Zobrazeno 1 - 10
of 283
pro vyhledávání: '"Borucki W"'
Autor:
Furlan, E., Ciardi, D. R., Cochran, W. D., Everett, M. E., Latham, D. W., Marcy, G. W., Buchhave, L. A., Endl, M., Isaacson, H., Petigura, E. A., Gautier III, T. N., Huber, D., Bieryla, A., Borucki, W. J., Brugamyer, E., Caldwell, C., Cochran, A., Howard, A. W., Howell, S. B., Johnson, M. C., MacQueen, P. J., Quinn, S. N., Robertson, P., Mathur, S., Batalha, N. M.
We present results from spectroscopic follow-up observations of stars identified in the Kepler field and carried out by teams of the Kepler Follow-Up Observation Program. Two samples of stars were observed over six years (2009-2015): 614 standard sta
Externí odkaz:
http://arxiv.org/abs/1805.12089
Akademický článek
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Autor:
Borucki, W. J., Agol, E., Fressin, F., Kaltenegger, L., Rowe, J., Isaacson, H., Fischer, D., Batalha, N., Lissauer, J. J., Marcy, G. W., Fabrycky, D., Désert, J. -M., Bryson, S. T., Barclay, T., Bastien, F., Boss, A., Brugamyer, E., Buchhave, L. A., Burke, Chris, Caldwell, D. A., Carter, J., Charbonneau, D., Crepp, J. R., Christensen-Dalsgaard, J., Christiansen, J. L., Ciardi, D., Cochran, W. D., DeVore, E., Doyle, L., Dupree, A. K., Endl, M., Everett, M. E., Ford, E. B., Fortney, J., Gautier III, T. N., Geary, J. C., Gould, A., Haas, M., Henze, C., Howard, A. W., Howell, S. B., Huber, D., Jenkins, J. M., Kjeldsen, H., Kolbl, R., Kolodziejczak, J., Latham, D. W., Lee, B. L., Lopez, E., Mullally, F., Orosz, J. A., Prsa, A., Quintana, E. V., Sanchez-Ojeda, R., Sasselov, D., Seader, S., Shporer, A., Steffen, J. H., Still, M., Tenenbaum, P., Thompson, S. E., Torres, G., Twicken, J. D., Welsh, W. F., Winn, J. N.
Publikováno v:
Science Express / http://www.sciencemag.org/content/early/recent / 18 April 2013 / Page 1/ 10.1126/science.1234702
We present the detection of five planets -- Kepler-62b, c, d, e, and f -- of size 1.31, 0.54, 1.95, 1.61 and 1.41 Earth radii, orbiting a K2V star at periods of 5.7, 12.4, 18.2, 122.4 and 267.3 days, respectively. The outermost planets (Kepler-62e &
Externí odkaz:
http://arxiv.org/abs/1304.7387
Autor:
Chaplin, W. J., Kjeldsen, H., Christensen-Dalsgaard, J., Basu, S., Miglio, A., Appourchaux, T., Bedding, T. R., Elsworth, Y., García, R. A., Gilliland, R. L., Girardi, L., Houdek, G., Karoff, C., Kawaler, S. D., Metcalfe, T. S., Molenda-Zakowicz, J., Monteiro, M. J. P. F. G., Thompson, M. J., Verner, G. A., Ballot, J., Bonanno, A., Brandao, I. M., Broomhall, A. -M., Bruntt, H., Campante, T. L., Corsaro, E., Creevey, O. L., Dogan, G., Esch, L., Gai, N., Gaulme, P., Hale, S. J., Handberg, R., Hekker, S., Huber, D., Jiménez, A., Mathur, S., Mazumdar, A., Mosser, B., New, R., Pinsonneault, M. H., Pricopi, D., Quirion, P. -O., Régulo, C., Salabert, D., Serenelli, A. M., Aguirre, V. Silva, Sousa, S. G., Stello, D., Stevens, I. R., Suran, M. D., Uytterhoeven, K., White, T. R., Borucki, W. J., Brown, T. M., Jenkins, J. M., Kinemuchi, K., Van Cleve, J., Klaus, T. C.
Publikováno v:
Science, 2011, volume 332, page 213
In addition to its search for extra-solar planets, the NASA Kepler Mission provides exquisite data on stellar oscillations. We report the detections of oscillations in 500 solartype stars in the Kepler field of view, an ensemble that is large enough
Externí odkaz:
http://arxiv.org/abs/1109.4723
Autor:
Nemec, J. M., Smolec, R., Benko, J. M., Moskalik, P., Kolenberg, K., Szabo, R., Kurtz, D. W., Bryson, S., Guggenberger, E., Chadid, M., Jeon, Y. -B., Kunder, A., Layden, A. C., Kinemuchi, K., Kiss, L. L., Poretti, E., Christensen-Dalsgaard, J., Kjeldsen, H., Caldwell, D., Ripepi, V., Derekas, A., Nuspl, J., Mullally, F., Thompson, S. E., Borucki, W. J.
