Zobrazeno 1 - 10
of 33
pro vyhledávání: '"Travis A. Berger"'
Autor:
Kendall Sullivan, Adam L. Kraus, Travis A. Berger, Trent J. Dupuy, Elise Evans, Eric Gaidos, Daniel Huber, Michael J. Ireland, Andrew W. Mann, Erik A. Petigura, Pa Chia Thao, Mackenna L. Wood, Jingwen Zhang
Publikováno v:
The Astronomical Journal, Vol 168, Iss 3, p 129 (2024)
Small planets ( R _p ≤ 4 R _⊕ ) are divided into rocky super-Earths and gaseous sub-Neptunes separated by a radius gap, but the mechanisms that produce these distinct planet populations remain unclear. Binary stars are the only main-sequence syst
Externí odkaz:
https://doaj.org/article/e0680466b4e24d9ab44940ef08d49701
Autor:
Thomas G. Williams, Janice C. Lee, Kirsten L. Larson, Adam K. Leroy, Karin Sandstrom, Eva Schinnerer, David A. Thilker, Francesco Belfiore, Oleg V. Egorov, Erik Rosolowsky, Jessica Sutter, Joseph DePasquale, Alyssa Pagan, Travis A. Berger, Gagandeep S. Anand, Ashley T. Barnes, Frank Bigiel, Médéric Boquien, Yixian Cao, Jérémy Chastenet, Mélanie Chevance, Ryan Chown, Daniel A. Dale, Sinan Deger, Cosima Eibensteiner, Eric Emsellem, Christopher M. Faesi, Simon C. O. Glover, Kathryn Grasha, Stephen Hannon, Hamid Hassani, Jonathan D. Henshaw, María J. Jiménez-Donaire, Jaeyeon Kim, Ralf S. Klessen, Eric W. Koch, Jing Li, Daizhong Liu, Sharon E. Meidt, J. Eduardo Méndez-Delgado, Eric J. Murphy, Justus Neumann, Lukas Neumann, Nadine Neumayer, Elias K. Oakes, Debosmita Pathak, Jérôme Pety, Francesca Pinna, Miguel Querejeta, Lise Ramambason, Andrea Romanelli, Mattia C. Sormani, Sophia K. Stuber, Jiayi Sun, Yu-Hsuan Teng, Antonio Usero, Elizabeth J. Watkins, Tony D. Weinbeck
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 273, Iss 1, p 13 (2024)
The exquisite angular resolution and sensitivity of JWST are opening a new window for our understanding of the Universe. In nearby galaxies, JWST observations are revolutionizing our understanding of the first phases of star formation and the dusty i
Externí odkaz:
https://doaj.org/article/24cf930b4edb45d99c558fd7403de00f
Autor:
Kendall Sullivan, Adam L. Kraus, Daniel Huber, Erik A. Petigura, Elise Evans, Trent Dupuy, Jingwen Zhang, Travis A. Berger, Eric Gaidos, Andrew W. Mann
Publikováno v:
The Astronomical Journal, Vol 165, Iss 4, p 177 (2023)
Binary stars are ubiquitous; the majority of solar-type stars exist in binaries. Exoplanet occurrence rate is suppressed in binaries, but some multiples do still host planets. Binaries cause observational biases in planet parameters, with undetected
Externí odkaz:
https://doaj.org/article/748f71f72ee648c5b8f78242a52b98f5
Autor:
Ellis A. Avallone, Jamie N. Tayar, Jennifer L. van Saders, Travis A. Berger, Zachary R. Claytor, Rachael L. Beaton, Johanna Teske, Diego Godoy-Rivera, Kaike Pan
Stellar rotation is a complex function of mass, metallicity, and age and can be altered by binarity. To understand the importance of these parameters in main sequence stars, we have assembled a sample of observations that spans a range of these param
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::40f5894556bd8de728aafea813775239
http://arxiv.org/abs/2203.15116
http://arxiv.org/abs/2203.15116
Autor:
Tomoyuki Kudo, Masato Ishizuka, Eric Gaidos, Travis A. Berger, A. Ueda, Takuma Serizawa, Shane Jacobson, Masayuki Kuzuhara, Andrew Vanderburg, Klaus W. Hodapp, Andrew W. Mann, Jun Nishikawa, Hiroki Harakawa, D A Owens, Takashi Kurokawa, M. Konishi, Teriyuki Hirano, Takayuki Kotani, M. Omiya, Motohide Tamura
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 495:650-662
We obtained high-resolution infrared spectroscopy and short-cadence photometry of the 600-800 Myr Praesepe star K2-100 during transits of its 1.67-day planet. This Neptune-size object, discovered by the NASA K2 mission, is an interloper in the "deser
Autor:
M. L. Winther, Zeynep Çelik Orhan, Jennifer L. van Saders, Richard H. D. Townsend, Daniel Huber, Maïssa Salama, Sibel Örtel, Victor Silva Aguirre, R. Paul Butler, Savita Mathur, Travis A. Berger, Keivan G. Stassun, Aldo Serenelli, Hans Kjeldsen, Ashley Chontos, Timothy R. Bedding, Jia Mian Joel Ong, Mia S. Lundkvist, Zachary R. Claytor, Steve B. Howell, Robert A. Wittenmyer, Warrick H. Ball, Martin Bo Nielsen, C. G. Tinney, Sarbani Basu, Travis S. Metcalfe, Mutlu Yildiz, Rafael A. García, Enrico Corsaro, William J. Chaplin
