Zobrazeno 1 - 10
of 20
pro vyhledávání: '"Howard Isaacson"'
Autor:
Merrin S. Peterson, Björn Benneke, Karen Collins, Caroline Piaulet, Ian J. M. Crossfield, Mohamad Ali-Dib, Jessie L. Christiansen, Jonathan Gagné, Jackie Faherty, Edwin Kite, Courtney Dressing, David Charbonneau, Felipe Murgas, Marion Cointepas, Jose Manuel Almenara, Xavier Bonfils, Stephen Kane, Michael W. Werner, Varoujan Gorjian, Pierre-Alexis Roy, Avi Shporer, Francisco J. Pozuelos, Quentin Jay Socia, Ryan Cloutier, Jeremy Dietrich, Jonathan Irwin, Lauren Weiss, William Waalkes, Zach Berta-Thomson, Thomas Evans, Daniel Apai, Hannu Parviainen, Enric Pallé, Norio Narita, Andrew W. Howard, Diana Dragomir, Khalid Barkaoui, Michaël Gillon, Emmanuel Jehin, Elsa Ducrot, Zouhair Benkhaldoun, Akihiko Fukui, Mayuko Mori, Taku Nishiumi, Kiyoe Kawauchi, George Ricker, David W. Latham, Joshua N. Winn, Sara Seager, Howard Isaacson, Alex Bixel, Aidan Gibbs, Jon M. Jenkins, Jeffrey C. Smith, Jose Perez Chavez, Benjamin V. Rackham, Thomas Henning, Paul Gabor, Wen-Ping Chen, Nestor Espinoza, Eric L. N. Jensen, Kevin I. Collins, Richard P. Schwarz, Dennis M. Conti, Gavin Wang, John F. Kielkopf, Shude Mao, Keith Horne, Ramotholo Sefako, Samuel N. Quinn, Dan Moldovan, Michael Fausnaugh, Gábor Fűűrész, Thomas Barclay
Publikováno v:
Nature. 617:701-705
Autor:
Gang Li, Andrew W. Mann, Michael J. Ireland, C. G. Tinney, Daniel Luke Holdsworth, Victoria Antoci, Hans Kjeldsen, Daniel R. Reese, Howard Isaacson, Jie Yu, Timothy R. White, Timothy R. Bedding, Jon M. Jenkins, Adam D. Rains, Dennis Stello, J. J. Hermes, George R. Ricker, Daniel Huber, Simon J. Murphy, William J. Chaplin, Warrick H. Ball, Yaguang Li, S. Sekaran, Roland Vanderspek, Tanda Li, Eric Gaidos, Isabel L. Colman, Christoph Bergmann, Andrew W. Howard, Curtis McCully, Timothy M. Brown, Barry Smalley, Markus Rabus, Daniel Harbeck, Jim Fuller, Daniel R. Hey
Publikováno v:
Nature
Nature, Nature Publishing Group, 2020, 581 (7807), pp.147-151. ⟨10.1038/s41586-020-2226-8⟩
Bedding, T R, Murphy, S J, Hey, D R, Huber, D, Li, T, Smalley, B, Stello, D, White, T R, Ball, W H, Chaplin, W J, Colman, I L, Fuller, J, Gaidos, E, Harbeck, D R, Hermes, J J, Holdsworth, D L, Li, G, Li, Y, Mann, A W, Reese, D R, Sekaran, S, Yu, J, Antoci, V, Bergmann, C, Brown, T M, Howard, A W, Ireland, M J, Isaacson, H, Jenkins, J M, Kjeldsen, H, McCully, C, Rabus, M, Rains, A D, Ricker, G R, Tinney, C G & Vanderspek, R K 2020, ' Very regular high-frequency pulsation modes in young intermediate-mass stars ', Nature, vol. 581, pp. 147-151 . https://doi.org/10.1038/s41586-020-2226-8
Bedding, T R, Murphy, S J, Hey, D R, Huber, D, Li, T, Smalley, B, Stello, D, White, T R, Ball, W H, Chaplin, W J, Colman, I L, Fuller, J, Gaidos, E, Harbeck, D R, Hermes, J J, Holdsworth, D L, Li, G, Li, Y, Mann, A W, Reese, D R, Sekaran, S, Yu, J, Antoci, V, Bergmann, C, Brown, T M, Howard, A W, Ireland, M J, Isaacson, H, Jenkins, J M, Kjeldsen, H, McCully, C, Rabus, M, Rains, A D, Ricker, G R, Tinney, C G & Vanderspek, R K 2020, ' Very regular high-frequency pulsation modes in young intermediate-mass stars ', Nature, vol. 581, no. 7807, pp. 147-151 . https://doi.org/10.1038/s41586-020-2226-8
