Zobrazeno 1 - 10
of 33
pro vyhledávání: '"Chandrasekaran, Hema"'
Autor:
Jenkins, Jon M., Borucki, William J., Koch, David G., Marcy, Geoffrey W., Cochran, William D., Basri, Gibor, Batalha, Natalie M., Buchhave, Lars A., Brown, Tim M., Caldwell, Douglas A., Dunham, Edward W., Endl, Michael, Fischer, Debra A., Gautier III, Thomas N., Geary, John C., Gilliland, Ronald L., Howell, Steve B., Isaacson, Howard, Johnson, John Asher, Latham, David W., Lissauer, Jack J., Monet, David G., Rowe, Jason F., Sasselov, Dimitar D., Welsh, William F., Howard, Andrew W., MacQueen, Phillip, Chandrasekaran, Hema, Twicken, Joseph D., Bryson, Stephen T., Quintana, Elisa V., Clarke, Bruce D., Li, Jie, Allen, Christopher, Tenenbaum, Peter, Wu, Hayley, Meibom, Soren, Klaus, Todd C., Middour, Christopher K., Cote, Miles T., McCauliff, Sean, Girouard, Forrest R., Gunter, Jay P., Wohler, Bill, Hall, Jennifer R., Ibrahim, Khadeejah, Uddin, AKM Kamal, Wu, Michael S., Bhavsar, Paresh A., Van Cleve, Jeffrey, Pletcher, David L., Dotson, Jessie A., Haas, Michael R.
We report the discovery and the Rossiter-McLaughlin effect of Kepler-8b, a transiting planet identified by the NASA Kepler Mission. Kepler photometry and Keck-HIRES radial velocities yield the radius and mass of the planet around this F8IV subgiant h
Externí odkaz:
http://arxiv.org/abs/1001.0416
Autor:
Bryson, Stephen T., Tenenbaum, Peter, Jenkins, Jon M., Chandrasekaran, Hema, Klaus, Todd, Caldwell, Douglas A., Gilliland, Ronald L., Haas, Michael R., Dotson, Jessie L., Koch, David G., Borucki, William J.
Kepler seeks to detect sequences of transits of Earth-size exoplanets orbiting Solar-like stars. Such transit signals are on the order of 100 ppm. The high photometric precision demanded by Kepler requires detailed knowledge of how the Kepler pixels
Externí odkaz:
http://arxiv.org/abs/1001.0331
Autor:
Jenkins, Jon M., Caldwell, Douglas A., Chandrasekaran, Hema, Twicken, Joseph D., Bryson, Stephen T., Quintana, Elisa V., Clarke, Bruce D., Li, Jie, Allen, Christopher, Tenenbaum, Peter, Wu, Hayley, Klaus, Todd C., Van Cleve, Jeffrey, Dotson, Jessie A., Haas, Michael R., Gilliland, Ronald L., Koch, David G., Borucki, William J.
The Kepler Mission seeks to detect Earth-size planets transiting solar-like stars in its ~115 deg^2 field of view over the course of its 3.5 year primary mission by monitoring the brightness of each of ~156,000 Long Cadence stellar targets with a tim
Externí odkaz:
http://arxiv.org/abs/1001.0256
Autor:
Koch, David G., Borucki, William J., Basri, Gibor, Batalha, Natalie M., Brown, Timothy M., Caldwell, Douglas, Christensen-Dalsgaard, Joergen, Cochran, William D., DeVore, Edna, Dunham, Edward W., Gautier III, Thomas N., Geary, John C., Gilliland, Ronald L., Gould, Alan, Jenkins, Jon, Kondo, Yoji, Latham, David W., Lissauer, Jack J., Marcy, Geoffrey, Monet, David, Sasselov, Dimitar, Boss, Alan, Brownlee, Donald, Caldwell, John, Dupree, Andrea K., Howell, Steve B., Kjeldsen, Hans, Meibom, Soeren, Morrison, David, Owen, Tobias, Reitsema, Harold, Tarter, Jill, Bryson, Stephen T., Dotson, Jessie L., Gazis, Paul, Haas, Michael R., Kolodziejczak, Jeffrey, Rowe, Jason F., Van Cleve, Jeffrey E., Allen, Christopher, Chandrasekaran, Hema, Clarke, Bruce D., Li, Jie, Quintana, Elisa V., Tenenbaum, Peter, Twicken, Joseph D., Wu, Hayley
The Kepler Mission, launched on Mar 6, 2009 was designed with the explicit capability to detect Earth-size planets in the habitable zone of solar-like stars using the transit photometry method. Results from just forty-three days of data along with gr
Externí odkaz:
http://arxiv.org/abs/1001.0268
Autor:
Caldwell, Douglas A., Kolodziejczak, Jeffery J., Van Cleve, Jeffrey E., Jenkins, Jon M., Gazis, Paul R., Argabright, Vic S., Bachtell, Eric E., Dunham, Edward W., Geary, John C., Gilliland, Ronald L., Chandrasekaran, Hema, Li, Jie, Tenenbaum, Peter, Wu, Hayley, Borucki, William J., Bryson, Stephen T., Dotson, Jessie L., Haas, Michael R., Koch, David G.