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Chontos, A, Huber, D, Berger, T A, Kjeldsen, H, Serenelli, A M, Silva Aguirre, V, Ball, W H, Basu, S, Bedding, T R, Chaplin, W J, Claytor, Z R, Corsaro, E, Garcia, R A, Howell, S B, Lundkvist, M S, Mathur, S, Metcalfe, T S, Nielsen, M B, Mian Joel Ong, J, Celik Orhan, Z, Ortel, S, Salama, M, Stassun, K G, Townsend, R H D, Van Saders, J L, Winther, M, Yildiz, M, Butler, R P, Tinney, C G & Wittenmyer, R A 2021, ' TESS Asteroseismology of α Mensae : Benchmark Ages for a G7 Dwarf and Its M Dwarf Companion ', Astrophysical Journal, vol. 922, no. 2, 229 . https://doi.org/10.3847/1538-4357/ac1269
instname
Chontos, A, Huber, D, Berger, T A, Kjeldsen, H, Serenelli, A M, Silva Aguirre, V, Ball, W H, Basu, S, Bedding, T R, Chaplin, W J, Claytor, Z R, Corsaro, E, Garcia, R A, Howell, S B, Lundkvist, M S, Mathur, S, Metcalfe, T S, Nielsen, M B, Mian Joel Ong, J, Celik Orhan, Z, Ortel, S, Salama, M, Stassun, K G, Townsend, R H D, Van Saders, J L, Winther, M, Yildiz, M, Butler, R P, Tinney, C G & Wittenmyer, R A 2021, ' TESS Asteroseismology of α Mensae : Benchmark Ages for a G7 Dwarf and Its M Dwarf Companion ', Astrophysical Journal, vol. 922, no. 2, 229 . https://doi.org/10.3847/1538-4357/ac1269
Asteroseismology of bright stars has become increasingly important as a method to determine the fundamental properties (in particular ages) of stars. The Kepler Space Telescope initiated a revolution by detecting oscillations in more than 500 main-se
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::abcd89a11dcf25bc55af6ddc2c47c1b9
http://hdl.handle.net/10261/261934
http://hdl.handle.net/10261/261934
Autor:
Travis A. Berger, Jennifer L. van Saders, Daniel Huber, Eric Gaidos, Joshua E. Schlieder, Zachary R. Claytor
Publikováno v:
The Astrophysical Journal. 936:100
Current spectroscopic surveys are producing large catalogs of chemical abundances for stars of all types. The yttrium to magnesium ratio, [Y/Mg], has emerged as a candidate age indicator for solar twins in the local stellar neighborhood. However, it
Autor:
Benjamin J. Hord, Knicole D. Colón, Travis A. Berger, Veselin Kostov, Michele L. Silverstein, Keivan G. Stassun, Jack J. Lissauer, Karen A. Collins, Richard P. Schwarz, Ramotholo Sefako, Carl Ziegler, César Briceño, Nicholas Law, Andrew W. Mann, George R. Ricker, David W. Latham, S. Seager, Joshua N. Winn, Jon M. Jenkins, Luke G. Bouma, Ben Falk, Guillermo Torres, Joseph D. Twicken, Andrew Vanderburg
Publikováno v:
The Astronomical Journal. 164:13
Hot Jupiters are generally observed to lack close planetary companions, a trend that has been interpreted as evidence for high-eccentricity migration. We present the discovery and validation of WASP-132 c (TOI-822.02), a 1.85 $\pm$ 0.10 $R_{\oplus}$
Autor:
A. Ueda, Klaus W. Hodapp, M. Salama, R. A. Lee, Samuel K. Grunblatt, Tomoyuki Kudo, E. Gaidos, Shane Jacobson, Takashi Kurokawa, Travis A. Berger, Jun Nishikawa, Hiroki Harakawa, Takuma Serizawa, Masayuki Kuzuhara, M. Ansdell, Sébastien Vievard, Takayuki Kotani, Adam L. Kraus, Michael C. Liu, Z. Zhang, M. Omiya, Motohide Tamura, Teriyuki Hirano, M. Konishi
We report the discovery of a resolved (0".9) substellar companion to a member of the 1-5 Myr Taurus star-forming region. The host star (2M0437) is a single mid-M type ($T_{eff}\approx$3100K) dwarf with a position, space motion, and color-magnitude th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9b2a5b22d6a543b930a50eb69419d9ad
Autor:
Ruth Angus, Daniel Foreman-Mackey, Yuxi Lu, Jennifer L. van Saders, Angus Beane, Travis A. Berger, Rocio Kiman, Adrian M. Price-Whelan, Elisabeth R. Newton, Jason L. Curtis, Lauren Anderson, Jacqueline K. Faherty
The rotational evolution of cool dwarfs is poorly constrained after around 1-2 Gyr due to a lack of precise ages and rotation periods for old main-sequence stars. In this work we use velocity dispersion as an age proxy to reveal the temperature-depen
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d2a93e60de55d8fd82fea82fe1431f49
http://arxiv.org/abs/2005.09387
http://arxiv.org/abs/2005.09387