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Probing Galaxy Evolution and the Baryon Cycle via Novel Statistical Techniques and Instrumentation
Probing Galaxy Evolution and the Baryon Cycle via Novel Statistical Techniques and Instrum...
Probing Galaxy Evolution and the Baryon Cycle via Novel Statistical Techniques and Instrumentation

Detailed Information

자료유형  
 학위논문 서양
최종처리일시  
20260202102958
ISBN  
9798286443574
DDC  
520
저자명  
Pasha, Imad.
서명/저자  
Probing Galaxy Evolution and the Baryon Cycle via Novel Statistical Techniques and Instrumentation
발행사항  
[Sl] : Yale University, 2025
발행사항  
Ann Arbor : ProQuest Dissertations & Theses, 2025
형태사항  
328 p
주기사항  
Source: Dissertations Abstracts International, Volume: 86-12, Section: B.
주기사항  
Advisor: van Dokkum, Pieter G.
학위논문주기  
Thesis (Ph.D.)--Yale University, 2025.
초록/해제  
요약Understanding the formation and evolution of galaxies across cosmic time requires both observations across redshift, wavelength, and method as well as sophisticated machinery for interpreting and carrying out inference on observations. Techniques such Bayesian Inference, Simulation Based Inference, and Machine learning are seeing increased use as attempts are made to extract meaningful results from challenging data. Meanwhile new instrumentation, from spectrographs on major telescopes (e.g., KCWI and MUSE) to new, novel designs (e.g., the Mothra Telescope Array) are providing new observational windows into heretofore invisible portions of the baryon cycle --- a fundamental cycle driving and describing how baryons move throughout the universe and into and out of galaxies. This thesis presents the development and application of statistical techniques and novel instrumentation to infer the properties of galaxies and their place within the baryon cycle.
일반주제명  
Astronomy
일반주제명  
Astrophysics
일반주제명  
Statistics
키워드  
Baryon cycle
키워드  
Bayesian inference
키워드  
Mothra Telescope Array
기타저자  
Yale University Astronomy
기본자료저록  
Dissertations Abstracts International. 86-12B.
전자적 위치 및 접속  
로그인 후 원문을 볼 수 있습니다.

MARC

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■020    ▼a9798286443574
■035    ▼a(MiAaPQ)AAI31770776
■040    ▼aMiAaPQ▼cMiAaPQ
■0820  ▼a520
■1001  ▼aPasha,  Imad.
■24510▼aProbing  Galaxy  Evolution  and  the  Baryon  Cycle  via  Novel  Statistical  Techniques  and  Instrumentation
■260    ▼a[Sl]▼bYale  University▼c2025
■260  1▼aAnn  Arbor▼bProQuest  Dissertations  &  Theses▼c2025
■300    ▼a328  p
■500    ▼aSource:  Dissertations  Abstracts  International,  Volume:  86-12,  Section:  B.
■500    ▼aAdvisor:  van  Dokkum,  Pieter  G.
■5021  ▼aThesis  (Ph.D.)--Yale  University,  2025.
■520    ▼aUnderstanding  the  formation  and  evolution  of  galaxies  across  cosmic  time  requires  both  observations  across  redshift,  wavelength,  and  method  as  well  as  sophisticated  machinery  for  interpreting  and  carrying  out  inference  on  observations.  Techniques  such  Bayesian  Inference,  Simulation  Based  Inference,  and  Machine  learning  are  seeing  increased  use  as  attempts  are  made  to  extract  meaningful  results  from  challenging  data.  Meanwhile  new  instrumentation,  from  spectrographs  on  major  telescopes  (e.g.,  KCWI  and  MUSE)  to  new,  novel  designs  (e.g.,  the  Mothra  Telescope  Array)  are  providing  new  observational  windows  into  heretofore  invisible  portions  of  the  baryon  cycle  ---  a  fundamental  cycle  driving  and  describing  how  baryons  move  throughout  the  universe  and  into  and  out  of  galaxies.  This  thesis  presents  the  development  and  application  of  statistical  techniques  and  novel  instrumentation  to  infer  the  properties  of  galaxies  and  their  place  within  the  baryon  cycle.
■590    ▼aSchool  code:  0265.
■650  4▼aAstronomy
■650  4▼aAstrophysics
■650  4▼aStatistics
■653    ▼aBaryon  cycle
■653    ▼aBayesian  inference
■653    ▼aMothra  Telescope  Array
■690    ▼a0606
■690    ▼a0596
■690    ▼a0463
■71020▼aYale  University▼bAstronomy.
■7730  ▼tDissertations  Abstracts  International▼g86-12B.
■790    ▼a0265
■791    ▼aPh.D.
■792    ▼a2025
■793    ▼aEnglish
■85640▼uhttp://www.riss.kr/pdu/ddodLink.do?id=T17356590▼nKERIS▼z이  자료의  원문은  한국교육학술정보원에서  제공합니다.

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