The Kepler Mission relies on precise differential photometry to detect the 80 parts per million (ppm) signal from an Earth-Sun equivalent transit. Such precision requires superb instrument stability on time scales up to ~2 days and systematic error r
Externí odkaz:
http://arxiv.org/abs/1001.0216
Autor:
Jenkins, Jon M., Caldwell, Douglas A., Chandrasekaran, Hema, Twicken, Joseph D., Bryson, Stephen T., Quintana, Elisa V., Clarke, Bruce D., Li, Jie, Allen, Christopher, Tenenbaum, Peter, Wu, Hayley, Klaus, Todd C., Middour, Christopher K., Cote, Miles T., McCauliff, Sean, Girouard, Forrest R., Gunter, Jay P., Wohler, Bill, Sommers, Jeneen, Hall, Jennifer R., Uddin, Kamal, Wu, Michael S., Bhavsar, Paresh A., Van Cleve, Jeffrey, Pletcher, David L., Dotson, Jessie A., Haas, Michael R., Gilliland, Ronald L., Koch, David G., Borucki, William J.
The Kepler Mission Science Operations Center (SOC) performs several critical functions including managing the ~156,000 target stars, associated target tables, science data compression tables and parameters, as well as processing the raw photometric d
Externí odkaz:
http://arxiv.org/abs/1001.0258
Autor:
Borucki, William J., Koch, David, Basri, Gibor, Batalha, Natalie, Brown, Timothy, Caldwell, Douglas, Caldwell, John, Christensen-Dalsgaard, Jørgen, Cochran, William D., DeVore, Edna, Dunham, Edward W., Dupree, Andrea K., Gautier, Thomas N., Geary, John C., Gilliland, Ronald, Gould, Alan, Howell, Steve B., Jenkins, Jon M., Kondo, Yoji, Latham, David W., Marcy, Geoffrey W., Meibom, Soren, Kjeldsen, Hans, Lissauer, Jack J ., Monet, David G., Morrison, David, Sasselov, Dimitar, Tarter, Jill, Boss, Alan, Brownlee, Don, Owen, Toby, Buzasi, Derek, Charbonneau, David, Doyle, Laurance, Fortney, Jonathan, Ford, Eric B., Holman, Matthew J., Seager, Sara, Steffen, Jason H., Welsh, William F., Rowe, Jason, Anderson, Howard, Buchhave, Lars, Ciardi, David, Walkowicz, Lucianne, Sherry, William, Horch, Elliott, Isaacson, Howard, Everett, Mark E., Fischer, Debra, Torres, Guillermo, Johnson, John Asher, Endl, Michael, MacQueen, Phillip, Bryson, Stephen T., Dotson, Jessie, Haas, Michael, Kolodziejczak, Jeffrey, Van Cleve, Jeffrey, Chandrasekaran, Hema, Twicken, Joseph D., Quintana, Elisa V., Clarke, Bruce D., Allen, Christopher, Li, Jie, Wu, Haley, Tenenbaum, Peter, Verner, Ekaterina, Bruhweiler, Frederick, Barnes, Jason, Prsa, Andrej
Publikováno v:
Science, 2010 Feb . 327(5968), 977-980.
Externí odkaz:
https://www.jstor.org/stable/40509955
Akademický článek
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Autor:
Chandrasekaran, Hema, Li, Jiang, Delashmit, W.H., Narasimha, P.L., Yu, Changhua, Manry, Michael T.
Publikováno v:
In Neurocomputing 2007 70(4):1022-1039
Akademický článek
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