Nature, Nature Publishing Group, 2020, 581 (7807), pp.147-151. ⟨10.1038/s41586-020-2226-8⟩
Bedding, T R, Murphy, S J, Hey, D R, Huber, D, Li, T, Smalley, B, Stello, D, White, T R, Ball, W H, Chaplin, W J, Colman, I L, Fuller, J, Gaidos, E, Harbeck, D R, Hermes, J J, Holdsworth, D L, Li, G, Li, Y, Mann, A W, Reese, D R, Sekaran, S, Yu, J, Antoci, V, Bergmann, C, Brown, T M, Howard, A W, Ireland, M J, Isaacson, H, Jenkins, J M, Kjeldsen, H, McCully, C, Rabus, M, Rains, A D, Ricker, G R, Tinney, C G & Vanderspek, R K 2020, ' Very regular high-frequency pulsation modes in young intermediate-mass stars ', Nature, vol. 581, pp. 147-151 . https://doi.org/10.1038/s41586-020-2226-8
Bedding, T R, Murphy, S J, Hey, D R, Huber, D, Li, T, Smalley, B, Stello, D, White, T R, Ball, W H, Chaplin, W J, Colman, I L, Fuller, J, Gaidos, E, Harbeck, D R, Hermes, J J, Holdsworth, D L, Li, G, Li, Y, Mann, A W, Reese, D R, Sekaran, S, Yu, J, Antoci, V, Bergmann, C, Brown, T M, Howard, A W, Ireland, M J, Isaacson, H, Jenkins, J M, Kjeldsen, H, McCully, C, Rabus, M, Rains, A D, Ricker, G R, Tinney, C G & Vanderspek, R K 2020, ' Very regular high-frequency pulsation modes in young intermediate-mass stars ', Nature, vol. 581, no. 7807, pp. 147-151 . https://doi.org/10.1038/s41586-020-2226-8
Asteroseismology is a powerful tool for probing the internal structures of stars by using their natural pulsation frequencies. It relies on identifying sequences of pulsation modes that can be compared with theoretical models, which has been done suc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e200b3c71d6845089388b59f6eb7653a
Autor:
Wei Zhang, Howard Isaacson, Kaiming Cui, Junbo Zhang, Hailong Yuan, Xiangqun Cui, Jujia Zhang, Wei-Min Gu, Lan Zhang, Zexi Niu, Haotong Zhang, Alexander Heger, Yilun Wang, Rosanne Di Stefano, Stephen Justham, Krzysztof Belczynski, Junfeng Wang, Yongheng Zhao, Xiang-Dong Li, Gang Zhao, Xiaoyong Mu, Rongfeng Shen, Lijing Shao, Zheng Zheng, Jianfeng Wu, Jorge Casares, Romano L. M. Corradi, Roberto Soria, Mario G. Lattanzi, Wei Wang, Qing-Zhong Liu, Huijuan Wang, Youjun Lu, Joel N. Bregman, Yu Bai, Zhanwen Han, Tianmeng Zhang, Zhaoxiang Qi, Tinggui Wang, Xiao-Feng Wang, Antonio Cabrera-Lavers, Xiaoli Wang, Yong Shao, Rafael Rebolo, Jifeng Liu, Chuanjie Zheng, Andrew W. Howard, Zhong-Rui Bai, Qing Gao, Ya-Juan Lei, Song Wang, Juanjuan Ren, Yaoquan Chu, Yi-Qiao Dong, Shilong Liao
Publikováno v:
Nature, 575(7784), 618-621. Nature Publishing Group
All stellar mass black holes have hitherto been identified by X-rays emitted by gas that is accreting onto the black hole from a companion star. These systems are all binaries with black holes below 30 M$_{\odot}$$^{1-4}$. Theory predicts, however, t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0259e769e3a394bb263b463b06fa3db6
