상세정보
Export to Refworks부가기능
Studying the Cosmic Microwave Background with Spider's First Flight
상세 프로파일
| 자료유형 | 학위논문 |
|---|---|
| 서명/저자사항 | Studying the Cosmic Microwave Background with Spider's First Flight. |
| 개인저자 | Young, Edward. |
| 단체저자명 | Princeton University. Physics. |
| 발행사항 | [S.l.]: Princeton University., 2018. |
| 발행사항 | Ann Arbor: ProQuest Dissertations & Theses, 2018. |
| 형태사항 | 286 p. |
| 기본자료 저록 | Dissertation Abstracts International 79-10B(E). Dissertation Abstract International |
| ISBN | 9780438048621 |
| 학위논문주기 | Thesis (Ph.D.)--Princeton University, 2018. |
| 일반주기 |
Source: Dissertation Abstracts International, Volume: 79-10(E), Section: B.
Adviser: William C. Jones. |
| 요약 | Gravitational waves are a prediction of many early Universe models. These waves generate a divergence-free polarization component, called B -modes, of the cosmic microwave background (CMB). |
| 요약 | Spider is a balloon-borne telescope designed to study the polarized emission from the CMB. The Spider payload flew in January 2015, with detectors at 95 GHz and 150 GHz. This thesis focuses on the development and deployment of the Spider-1 paylo |
| 요약 | Our understanding of foregrounds currently limits our ability to measure B-modes from the CMB. Spider-2, with its 280 GHz channel, will be a powerful tool in constraining foregrounds. |
| 일반주제명 | Astrophysics. |
| 언어 | 영어 |
| 바로가기 | 
: 이 자료의 원문은 한국교육학술정보원에서 제공합니다. |
