Zobrazeno 1 - 10 of 15 pro vyhledávání: '"Samantha Chappell"'
1
Relativistic redshift of the star S0-2 orbiting the Galactic center supermassive black hole
Autor: Yohsuke Takamori, Tuan Do, Samantha Chappell, Kelly Kosmo O'Neil, Shoko Sakai, Zhuo Chen, Aurélien Hees, Hiromi Saida, Arezu Dehghanfar, Wolfgang Kerzendorf, Siyao Jia, Devin S. Chu, Randy Campbell, Shogo Nishiyama, Rainer Schödel, Eric E. Becklin, Abhimat K. Gautam, E. Gallego-Cano, Gunther Witzel, Gregory D. Martinez, Peter Wizinowich, Keith Matthews, James E. Lyke, Andrea M. Ghez, Mark Morris, Smadar Naoz, Masaaki Takahashi, Anna Ciurlo, Jessica R. Lu
Publikováno v: Science
Science, 2019, 365 (6454), pp.664-668. ⟨10.1126/science.aav8137⟩
Science, American Association for the Advancement of Science, 2019, 365 (6454), pp.664-668. ⟨10.1126/science.aav8137⟩
Science (New York, N.Y.), vol 365, iss 6454
Digital.CSIC. Repositorio Institucional del CSIC
instname
The general theory of relativity predicts that a star passing close to a supermassive black hole should exhibit a relativistic redshift. In this study, we used observations of the Galactic Center star S0-2 to test this prediction.We combined existing
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::edb789acf2e2695afe80f69342fcf07c
https://hal.archives-ouvertes.fr/hal-02290831
Zobrazit plný text záznamu
2
Characterizing and Improving the Data Reduction Pipeline for the Keck OSIRIS Integral Field Spectrograph
Autor: Etsuko Mieda, Anna Boehle, Tuan Do, James E. Lyke, Andrea M. Ghez, Alexander R. Rudy, Shelley A. Wright, Samantha Chappell, Kelly E. Lockhart, Randy Campbell, James E. Larkin, Anna Ciurlo, Andrey Vayner, Gregory Walth, Maren Cosens, Michael P. Fitzgerald, Jessica R. Lu, Devin S. Chu
Publikováno v: Astronomical Journal, vol 157, iss 2
The Astronomical Journal, vol 157, iss 2
OSIRIS is a near-infrared (1.0--2.4 $\mu$m) integral field spectrograph operating behind the adaptive optics system at Keck Observatory, and is one of the first lenslet-based integral field spectrographs. Since its commissioning in 2005, it has been
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bda7a72c3ee59b8306bea402e08d63cc
http://arxiv.org/abs/1812.02053
Zobrazit plný text záznamu
3
Testing General Relativity with Stellar Orbits around the Supermassive Black Hole in Our Galactic Center
Autor: Mark Morris, E. E. Becklin, Smadar Naoz, Tuan Do, Anna Boehle, Shoko Sakai, G. D. Martinez, Samantha Chappell, Aurélien Hees, G. Witzel, Kelly Kosmo, Rainer Schödel, Andrea M. Ghez, Jessica R. Lu, Devin S. Chu, Arezu Dehghanfar, Keith Matthews
Publikováno v: Hees, A; Do, T; Ghez, AM; Martinez, GD; Naoz, S; Becklin, EE; et al.(2017). Testing General Relativity with Stellar Orbits around the Supermassive Black Hole in Our Galactic Center. PHYSICAL REVIEW LETTERS, 118(21). doi: 10.1103/PhysRevLett.118.211101. UCLA: Retrieved from: http://www.escholarship.org/uc/item/4b98m1n3
Physical review letters, vol 118, iss 21
In this Letter, we demonstrate that short-period stars orbiting around the supermassive black hole in our Galactic Center can successfully be used to probe the gravitational theory in a strong regime. We use 19 years of observations of the two best m
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0bf0d6deb47cb9609bca5df770155717
https://doi.org/10.1103/physrevlett.118.211101
Zobrazit plný text záznamu
4
Observational constraints on the formation and evolution of the Milky Way nuclear star cluster with Keck and Gemini
Autor: Samantha Chappell, Anja Feldmeier-Krause, Mark Morris, Wolfgang Kerzendorf, Andrea M. Ghez, Gregory D. Martinez, Jessica R. Lu, Norm Murray, Tuan Do, Nathan Winsor
Publikováno v: NASA Astrophysics Data System