https://dare.uva.nl/personal/pure/en/publications/a-wide-starblackhole-binary-system-from-radialvelocity-measurements(544605e5-63c8-40eb-99ba-aa36849c9587).html
https://dare.uva.nl/personal/pure/en/publications/a-wide-starblackhole-binary-system-from-radialvelocity-measurements(544605e5-63c8-40eb-99ba-aa36849c9587).html
Autor:
David R. Ciardi, Ann Marie Cody, Scott A. Barenfeld, Ian J. M. Crossfield, Andrew W. Howard, Erik A. Petigura, Howard Isaacson, Charles Beichman, Lynne A. Hillenbrand, Sasha Hinkley, Trevor J. David, John M. Carpenter, Joshua E. Schlieder
Publikováno v:
Nature. 534:658-661
Theories of the formation and early evolution of planetary systems postulate that planets are born in circumstellar disks, and undergo radial migration during and after dissipation of the dust and gas disk from which they formed. The precise ages of
Autor:
Elliott P. Horch, Steve B. Howell, Eric B. Ford, Jeffrey L. Coughlin, Christopher E. Henze, Stephen R. Kane, Jack J. Lissauer, Thomas Barclay, David R. Ciardi, Martin Still, Fred C. Adams, Mark E. Everett, Emeline Bolmont, Sean N. Raymond, Justin R. Crepp, Daniel Huber, Jason F. Rowe, Billy Quarles, Howard Isaacson, Elisa V. Quintana, Douglas A. Caldwell, Roger C. Hunter, Franck Selsis
Publikováno v:
Science
Science, American Association for the Advancement of Science, 2014, 344 (6181), pp.277-280. ⟨10.1126/science.1249403⟩
Science, American Association for the Advancement of Science, 2014, 344 (6181), pp.277-280. ⟨10.1126/science.1249403⟩
The quest for Earth-like planets represents a major focus of current exoplanet research. While planets that are Earth-sized and smaller have been detected, these planets reside in orbits that are too close to their host star to allow liquid water on
Autor:
Elliott P. Horch, Jon M. Jenkins, Leslie A. Rogers, Jason F. Rowe, David W. Latham, Søren Meibom, Sydney A. Barnes, Christopher E. Henze, Guillermo Torres, David R. Ciardi, Geoffrey W. Marcy, Francois Fressin, Justin R. Crepp, Kenneth A. Janes, S. T. Bryson, Steve B. Howell, Howard Isaacson, Debra A. Fischer, Simon C. Schuler
Publikováno v:
Nature. 499:55-58
Most stars and their planets form in open clusters. Over 95 per cent of such clusters have stellar densities too low (less than a hundred stars per cubic parsec) to withstand internal and external dynamical stresses and fall apart within a few hundre
Autor:
Mark E. Everett, Peter Tenenbaum, Laurance R. Doyle, Andrea K. Dupree, Jonathan J. Fortney, Rea Kolbl, Jessie L. Christiansen, William F. Welsh, Susan E. Thompson, Jean-Michel Desert, Geoffrey W. Marcy, Martin Still, Stephen T. Bryson, Daniel C. Fabrycky, Debra A. Fischer, David Charbonneau, Elisa V. Quintana, John C. Geary, Guillermo Torres, Thomas N. Gautier, David W. Latham, Eric B. Ford, Shawn Seader, Douglas A. Caldwell, Jason F. Rowe, Erik Brugamyer, Joseph D. Twicken, Michael R. Haas, Avi Shporer, Jason H. Steffen, Fergal Mullally, Francois Fressin, Justin R. Crepp, Andrew W. Howard, Jeffery J. Kolodziejczak, Andrej