Zobrazeno 1 - 10
of 129
pro vyhledávání: '"Rowe J. F."'
Autor:
Campante T. L., Barclay T., Swift J. J., Huber D., Adibekyan V. Zh., Cochran W., Burke C. J., Isaacson H., Quintana E. V., Davies G. R., Silva Aguirre V., Ragozzine D., Riddle R., Baranec C., Basu S., Chaplin W. J., Christensen-Dalsgaard J., Metcalfe T. S., Bedding T. R., Handberg R., Stello D., Brewer J. M., Hekker S., Karoff C., Kolbl R., Law N. M., Lundkvist M., Miglio A., Rowe J. F., Santos N. C., Van Laerhoven C., Arentoft T., Elsworth Y. P., Fischer D. A., Kawaler S. D., Kjeldsen H., Lund M. N., Marcy G. W., Sousa S. G., Sozzetti A., White T. R.
Publikováno v:
EPJ Web of Conferences, Vol 101, p 02004 (2015)
The first discoveries of exoplanets around Sun-like stars have fueled efforts to find ever smaller worlds evocative of Earth and other terrestrial planets in the Solar System. While gas-giant planets appear to form preferentially around metal-rich st
Externí odkaz:
https://doaj.org/article/88d4a77566b74be7bc827926515b813e
Autor:
Sulis, S., Dragomir, D., Lendl, M., Bourrier, V., Demory, B. O., Fossati, L., Cubillos, P. E., Guenther, D. B., Kane, S. R., Kuschnig, R., Matthews, J. M., Moffat, A. F. J., Rowe, J. F., Sasselov, D., Weiss, W. W., Winn, J. N.
Publikováno v:
A&A 631, A129 (2019)
Context. 55 Cnc e is a transiting super-Earth orbiting a solar-like star with an orbital period of 17.7 hours. In 2011, using the MOST space telescope, a quasi-sinusoidal modulation in flux was detected with the same period as the planetary orbit. Th
Externí odkaz:
http://arxiv.org/abs/1910.00383
Autor:
Siwak, M., Ogloza, W., Moffat, A. F. J., Matthews, J. M., Rucinski, S. M., Kallinger, T., Kuschnig, R., Cameron, C., Weiss, W. W., Rowe, J. F., Guenther, D. B., Sasselov, D.
This is the final photometric study of TW Hya based on new MOST satellite observations. During 2014 and 2017 the light curves showed stable 3.75 and 3.69 d quasi-periodic oscillations, respectively. Both values appear to be closely related with the s
Externí odkaz:
http://arxiv.org/abs/1805.04547
Autor:
Gaulme, P., Rowe, J. F., Bedding, T. R., Benomar, O., Corsaro, E., Davies, G. R., Hale, S. J., Howe, R., Garcia, R. A., Huber, D., Jiménez, A., Mathur, S., Mosser, B., Appourchaux, T., Boumier, P., Jackiewicz, J., Leibacher, J., Schmider, F. -X., Hammel, H. B., Lissauer, J. J., Marley, M. S., Simon, A. A., Chaplin, W. J., Elsworth, Y., Guzik, J. A., Murphy, N., Aguirre, V. Silva
Publikováno v:
The Astrophysical Journal Letters, Volume 833, Issue 1, article id. L13, 7 pp. (2016)
Starting in December 2014, Kepler K2 observed Neptune continuously for 49 days at a 1-minute cadence. The goals consisted of studying its atmospheric dynamics (Simon et al. 2016), detecting its global acoustic oscillations (Rowe et al., submitted), a
Externí odkaz:
http://arxiv.org/abs/1612.04287
Autor:
Guzik, J. A., Houdek, G., Chaplin, W. J., Smalley, B., Kurtz, D. W., Gilliland, R. L., Mullally, F., Rowe, J. F., Bryson, S. T., Still, M. D., Antoci, V., Appourchaux, T., Basu, S., Bedding, T. R., Benomar, O., Garcia, R. A., Huber, D., Kjeldsen, H., Latham, D. W., Metcalfe, T. S., Pápics, P. I., White, T. R., Aerts, C., Ballot, J., Boyajian, T. S., Briquet, M., Bruntt, H., Buchhave, L. A., Campante, T. L., Catanzaro, G., Christensen-Dalsgaard, J., Davies, G. R., Doğan, G., Dragomir, D., Doyle, A. P., Elsworth, Y., Frasca, A., Gaulme, P., Gruberbauer, M., Handberg, R., Hekker, S., Karoff, C., Lehmann, H., Mathias, P., Mathur, S., Miglio, A., Molenda-Żakowicz, J., Mosser, B., Murphy, S. J., Régulo, C., Ripepi, V., Salabert, D., Sousa, S. G., Stello, D., Uytterhoeven, K.
