Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Stephen R. Kane"'
Autor:
Denise Weigand, Jason J. Wang, Bertrand Mennesson, Veronica Roccatagliata, Dennis A. Afanasev, Russel White, F. Giddens, Diana Dragomir, David W. Latham, Matthew W. Mengel, Andrew Cancino, C. A. Beichman, Johanna Teske, Allison Youngblood, Chris Klenke, Akshata Krishnamurthy, Robert A. Wittenmyer, Keivan G. Stassun, Hui Zhang, Sharon X. Wang, George R. Ricker, Roland Vanderspek, Bernie Walp, Perri Zilberman, Matthew A. Kenworthy, Joshua E. Schlieder, Duncan J. Wright, Natasha Latouf, Joshua Pepper, Ryan Hall, Joshua N. Winn, Thomas Barclay, Ben Tieu, Ian J. M. Crossfield, Karen A. Collins, Dax L. Feliz, Guillem Anglada-Escudé, Daniel Foreman-Mackey, B. Cale, Fred C. Adams, Sean M. Mills, Andrew W. Howard, Jonathan Horner, Brendan P. Bowler, Scott Dynes, Claire Geneser, Angelle Tanner, Emily A. Gilbert, Michael Bottom, John F. Kielkopf, Jonathan Gagné, Jon M. Jenkins, Carolyn Brinkworth, Coel Hellier, David Berardo, Andrew Vanderburg, Sara Seager, William Matzko, S. N. Quinn, America Nishimoto, Carolyn Brown, Elisa V. Quintana, Jack Okumura, David M. Kipping, Kaspar von Braun, John P. Doty, Stephen R. Kane, Joseph Huber, Patrick Lowrance, Cassy Davison, Elisabeth R. Newton, Elise Furlan, Peter Gao, Eric Gaidos, Ethan Kruse, David R. Ciardi, Norio Narita, Timothy D. Morton, Peter Plavchan, Enric Palle, C. G. Tinney, Todd J. Henry, Aki Roberge, Stephen A. Rinehart, Jake T. Clark, Mark Clampin, Chelsea X. Huang
Publikováno v:
Nature. 583:E31-E31
Autor:
Vlada Stamenkovic, Emeline Bolmont, Nikole K. Lewis, Kevin Heng, Stephen R. Kane, Björn Benneke, Julien de Wit, Nikku Madhusudhan, Jessica Krick, Didier Queloz, Tiffany Kataria, Michaël Gillon, Brice-Olivier Demory, Renyu Hu
Publikováno v:
Nature. 532
Over the past decade, observations of giant exoplanets (Jupiter-size) have provided key insights into their atmospheres, but the properties of lower-mass exoplanets (sub-Neptune) remain largely unconstrained because of the challenges of observing sma
Autor:
Kailash C. Sahu, M. Zub, J. P. Beaulieu, D. Kubas, Takahiro Sumi, Radosław Poleski, K. Hill, Martin Dominik, Pascal Fouqué, Ch. Coutures, Igor Soszyński, M. Kubiak, Grzegorz Pietrzyński, J. G. Greenhill, Andrew A. Cole, V. Batista, B. Watson, Arnaud Cassan, J. W. Menzies, J. B. Marquette, J. A. R. Caldwell, C. Vinter, Krzysztof Ulaczyk, J. Donatowicz, D. Warren, K. H. Cook, David P. Bennett, Andrzej Udalski, Michał K. Szymański, S. Brillant, S. Dieters, N. Kains, D. Dominis Prester, Stephen R. Kane, Michael D. Albrow, Andrew Williams, K. R. Pollard, Joachim Wambsganss, U. G. Jørgensen, Łukasz Wyrzykowski, R. Martin, Keith Horne
Publikováno v:
Nature
Most known extrasolar planets (exoplanets) have been discovered using the radial velocity$^{\bf 1,2}$ or transit$^{\bf 3}$ methods. Both are biased towards planets that are relatively close to their parent stars, and studies find that around 17--30%