Prsa, Eric D. Lopez, Christopher J. Burke, Hans Kjeldsen, Michael Endl, Eric Agol, Fabienne A. Bastien, Lars A. Buchhave, Jerome A. Orosz, Lisa Kaltenegger, Natalie M. Batalha, Alan Gould, David R. Ciardi, Jrøgen Christensen-Dalsgaard, Jon M. Jenkins, Alan P. Boss, Steve B. Howell, Brian Lee, Edna DeVore, William D. Cochran, Howard Isaacson, William J. Borucki, J. A. Carter, Joshua N. Winn, Dimitar Sasselov, Roberto Sanchis-Ojeda, Jack J. Lissauer, Thomas Barclay, Christopher E. Henze, Daniel Huber
Publikováno v:
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, C, 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, Sanchis-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 2013, ' Kepler-62 : A five-planet system with planets of 1.4 and 1.6 Earth radii in the habitable zone ', Science, vol. 340, no. 6132, pp. 587-590 . https://doi.org/10.1126/science.1234702
arXiv
arXiv
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 (R[subscript ⊕]), orbiting a K2V star at periods of 5.7, 12.4, 18.2, 122.4, and 267.3 days, respectively. The outermost plan
Autor:
Steve B. Howell, Joshua A. Carter, Jonathan J. Fortney, William D. Cochran, Daniel C. Fabrycky, Samuel N. Quinn, Guillermo Torres, Donald R. Short, Michael R. Haas, Howard Isaacson, Eric B. Ford, Erik Brugamyer, Elisa V. Quintana, Paul Robertson, Andrej Prsa, Michael Endl, Jerome A. Orosz, Natalie M. Batalha, David R. Ciardi, Tsevi Mazeh, Douglas A. Caldwell, Lars A. Buchhave, William J. Borucki, David W. Latham, Thomas N. Gautier, Ronald L. Gilliland, Jack J. Lissauer, Laurance R. Doyle, Avi Shporer, William F. Welsh, Todd C. Klaus, Caroline Caldwell, Darin Ragozzine, Jie Li, Matthew J. Holman, David G. Koch, Thomas Barclay, Gur Windmiller, Steven Bloemen, Jon M. Jenkins, Jessie L. Christiansen, Geoffrey W. Marcy, Andrew W. Howard, Jason H. Steffen, Joshua N. Winn, Jennifer R. Hall
Publikováno v:
Nature. 481:475-479
Most Sun-like stars in the Galaxy reside in gravitationally bound pairs of stars (binaries). Although long anticipated, the existence of a 'circumbinary planet' orbiting such a pair of normal stars was not definitively established until the discovery
Autor:
Howard Isaacson, Daniel C. Fabrycky, S. M. Mills, Eric B. Ford, Erik A. Petigura, Cezary Migaszewski
Publikováno v:
Nature. 533(7604)
Surveys have revealed many multi-planet systems containing super-Earths and Neptunes in orbits of a few days to a few months. There is debate whether in situ assembly or inward migration is the dominant mechanism of the formation of such planetary sy
Autor:
William D. Cochran, Martin Bizzarro, Dimitar Sasselov, David W. Latham, Geoffrey W. Marcy, Lars A. Buchhave, Michael Endl, Diana Juncher, Howard Isaacson
Publikováno v:
Nature, vol 509, iss 7502
Approximately half of the extrasolar planets (exoplanets) with radii less than four Earth radii are in orbits with short periods. Despite their sheer abundance, the compositions of such planets are largely unknown. The available evidence suggests tha