LDR | | 00000nam u2200205 4500 |
001 | | 000000432236 |
005 | | 20200224115246 |
008 | | 200131s2019 ||||||||||||||||| ||eng d |
020 | |
▼a 9781088337370 |
035 | |
▼a (MiAaPQ)AAI13903061 |
040 | |
▼a MiAaPQ
▼c MiAaPQ
▼d 247004 |
082 | 0 |
▼a 520 |
100 | 1 |
▼a Brout, Dillon. |
245 | 10 |
▼a Measuring Cosmic Acceleration and Constraining Dark Energy Models With Transients Discovered in the Dark Energy Survey. |
260 | |
▼a [S.l.]:
▼b University of Pennsylvania.,
▼c 2019. |
260 | 1 |
▼a Ann Arbor:
▼b ProQuest Dissertations & Theses,
▼c 2019. |
300 | |
▼a 182 p. |
500 | |
▼a Source: Dissertations Abstracts International, Volume: 81-04, Section: B. |
500 | |
▼a Advisor: Sako, Masao. |
502 | 1 |
▼a Thesis (Ph.D.)--University of Pennsylvania, 2019. |
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▼a This item must not be sold to any third party vendors. |
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▼a Now 20 years after the discovery of the accelerating universe, distance measurements from Type Ia supernovae over a large span in redshift remain a vital tool in constraining models for cosmic acceleration and dark energy. There has been much effort focused on generating larger and more precise datasets with good control of systematic uncertainties. The Dark Energy Survey Supernova Program (DES-SN) is the most recent such effort and has doubled the number of cosmologically viable SNe. In addition, the Dark Energy Survey Gravitational Waves program (DES-GW) identified the optical counterpart of the Binary Neutron star merger GW170817 and facilitated the first ever "standard siren" measurement of H0 |
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▼a School code: 0175. |
650 | 4 |
▼a Astrophysics. |
650 | 4 |
▼a Physics. |
650 | 4 |
▼a Astronomy. |
690 | |
▼a 0596 |
690 | |
▼a 0605 |
690 | |
▼a 0606 |
710 | 20 |
▼a University of Pennsylvania.
▼b Physics and Astronomy. |
773 | 0 |
▼t Dissertations Abstracts International
▼g 81-04B. |
773 | |
▼t Dissertation Abstract International |
790 | |
▼a 0175 |
791 | |
▼a Ph.D. |
792 | |
▼a 2019 |
793 | |
▼a English |
856 | 40 |
▼u http://www.riss.kr/pdu/ddodLink.do?id=T15492423
▼n KERIS
▼z 이 자료의 원문은 한국교육학술정보원에서 제공합니다. |
980 | |
▼a 202002
▼f 2020 |
990 | |
▼a ***1008102 |
991 | |
▼a E-BOOK |