MARC보기
LDR00000nam u2200205 4500
001000000432307
00520200224120511
008200131s2019 ||||||||||||||||| ||eng d
020 ▼a 9781085799782
035 ▼a (MiAaPQ)AAI13900334
040 ▼a MiAaPQ ▼c MiAaPQ ▼d 247004
0820 ▼a 523
1001 ▼a Fuzia, Brittany.
24514 ▼a The Sunyaev-Zel'dovich Effect in Galaxy Clusters.
260 ▼a [S.l.]: ▼b The Florida State University., ▼c 2019.
260 1 ▼a Ann Arbor: ▼b ProQuest Dissertations & Theses, ▼c 2019.
300 ▼a 124 p.
500 ▼a Source: Dissertations Abstracts International, Volume: 81-04, Section: B.
500 ▼a Advisor: Huffenberger, Kevin.
5021 ▼a Thesis (Ph.D.)--The Florida State University, 2019.
506 ▼a This item must not be sold to any third party vendors.
506 ▼a This item must not be added to any third party search indexes.
520 ▼a Galaxy clusters are the largest gravitationally bound structures in the Universe, and they provide valuable insights into astrophysics and cosmology. One method of studying galaxy clusters-the Sunyaev-Zel'dovich Effect-involves using the Cosmic Microwave Background (CMB) as a backlight. As CMB photons pass through the hot electron gas of the intracluster medium, a small portion are scattered and gain energy. This causes a distortion in the spectrum of the CMB which depends mainly on the total mass of the galaxy cluster and is independent of redshift, making it an important means of probing high-redshift systems. Only recently have telescopes become sensitive enough to detect the Sunyaev-Zel'dovich effect for low masses. In this thesis, we discuss the work done using the Sunyaev-Zel'dovich effect to study low-mass galaxy clusters and to identify new galaxy clusters in CMB maps.
590 ▼a School code: 0071.
650 4 ▼a Astrophysics.
690 ▼a 0596
71020 ▼a The Florida State University. ▼b Physics.
7730 ▼t Dissertations Abstracts International ▼g 81-04B.
773 ▼t Dissertation Abstract International
790 ▼a 0071
791 ▼a Ph.D.
792 ▼a 2019
793 ▼a English
85640 ▼u http://www.riss.kr/pdu/ddodLink.do?id=T15492171 ▼n KERIS ▼z 이 자료의 원문은 한국교육학술정보원에서 제공합니다.
980 ▼a 202002 ▼f 2020
990 ▼a ***1008102
991 ▼a E-BOOK