$\theta$ Cygni is an F3 spectral-type main-sequence star with visual magnitude V=4.48. This star was the brightest star observed by the original Kepler spacecraft mission. Short-cadence (58.8 s) photometric data using a custom aperture were obtained
Externí odkaz:
http://arxiv.org/abs/1607.01035
Autor:
Lundkvist, M. S., Kjeldsen, H., Albrecht, S., Davies, G. R., Basu, S., Huber, D., Justesen, A. B., Karoff, C., Aguirre, V. Silva, Van Eylen, V., Vang, C., Arentoft, T., Barclay, T., Bedding, T. R., Campante, T. L., Chaplin, W. J., Christensen-Dalsgaard, J., Elsworth, Y. P., Gilliland, R. L., Handberg, R., Hekker, S., Kawaler, S. D., Lund, M. N., Metcalfe, T. S., Miglio, A., Rowe, J. F., Stello, D., Tingley, B., White, T. R.
Publikováno v:
Nature Communications, Volume 7, id. 11201 (2016)
Simulations predict that hot super-Earth sized exoplanets can have their envelopes stripped by photo-evaporation, which would present itself as a lack of these exoplanets. However, this absence in the exoplanet population has escaped a firm detection
Externí odkaz:
http://arxiv.org/abs/1604.05220
Autor:
Tkachenko, A., Matthews, J. M., Aerts, C., Pavlovski, K., Papics, P. I., Zwintz, K., Cameron, C., Walker, G. A. H., Kuschnig, R., Degroote, P., Debosscher, J., Moravveji, E., Kolbas, V., Guenther, D. B., Moffat, A. F. J., Rowe, J. F., Rucinski, S. M., Sasselov, D., Weiss, W. W.
Binary stars provide a valuable test of stellar structure and evolution, because the masses of the individual stellar components can be derived with high accuracy and in a model-independent way. In this work, we study Spica, an eccentric double-lined
Externí odkaz:
http://arxiv.org/abs/1601.08069
Autor:
Campante, T. L., Barclay, T., Swift, J. J., Huber, D., Adibekyan, V. Zh., Cochran, W., Burke, C. J., Isaacson, H., Quintana, E. V., Davies, G. R., Aguirre, V. Silva, Ragozzine, D., Riddle, R., Baranec, C., Basu, S., Chaplin, W. J., Christensen-Dalsgaard, J., Metcalfe, T. S., Bedding, T. R., Handberg, R., Stello, D., Brewer, J. M., Hekker, S., Karoff, C., Kolbl, R., Law, N. M., Lundkvist, M., Miglio, A., Rowe, J. F., Santos, N. C., Van Laerhoven, C., Arentoft, T., Elsworth, Y. P., Fischer, D. A., Kawaler, S. D., Kjeldsen, H., Lund, M. N., Marcy, G. W., Sousa, S. G., Sozzetti, A., White, T. R.
The chemical composition of stars hosting small exoplanets (with radii less than four Earth radii) appears to be more diverse than that of gas-giant hosts, which tend to be metal-rich. This implies that small, including Earth-size, planets may have r
Externí odkaz:
http://arxiv.org/abs/1501.06227
Autor:
Evans, N. R., Szabó, R., Derekas, A., Szabados, L., Cameron, C., Matthews, J. M., Sasselov, D., Kuschnig, R., Rowe, J. F., Guenther, D. B., Moffat, A. F. J., Rucinski, S. M., Weiss, W. W.
The quantity and quality of satellite photometric data strings is revealing details in Cepheid variation at very low levels. Specifically, we observed a Cepheid pulsating in the fundamental mode and one pulsating in the first overtone with the Canadi
Externí odkaz:
http://arxiv.org/abs/1411.1730
Autor:
Sódor, Á., Chené, A. -N., De Cat, P., Bognár, Zs., Wright, D. J., Marois, C., Walker, G. A. H., Matthews, J. M., Kallinger, T., Rowe, J. F., Kuschnig, R., Guenther, D. B., Moffat, A. F. J., Rucinski, S. M., Sasselov, D., Weiss, W. W.
Publikováno v:
A&A 568, A106 (2014)
Context: The central star of the HR 8799 system is a gamma Doradus-type pulsator. The system harbours four planetary-mass companions detected by direct imaging, and is a good solar system analogue. The masses of the companions are not known accuratel
Externí odkaz:
http://arxiv.org/abs/1407.0267