Proceedings of the International Astronomical Union, vol 11, iss S322
Due to its proximity, the Milky Way nuclear star cluster provides us with a wealth of data not available in other galactic nuclei. In particular, with adaptive optics, we can observe the detailed properties of individual stars, which can offer insigh
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5478869fc6d1753eaac7f9ff39ba783a
Zobrazit plný text záznamu
6
Constraining the Variability and Binary Fraction of Galactic Center Young Stars
Autor: Samantha Chappell, Abhimat K. Gautam, Shoko Sakai, Gunther Witzel, Jessica R. Lu, Andrea M. Ghez, Breann N. Sitarski, Tuan Do, Mark Morris
Publikováno v: Proceedings of the International Astronomical Union, vol 11, iss S322
NASA Astrophysics Data System
Gautam, AK; Do, T; Ghez, AM; Lu, JR; Morris, MR; Sakai, S; et al.(2017). Constraining the Variability and Binary Fraction of Galactic Center Young Stars. UCLA: Retrieved from: http://www.escholarship.org/uc/item/179199wq
We present constraints on the variability and binarity of young stars in the central 10 arcseconds (~0.4 pc) of the Milky Way Galactic Center (GC) using Keck Adaptive Optics data over a 12 year baseline. Given our experiment's photometric uncertainti
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d9f3353e6a5d74903b950ca3378e1497
https://doi.org/10.1017/s1743921316011996
Zobrazit plný text záznamu
7
Detection of Galactic Center Source G2 at 3.8 μm during Periapse Passage
Autor: Leo Meyer, Randall D. Campbell, Tuan Do, Sylvana Yelda, Mark Morris, Breann N. Sitarski, Eric E. Becklin, Alan Stockton, Keith Matthews, Anna Boehle, Andrea M. Ghez, Samantha Chappell, Smadar Naoz, Gabriela Canalizo, Jessica R. Lu, Gunther Witzel, Peter Wizinowich
Publikováno v: Witzel, G; Ghez, AM; Morris, MR; Sitarski, BN; Boehle, A; Naoz, S; et al.(2014). Detection of Galactic Center source G2 at 3.8 μm during periapse passage. Astrophysical Journal Letters, 796(1). doi: 10.1088/2041-8205/796/1/L8. UCLA: Retrieved from: http://www.escholarship.org/uc/item/7kc2v20t
Astrophysical Journal Letters, vol 796, iss 1
The Astrophysical Journal Letters, vol 796, iss 1
We report new observations of the Galactic Center source G2 from the W. M. Keck Observatory. G2 is a dusty red object associated with gas that shows tidal interactions as it nears closest approach with the Galaxy's central black hole. Our observation
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::55813bf928e1f47558cfdaeb11ec2738
https://resolver.caltech.edu/CaltechAUTHORS:20141215-090620639
Zobrazit plný text záznamu
10
Investigating the Binarity of S0-2: Implications for its Origins and Robustness as a Probe of the Laws of Gravity around a Supermassive Black Hole
Autor: Samantha Chappell, Devin S. Chu, Gunther Witzel, Keith Matthews, Andrea M. Ghez, Tuan Do, Abhimat K. Gautam, Smadar Naoz, Shoko Sakai, Aurélien Hees, Jessica R. Lu
Publikováno v: NASA Astrophysics Data System
Astrophysical Journal, vol 854, iss 1
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2018, 854 (1), pp.12. ⟨10.3847/1538-4357/aaa3eb⟩
The Astrophysical Journal, vol 854, iss 1
The star S0-2, which orbits the supermassive black hole (SMBH) in our Galaxy with a period of 16 years, provides the strongest constraint on both the mass of the SMBH and the distance to the Galactic center. S0-2 will soon provide the first measureme
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a514d4f2300bdf14db27e2af65d4d9b3
https://ui.adsabs.harvard.edu/#abs/2018AAS...23131102C
Zobrazit plný text záznamu

Vyhledávací nástroje:

Upřesnit hledání

Omezení vyhledávání
Plný text Recenzováno Digitální knihovna AV ČR
Zdroje