| LDR | | 01808nmm uu200385 4500 |
| 001 | | 000000333915 |
| 005 | | 20240805174758 |
| 008 | | 181129s2018 |||||||||||||||||c||eng d |
| 020 | |
▼a 9780438122413 |
| 035 | |
▼a (MiAaPQ)AAI10743957 |
| 035 | |
▼a (MiAaPQ)ucsd:17146 |
| 040 | |
▼a MiAaPQ
▼c MiAaPQ
▼d 248032 |
| 082 | 0 |
▼a 530 |
| 100 | 1 |
▼a Siritanasak, Praween. |
| 245 | 10 |
▼a Precise Measurement of B-mode polarization signal from the cosmic microwave background with the Polarbear and the Simons Array. |
| 260 | |
▼a [S.l.] :
▼b University of California, San Diego.,
▼c 2018 |
| 260 | 1 |
▼a Ann Arbor :
▼b ProQuest Dissertations & Theses,
▼c 2018 |
| 300 | |
▼a 172 p. |
| 500 | |
▼a Source: Dissertation Abstracts International, Volume: 79-11(E), Section: B. |
| 500 | |
▼a Adviser: Brian Keating. |
| 502 | 1 |
▼a Thesis (Ph.D.)--University of California, San Diego, 2018. |
| 520 | |
▼a Throughout history, human beings have always sought to answer the question ''what was the origin of the universe?'' The Cosmic Microwave Background (CMB) is one of the most essential scientific tools that will help us better understand the unive |
| 520 | |
▼a This dissertation describes the details of the Polarbear instrument which is designed to detect CMB B-mode polarization. The results from the first and second observational season are also described. Furthermore, this dissertation discusses the |
| 590 | |
▼a School code: 0033. |
| 650 | 4 |
▼a Physics. |
| 690 | |
▼a 0605 |
| 710 | 20 |
▼a University of California, San Diego.
▼b Physics. |
| 773 | 0 |
▼t Dissertation Abstracts International
▼g 79-11B(E). |
| 773 | |
▼t Dissertation Abstract International |
| 790 | |
▼a 0033 |
| 791 | |
▼a Ph.D. |
| 792 | |
▼a 2018 |
| 793 | |
▼a English |
| 856 | 40 |
▼u http://www.riss.kr/pdu/ddodLink.do?id=T14996823
▼n KERIS |
| 980 | |
▼a 201812
▼f 2019 |
| 990 | |
▼a 관리자 |