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pro vyhledávání: '"Latham, Dave W."'
Autor:
Teske, Johanna, Wang, Sharon Xuesong, Wolfgang, Angie, Gan, Tianjun, Plotnykov, Mykhaylo, Armstrong, David J., Butler, R. Paul, Cale, Bryson, Crane, Jeffrey D., Howard, Ward, Jensen, Eric L. N., Law, Nicholas, Shectman, Stephen A., Plavchan, Peter, Valencia, Diana, Vanderburg, Andrew, Ricker, George, Vanderspek, Roland, Latham, Dave W., Seager, Sara, Winn, Joshua W., Jenkins, Jon M., Adibekyan, Vardan, Barrado, David, Barros, Susana C. C., Benkhaldoun, Zouhair, Brown, David J. A., Bryant, Edward M., Burt, Jennifer, Caldwell, Douglas A., Charbonneau, David, Cloutier, Ryan, Collins, Karen A., Collins, Kevin I., Colon, Nicole D., Conti, Dennis M., Demangeon, Olivier D. S., Eastman, Jason D., Elmufti, Mohammed, Feng, Fabo, Flowers, Erin, Guerrero, Natalia M., Hojjatpanah, Saeed, Irwin, Jonathan M., Isopi, Giovanni, Lillo-Box, Jorge, Mallia, Franco, Massey, Bob, Mori, Mayuko, Mullally, Susan E., Narita, Norio, Nishiumi, Taku, Osborn, Ares, Paegert, Martin, de Leon, Jerome Pitogo, Quinn, Samuel N., Reefe, Michael, Schwarz, Richard P., Shporer, Avi, Soubkiou, Abderahmane, Sousa, Sérgio G., Stockdale, Chris, Strøm, Paul A., Tan, Thiam-Guan, Tenenbaum, Peter, Wheatley, Peter J., Wittrock, Justin, Yahalomi, Daniel A., Zohrabi, Farzaneh
$Kepler$ revealed that roughly one-third of Sun-like stars host planets orbiting within 100 days and between the size of Earth and Neptune. How do these planets form, what are they made of, and do they represent a continuous population or multiple po
Externí odkaz:
http://arxiv.org/abs/2011.11560
We present the first case in which the BEER algorithm identified a hot Jupiter in the Kepler light curve, and its reality was confirmed by orbital solutions based on follow-up spectroscopy. The companion Kepler-76b was identified by the BEER algorith
Externí odkaz:
http://arxiv.org/abs/1304.6841
Autor:
Shporer, Avi, Bakos, Gaspar A., Bouchy, Francois, Pont, Frederic, Kovacs, Geza, Latham, Dave W., Sipocz, Brigitta, Torres, Guillermo, Mazeh, Tsevi, Esquerdo, Gilbert A., Pal, Andras, Noyes, Robert W., Sasselov, Dimitar D., Lazar, Jozsef, Papp, Istvan, Sari, Pal, Kovacs, Gabor
Publikováno v:
Astrophys.J.690:1393-1400,2009
We report the discovery of a planet transiting a moderately faint (V=12.3 mag) late F star, with an orbital period of 3.92289 +/- 0.00004 days. From the transit light curve and radial velocity measurements we determine that the radius of the planet i
Externí odkaz:
http://arxiv.org/abs/0806.4008
Akademický článek
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