel, B., S. Flender, K. T. Story, et al. "Detection of the kinematic Sunyaev–Zel'dovich effect with DES Year 1 and SPT." OXFORD UNIV PRESS, 2016. http://hdl.handle.net/10150/621727.

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We detect the kinematic Sunyaev-Zel'dovich (kSZ) effect with a statistical significance of 4.2 sigma by combining a cluster catalogue derived from the first year data of the Dark Energy Survey with cosmic microwave background temperature maps from the South Pole Telescope Sunyaev-Zel'dovich Survey. This measurement is performed with a differential statistic that isolates the pairwise kSZ signal, providing the first detection of the large-scale, pairwise motion of clusters using redshifts derived from photometric data. By fitting the pairwise kSZ signal to a theoretical template, we measure the
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41

Herbig, Thomas Readhead Anthony C. S. "A measurement of the Sunyaev-Zeldovich effect in the coma cluster of galaxies /." Diss., Pasadena, Calif. : California Institute of Technology, 1994. http://resolver.caltech.edu/CaltechETD:etd-09102008-151722.

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42

Soergel, Bjoern. "The kinematic and thermal Sunyaev-Zel'dovich effects as probes of cosmology and astrophysics." Thesis, University of Cambridge, 2018. https://www.repository.cam.ac.uk/handle/1810/277657.

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A small fraction of cosmic microwave background (CMB) photons scatter off electrons in the ionised gas in collapsed structures. This process, known as the Sunyaev-Zel'dovich effect, is usually broken down into a thermal (tSZ) and a kinematic (kSZ) contribution. While the former is sensitive to the random velocities of the electrons in the hot gas, the latter is sourced by the bulk motion of the entire object. In this thesis I measure the signature of both of these effects by cross-correlating CMB data with different tracers of the large-scale structure. I further study how these effects can be
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43

Ruppin, Florian. "Cosmologie via les observations d'amas de galaxies par effet Sunyaev-Zel'dovich avec NIKA2." Thesis, Université Grenoble Alpes (ComUE), 2018. http://www.theses.fr/2018GREAY029/document.

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La distribution de masse dans l'Univers telle que tracée par les amas de galaxies constitue une sonde cosmologique puissante. La caractérisation des processus associés à l'origine et à la croissance des grandes structures permet de contraindre des paramètres cosmologiques via l'étude de la distribution des amas en fonction de leur masse et de leur redshift. Cependant, il existe un désaccord statistiquement significatif observé entre les contraintes cosmologiques établies par l'étude des anisotropies primaires du fond diffus cosmologique et celles issues de l'analyse de la distribution des amas
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SILVA, NETO Gival Pordeus da. "Testando a robustez na determinação da constante de hubble, H0, via observáveis em redshifts intermediários." Universidade Federal de Campina Grande, 2015. http://dspace.sti.ufcg.edu.br:8080/jspui/handle/riufcg/1988.

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Submitted by Emanuel Varela Cardoso (emanuel.varela@ufcg.edu.br) on 2018-10-16T19:37:30Z No. of bitstreams: 1 GIVAL PORDEUS DA SILVA NETO – DISSERTAÇÃO (PPGFísica) 2015.pdf: 4886479 bytes, checksum: 8589cc7f91d5dab59210f3bf9b9a3d97 (MD5)<br>Made available in DSpace on 2018-10-16T19:37:30Z (GMT). No. of bitstreams: 1 GIVAL PORDEUS DA SILVA NETO – DISSERTAÇÃO (PPGFísica) 2015.pdf: 4886479 bytes, checksum: 8589cc7f91d5dab59210f3bf9b9a3d97 (MD5) Previous issue date: 2015-05-08<br>Capes<br>A constante de Hubble (H0) é considerada fundamental na cosmologia. Ela é crucial para qualquer modelo cosm
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Tenzin, Kencho. "Shankara a Hindu revivalist or a crypto-Buddhist? /." unrestricted, 2006. http://etd.gsu.edu/theses/available/etd-11302006-094652/.

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Thesis (M.A.)--Georgia State University, 2006.<br>Kathryn McClymond, committee chair; Jonathan Herman, Christopher White, committee members. Electronic text (70 p.) : digital, PDF file. Description based on contents viewed Apr. 20, 2007; title from title screen. Includes bibliographical references (p. 60-61).
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Hennig, Christina [Verfasser], and Joseph [Akademischer Betreuer] Mohr. "The galaxy population evolution of Sunyaev-Zeldovich selected clusters / Christina Hennig. Betreuer: Joseph Mohr." München : Universitätsbibliothek der Ludwig-Maximilians-Universität, 2015. http://d-nb.info/1074358716/34.

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Koliopanos, Filippos [Verfasser], and Rashid [Akademischer Betreuer] Sunyaev. "X-ray diagnostics of ultra-compact X-ray binaries / Filippos Koliopanos. Betreuer: Rashid Sunyaev." München : Universitätsbibliothek der Ludwig-Maximilians-Universität, 2015. http://d-nb.info/1073825965/34.

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Valkonen, Laura Elina. "The Sunyaev-Zel'dovich effect in galaxy clusters as a tool for estimating cosmological parameters." Thesis, University of Sussex, 2007. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.487558.

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Clusters of galaxies provide us with a sensitive probe with which to study the Universe. Their mass function is strongly dependent on the cosmological parameters, which govern the dynamical evolution of the Universe and they also provide a representative sample of ~he Universal matter distribution. The Sunyaev-Zel'dovich effect (SZE) is a promising method for detecting clusters out to their form.ation redshift and has also been shown to be a good estimator for cluster masses, A combination. of X-ray and SZE data can also be used to measure the dista:nce to the cluster, independently of the cos
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Nagarajan, Aarti [Verfasser]. "Mass calibration of the Sunyaev-Zel'dovich effect using APEX-SZ galaxy clusters / Aarti Nagarajan." Bonn : Universitäts- und Landesbibliothek Bonn, 2018. http://d-nb.info/1177881705/34.

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Novaes, Camila Paiva. "Identificação de aglomerados de galáxias em mapas da RCFM utilizando o efeito Sunyaev Zel'dovich." Instituto Nacional de Pesquisas Espaciais, 2011. http://urlib.net/sid.inpe.br/mtc-m19/2011/02.09.13.23.

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A Radiação Cósmica de Fundo em Microondas (RCFM) é considerada um dos mais importantes observáveis astrofísicos. O entendimento das propriedades (espectro, distribuição angular e polarização) que caracterizam esse campo de radiação são de extrema importância para o estudo da formação das estruturas que hoje observamos no Universo. Existem também processos secundários de produção de flutuações de temperatura, gerados após a recombinação, que podem mascarar o sinal primário da RCFM, atrapalhando o estudo de suas propriedades intrínsecas. Um desses processos é o chamado efeito Sunyaev-Zel'dovich
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