Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Wolf Cukier"'
Autor:
Jason F. Rowe, Damien Ségransan, Trifon Trifonov, Francesco Pepe, David W. Latham, Giuseppe Pappa, Andrei Tokovinin, Roland Vanderspek, Jon M. Jenkins, Guillermo Torres, Patricia T. Boyd, Billy Quarles, Cesar Briceno, Joel Bergeron, Marc Huten, Andrew Collier Cameron, Stephen R. Kane, Don Pollacco, Joshua N. Winn, Ravi Kumar Kopparapu, Peter Ansorge, Oliver Turner, Gongjie Li, William F. Welsh, Pierre F. L. Maxted, Frank Barnet, Carl Ziegler, Stéphane Udry, Coel Hellier, Eric T. Wolf, Nader Haghighipour, Tsevi Mazeh, Emily A. Gilbert, Nicholas M. Law, Alan M. Levine, Michaël Gillon, Sara Seager, Thomas Barclay, Andrew W. Mann, Daniel C. Fabrycky, Alexandre C. M. Correia, David V. Martin, Jack J. Lissauer, Adina D. Feinstein, Rosemary A. Mardling, Courtney D. Dressing, Vedad Kunovac Hodžić, Benjamin T. Montet, Jacob Haqq-Misra, Nora L. Eisner, Jerome A. Orosz, Samuel N. Quinn, Mark E. Rose, Wolf Cukier, Matthew R. Standing, Donald R. Short, Timo van der Straeten, Veselin B. Kostov, J. Pepper, G. Furesz, Alexandre Santerne, Joseph D. Twicken, Samuel Gill, George R. Ricker, Amaury H. M. J. Triaud, Chris Lintott, Jeffrey C. Smith, Elisa V. Quintana
Publikováno v:
The Astronomical Journal
The Astronomical Journal, 2020, 159, ⟨10.3847/1538-3881/ab8a48⟩
The Astronomical Journal, 2020, 159, ⟨10.3847/1538-3881/ab8a48⟩
We report the detection of the first circumbinary planet found by TESS. The target, a known eclipsing binary, was observed in sectors 1 through 12 at 30-minute cadence and in sectors 4 through 12 at two-minute cadence. It consists of two stars with m
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::aa8fd651d3a229bf408598d963de6f48
https://eprints.keele.ac.uk/8818/1/Kostov_2020_AJ_159_253.pdf
https://eprints.keele.ac.uk/8818/1/Kostov_2020_AJ_159_253.pdf
Autor:
Veselin B. Kostov, Stephen R. Kane, Ravi Kumar Kopparapu, Eric T. Wolf, Jacob Haqq-Misra, Wolf Cukier, William F. Welsh
We use a one-dimensional (1-D) cloud-free climate model to estimate habitable zone (HZ) boundaries for terrestrial planets of masses 0.1 M$_{E}$ and 5 M$_{E}$ around circumbinary stars of various spectral type combinations. Specifically, we consider
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7275f615614f64993fa6f09f84d7e01a
http://arxiv.org/abs/1911.02983
http://arxiv.org/abs/1911.02983
Autor:
Wolf Cukier, Ravi kumar Kopparapu, Stephen R. Kane, William Welsh, Eric Wolf, Veselin Kostov, Jacob Haqq-Misra
Publikováno v:
Publications of the Astronomical Society of the Pacific; Dec2019, Vol. 131 Issue 1006, p1-1, 1p
