| LDR | | 02624nmm uu200445 4500 |
| 001 | | 000000332416 |
| 005 | | 20240805170742 |
| 008 | | 181129s2018 |||||||||||||||||c||eng d |
| 020 | |
▼a 9780438034099 |
| 035 | |
▼a (MiAaPQ)AAI10785727 |
| 035 | |
▼a (MiAaPQ)unc:17574 |
| 040 | |
▼a MiAaPQ
▼c MiAaPQ
▼d 248032 |
| 082 | 0 |
▼a 523 |
| 100 | 1 |
▼a Ziegler, Carl Andrew. |
| 245 | 10 |
▼a Characterization of Exoplanets and Stellar Systems with New Robots. |
| 260 | |
▼a [S.l.] :
▼b The University of North Carolina at Chapel Hill.,
▼c 2018 |
| 260 | 1 |
▼a Ann Arbor :
▼b ProQuest Dissertations & Theses,
▼c 2018 |
| 300 | |
▼a 246 p. |
| 500 | |
▼a Source: Dissertation Abstracts International, Volume: 79-10(E), Section: B. |
| 500 | |
▼a Adviser: Nicholas M. Law. |
| 502 | 1 |
▼a Thesis (Ph.D.)--The University of North Carolina at Chapel Hill, 2018. |
| 520 | |
▼a Large astronomical surveys find thousands of interesting transient events, such as exoplanets. Beyond detection, these surveys are limited in their ability to study the properties of these discoveries. In particular, a common problem with wide-f |
| 520 | |
▼a I present first the design and construction of Robo-SOAR, a moderate-order NGS-AO system in development for the SOAR telescope. With robotic software adapted from Robo-AO, Robo-SOAR will be capable of observing hundreds of targets a night. With |
| 520 | |
▼a I then discuss the observations of 348 cool subdwarf stars with Robo-AO, a pilot study for future kilo-target surveys. Cool subdwarfs are remnants of the first population of stars formed in the Milky Way. I find that approximately 12% of cool su |
| 520 | |
▼a I report the results of the Robo-AO survey of every planetary candidate discovered with Kepler to search for previously unknown nearby stars. These stars contaminate the exquisite photometry of Kepler and can either dilute the transit signal fr |
| 520 | |
▼a Lastly, I use the results of the Robo-AO Kepler survey to search for evidence of the impact multiple star systems have on planets. The presence of a companion star is believed to have a significant impact on the properties of planetary systems. |
| 590 | |
▼a School code: 0153. |
| 650 | 4 |
▼a Astrophysics. |
| 650 | 4 |
▼a Astronomy. |
| 690 | |
▼a 0596 |
| 690 | |
▼a 0606 |
| 710 | 20 |
▼a The University of North Carolina at Chapel Hill.
▼b Physics. |
| 773 | 0 |
▼t Dissertation Abstracts International
▼g 79-10B(E). |
| 773 | |
▼t Dissertation Abstract International |
| 790 | |
▼a 0153 |
| 791 | |
▼a Ph.D. |
| 792 | |
▼a 2018 |
| 793 | |
▼a English |
| 856 | 40 |
▼u http://www.riss.kr/pdu/ddodLink.do?id=T14997321
▼n KERIS |
| 980 | |
▼a 201812
▼f 2019 |
| 990 | |
▼a 관리자 |