Zobrazeno 1 - 2
of 2
pro vyhledávání: '"Thomas N. Gautier III"'
Autor:
William J. Borucki, David G. Koch, Gibor Basri, Natalie Batalha, Alan Boss, Timothy M. Brown, Douglas Caldwell, Jørgen Christensen-Dalsgaard, William D. Cochran, Edna DeVore, Edward W. Dunham, Andrea K. Dupree, Thomas N. Gautier III, John C. Geary, Ronald Gilliland, Alan Gould, Steve B. Howell, Jon M. Jenkins, Hans Kjeldsen, David W. Latham, Jack J. Lissauer, Geoffrey W. Marcy, David G. Monet, Dimitar Sasselov, Jill Tarter, David Charbonneau, Laurance Doyle, Eric B. Ford, Jonathan Fortney, Matthew J. Holman, Sara Seager, Jason H. Steffen, William F. Welsh, Christopher Allen, Stephen T. Bryson, Lars Buchhave, Hema Chandrasekaran, Jessie L. Christiansen, David Ciardi, Bruce D. Clarke, Jessie L. Dotson, Michael Endl, Debra Fischer, Francois Fressin, Michael Haas, Elliott Horch, Andrew Howard, Howard Isaacson, Jeffery Kolodziejczak, Jie Li, Phillip MacQueen, Søren Meibom, Andrej Prsa, Elisa V. Quintana, Jason Rowe, William Sherry, Peter Tenenbaum, Guillermo Torres, Joseph D. Twicken, Jeffrey Van Cleve, Lucianne Walkowicz, Hayley Wu
Publikováno v:
Borucki, W J, Koch, D G, Basri, G, Batalha, N, Boss, A, Brown, T M, Caldwell, D, Christensen-Dalsgaard, J, Cochran, W D, DeVore, E, Dunham, E W, Dupree, A K, Gautier III, T N, Geary, J C, Gilliland, R, Gould, A, Howell, S B, Jenkins, J M, Kjeldsen, H, Latham, D W, Lissauer, J J, Marcy, G W, Monet, D G, Sasselov, D, Tarter, J, Charbonneau, D, Doyle, L, Ford, E B, Fortney, J, Holman, M J, Seager, S, Steffen, J H, Welsh, W F, Allen, C, Bryson, S T, Buchhave, L, Chandrasekaran, H, Christiansen, J L, Ciardi, D, Clarke, B D, Dotson, J L, Endl, M, Fischer, D, Fressin, F, Haas, M, Horch, E, Howard, A, Isaacson, H, Kolodziejczak, J, Li, J, MacQueen, P, Meibom, S, Prsa, A, Quintana, E V, Rowe, J, Sherry, W, Tenenbaum, P, Torres, G, Twicken, J D, Van Cleve, J, Walkowicz, L & Wu, H 2011, ' Characteristics of Kepler Planetary Candidates Based on the First Data Set ', Astrophysical Journal, vol. 728, no. 2/article id. 117 . https://doi.org/10.1088/0004-637X/728/2/117
In the spring of 2009, the Kepler Mission commenced high-precision photometry on nearly 156,000 stars to determine the frequency and characteristics of small exoplanets, conduct a guest observer program, and obtain asteroseismic data on a wide variet
Autor:
Guillermo Torres, François Fressin, Natalie M. Batalha, William J. Borucki, Timothy M. Brown, Stephen T. Bryson, Lars A. Buchhave, David Charbonneau, David R. Ciardi, Edward W. Dunham, Daniel C. Fabrycky, Eric B. Ford, Thomas N. Gautier III, Ronald L. Gilliland, Matthew J. Holman, Steve B. Howell, Howard Isaacson, Jon M. Jenkins, David G. Koch, David W. Latham, Jack J. Lissauer, Geoffrey W. Marcy, David G. Monet, Andrej Prsa, Samuel N. Quinn, Darin Ragozzine, Jason F. Rowe, Dimitar D. Sasselov, Jason H. Steffen, William F. Welsh
Publikováno v:
The Astrophysical Journal. 727:24
Light curves from the Kepler Mission contain valuable information on the nature of the phenomena producing the transit-like signals. To assist in exploring the possibility that they are due to an astrophysical false positive, we describe a procedure