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New Views of the Hot and Diffuse Gaseous Universe With the Thermal Sunyaev-Zel'dovich Effect
New Views of the Hot and Diffuse Gaseous Universe With the Thermal Sunyaev-Zel'dovich Effe...
New Views of the Hot and Diffuse Gaseous Universe With the Thermal Sunyaev-Zel'dovich Effect

상세정보

자료유형  
 학위논문 서양
최종처리일시  
20250211153013
ISBN  
9798384045359
DDC  
523
저자명  
Pratt, Cameron T.
서명/저자  
New Views of the Hot and Diffuse Gaseous Universe With the Thermal Sunyaev-Zeldovich Effect
발행사항  
[Sl] : University of Michigan, 2024
발행사항  
Ann Arbor : ProQuest Dissertations & Theses, 2024
형태사항  
150 p
주기사항  
Source: Dissertations Abstracts International, Volume: 86-04, Section: B.
주기사항  
Advisor: Bregman, Joel N.
학위논문주기  
Thesis (Ph.D.)--University of Michigan, 2024.
초록/해제  
요약Most of the baryonic matter in the Universe is expected to exist as diffuse gas surrounding galaxies, galaxy groups, and galaxy clusters. Detecting this is a difficult task, especially when it is too diffuse to see in X-ray emission. The Sunyaev-Zel'dovich (SZ) effect offers an independent view of cosmological gas by measuring spectral distortions in the cosmic microwave background (CMB). In this thesis, I present the process of extracting SZ maps (y-maps) from Planck and WMAP data. These y-maps are used to estimate the gaseous contents around individual systems, particularly galaxy groups. Moreover, part of this work includes the first resolved SZ signal measured from a stack of nearby galaxy groups. Then I describe the efforts made improve the quality of current SZ data using machine learning. Specifically, I discuss two methodologies to extract the SZ signal with deep learning. Finally, I will conclude with a statement regarding the current state of SZ data and the notable caveats of using mock data and supervised learning to make real-world predictions.
일반주제명  
Astrophysics
일반주제명  
Astronomy
일반주제명  
Computer science
일반주제명  
Computational physics
키워드  
Missing baryon problem
키워드  
Sunyaev-Zel'dovich effect
키워드  
Machine learning
키워드  
Galaxy groups
키워드  
Deep learning
기타저자  
University of Michigan Astronomy and Astrophysics
기본자료저록  
Dissertations Abstracts International. 86-04B.
전자적 위치 및 접속  
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■1001  ▼aPratt,  Cameron  T.
■24510▼aNew  Views  of  the  Hot  and  Diffuse  Gaseous  Universe  With  the  Thermal  Sunyaev-Zel'dovich  Effect
■260    ▼a[Sl]▼bUniversity  of  Michigan▼c2024
■260  1▼aAnn  Arbor▼bProQuest  Dissertations  &  Theses▼c2024
■300    ▼a150  p
■500    ▼aSource:  Dissertations  Abstracts  International,  Volume:  86-04,  Section:  B.
■500    ▼aAdvisor:  Bregman,  Joel  N.
■5021  ▼aThesis  (Ph.D.)--University  of  Michigan,  2024.
■520    ▼aMost  of  the  baryonic  matter  in  the  Universe  is  expected  to  exist  as  diffuse  gas  surrounding  galaxies,  galaxy  groups,  and  galaxy  clusters.  Detecting  this  is  a  difficult  task,  especially  when  it  is  too  diffuse  to  see  in  X-ray  emission.  The  Sunyaev-Zel'dovich  (SZ)  effect  offers  an  independent  view  of  cosmological  gas  by  measuring  spectral  distortions  in  the  cosmic  microwave  background  (CMB).  In  this  thesis,  I  present  the  process  of  extracting  SZ  maps  (y-maps)  from  Planck  and  WMAP  data.  These  y-maps  are  used  to  estimate  the  gaseous  contents  around  individual  systems,  particularly  galaxy  groups.  Moreover,  part  of  this  work  includes  the  first  resolved  SZ  signal  measured  from  a  stack  of  nearby  galaxy  groups.  Then  I  describe  the  efforts  made  improve  the  quality  of  current  SZ  data  using  machine  learning.  Specifically,  I  discuss  two  methodologies  to  extract  the  SZ  signal  with  deep  learning.  Finally,  I  will  conclude  with  a  statement  regarding  the  current  state  of  SZ  data  and  the  notable  caveats  of  using  mock  data  and  supervised  learning  to  make  real-world  predictions.
■590    ▼aSchool  code:  0127.
■650  4▼aAstrophysics
■650  4▼aAstronomy
■650  4▼aComputer  science
■650  4▼aComputational  physics
■653    ▼aMissing  baryon  problem
■653    ▼aSunyaev-Zel'dovich  effect
■653    ▼aMachine  learning
■653    ▼aGalaxy  groups
■653    ▼aDeep  learning
■690    ▼a0596
■690    ▼a0606
■690    ▼a0984
■690    ▼a0800
■690    ▼a0216
■71020▼aUniversity  of  Michigan▼bAstronomy  and  Astrophysics.
■7730  ▼tDissertations  Abstracts  International▼g86-04B.
■790    ▼a0127
■791    ▼aPh.D.
■792    ▼a2024
■793    ▼aEnglish
■85640▼uhttp://www.riss.kr/pdu/ddodLink.do?id=T17164531▼nKERIS▼z이  자료의  원문은  한국교육학술정보원에서  제공합니다.

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