This paper summarizes the main results of our recent study of the non-Blazhko RR Lyrae stars observed with the Kepler space telescope. These stars offer the opportunity for studying the stability of the pulsations of RR Lyrae stars and for providing
Externí odkaz:
http://arxiv.org/abs/1108.5683
Autor:
Nemec, J. M., Smolec, R., Benko, J. M., Moskalik, P., Kolenberg, K., Szabo, R., Kurtz, D. W., Bryson, S., Guggenberger, E., Chadid, M., Jeon, Y. -B., Kunder, A., Layden, A. C., Kinemuchi, K., Kiss, L. L., Poretti, E., Christensen-Dalsgaard, J., Kjeldsen, H., Caldwell, D., Ripepi, V., Derekas, A., Nuspl, J., Mullally, F., Thompson, S. E., Borucki, W. J.
Publikováno v:
MNRAS 417, 1022-1053, 2011
Nineteen of the ~40 RR Lyr stars in the Kepler field have been identified as candidate non-Blazhko (or unmodulated) stars. In this paper we present the results of Fourier decomposition of the time-series photometry of these stars acquired during the
Externí odkaz:
http://arxiv.org/abs/1106.6120
Autor:
Steffen, J. H., Quinn, S. N., Borucki, W. J., Brugamyer, E., Bryson, S. T., Buchhave, L. A., Cochran, W. D., Endl, M., Fabrycky, D. C., Ford, E. B., Holman, M. J., Jenkins, J., Koch, D., Latham, D. W., MacQueen, P., Mullally, F., Prsa, A., Ragozzine, D., Rowe, J. F., Sanderfer, D. T., Seader, S. E., Short, D., Shporer, A., Thompson, S. E., Torres, G., Twicken, J. D., Welsh, W. F., Windmiller, G.
We present a hierarchical triple star system (KIC 9140402) where a low mass eclipsing binary orbits a more massive third star. The orbital period of the binary (4.98829 Days) is determined by the eclipse times seen in photometry from NASA's Kepler sp
Externí odkaz:
http://arxiv.org/abs/1106.4530
Autor:
Chaplin, W. J., Kjeldsen, H., Bedding, T. R., Christensen-Dalsgaard, J., Gilliland, R. L., Kawaler, S. D., Appourchaux, T., Elsworth, Y., Garcia, R. A., Houdek, G., Karoff, C., Metcalfe, T. S., Molenda-Zakowicz, J., Monteiro, M. J. P. F. G., Thompson, M. J., Verner, G. A., Batalha, N., Borucki, W. J., Brown, T. M., Bryson, S. T., Christiansen, J. L., Clarke, B. D., Jenkins, J. M., Klaus, T. C., Koch, D., An, D., Ballot, J., Basu, S., Benomar, O., Bonanno, A., Broomhall, A. -M., Campante, T. L., Corsaro, E., Creevey, O. L., Esch, L., Gai, N., Gaulme, P., Hale, S. J., Handberg, R., Hekker, S., Huber, D., Mathur, S., Mosser, B., New, R., Pinsonneault, M. H., Pricopi, D., Quirion, P. -O., Regulo, C., Roxburgh, I. W., Salabert, D., Stello, D., Suran, M. D.
Asteroseismology of solar-type stars has an important part to play in the exoplanet program of the NASA Kepler Mission. Precise and accurate inferences on the stellar properties that are made possible by the seismic data allow very tight constraints
Externí odkaz:
http://arxiv.org/abs/1103.0702
Autor:
Kolenberg, K., Bryson, S., Szabó, R., Kurtz, D. W., Smolec, R., Nemec, J. M., Guggenberger, E., Moskalik, P., Benkő, J. M., Chadid, M., Jeon, Y. -B., Kiss, L. L., Kopacki, G., Nuspl, J., Still, M., Christensen-Dalsgaard, J., Kjeldsen, H., Borucki, W. J., Caldwell, D. A., Jenkins, J. M., Koch, D.
Publikováno v:
MNRAS, 411, 878 (2011)
We present our analysis of the long cadence Kepler data for the well-studied Blazhko star RR Lyr, gathered during the first two quarters of the satellite's observations and covering a total of 127d. Besides being of great importance for our understan
Externí odkaz:
http://arxiv.org/abs/1011.5908
Autor:
Kallinger, T., Mosser, B., Hekker, S., Huber, D., Stello, D., Mathur, S., Basu, S., Bedding, T. R., Chaplin, W. J., De Ridder, J., Elsworth, Y. P., Frandsen, S., Garcia, R. A., Gruberbauer, M., Matthews, J. M., Borucki, W. J., Bruntt, H., Christensen-Dalsgaard, J., Gilliland, R. L., Kjeldsen, H., Koch, D. G.
Clear power excess in a frequency range typical for solar-type oscillations in red giants has been detected in more than 1000 stars, which have been observed during the first 138 days of the science operation of the NASA Kepler satellite. This sample
Externí odkaz:
http://arxiv.org/abs/1010.4589