| LDR | | 01855nmm uu200397 4500 |
| 001 | | 000000329736 |
| 005 | | 20240805155158 |
| 008 | | 181129s2018 |||||||||||||||||c||eng d |
| 020 | |
▼a 9780438048621 |
| 035 | |
▼a (MiAaPQ)AAI10822619 |
| 035 | |
▼a (MiAaPQ)princeton:12564 |
| 040 | |
▼a MiAaPQ
▼c MiAaPQ
▼d 248032 |
| 082 | 0 |
▼a 523 |
| 100 | 1 |
▼a Young, Edward. |
| 245 | 10 |
▼a Studying the Cosmic Microwave Background with Spider's First Flight. |
| 260 | |
▼a [S.l.] :
▼b Princeton University.,
▼c 2018 |
| 260 | 1 |
▼a Ann Arbor :
▼b ProQuest Dissertations & Theses,
▼c 2018 |
| 300 | |
▼a 286 p. |
| 500 | |
▼a Source: Dissertation Abstracts International, Volume: 79-10(E), Section: B. |
| 500 | |
▼a Adviser: William C. Jones. |
| 502 | 1 |
▼a Thesis (Ph.D.)--Princeton University, 2018. |
| 520 | |
▼a 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). |
| 520 | |
▼a 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 |
| 520 | |
▼a 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. |
| 590 | |
▼a School code: 0181. |
| 650 | 4 |
▼a Astrophysics. |
| 690 | |
▼a 0596 |
| 710 | 20 |
▼a Princeton University.
▼b Physics. |
| 773 | 0 |
▼t Dissertation Abstracts International
▼g 79-10B(E). |
| 773 | |
▼t Dissertation Abstract International |
| 790 | |
▼a 0181 |
| 791 | |
▼a Ph.D. |
| 792 | |
▼a 2018 |
| 793 | |
▼a English |
| 856 | 40 |
▼u http://www.riss.kr/pdu/ddodLink.do?id=T14998490
▼n KERIS |
| 980 | |
▼a 201812
▼f 2019 |
| 990 | |
▼a 관리자 |