Zobrazeno 1 - 10
of 27
pro vyhledávání: '"Howard Isaacson"'
Autor:
Stephen R. Kane, Tiago L. Campante, Ekrem Murat Esmer, Rodrigo F. Díaz, Özgür Baştürk, Magali Deleuil, Stéphane Udry, Natalie R. Hinkel, Howard Isaacson, Simon J. O'Toole, Brad D. Carter, Maxime Marmier, Damien Ségransan, Margaret C. Turnbull, R. Paul Butler, H. P. Osborn, Jason T. Wright, Francesco Pepe, Christophe Lovis, Andrew W. Howard, Xavier Dumusque, Jon M. Jenkins, François Bouchy, Sara Seager, Jeremy Bailey, Robert A. Wittenmyer, Andrew Vanderburg, Geoffrey W. Marcy, Joshua N. Winn, Duncan J. Wright, Roland Vanderspek, Martti H. Kristiansen, Louise D. Nielsen, Darin Ragozzine, Hugh R. A. Jones, Jacob L. Bean, David Ehrenreich, Tansu Daylan, Selçuk Yalçınkaya, George R. Ricker, C. G. Tinney, Romain Allart, David W. Latham, Jonathan Horner, Colby Ostberg, Tara Fetherolf, Paul A. Dalba, Teo Mocnik
Publikováno v:
The Astronomical Journal
The Astronomical Journal, 2020, 160, ⟨10.3847/1538-3881/aba835⟩
Kane, S R, Yalçinkaya, S, Osborn, H P, Dalba, P A, Nielsen, L D, Vanderburg, A, Močnik, T, Hinkel, N R, Ostberg, C, Esmer, E M, Udry, S, Fetherolf, T, Baştürk, Ö, Ricker, G R, Vanderspek, R, Latham, D W, Seager, S, Winn, J N, Jenkins, J M, Allart, R, Bailey, J, Bean, J L, Bouchy, F, Butler, R P, Campante, T L, Carter, B D, Daylan, T, Deleuil, M, Diaz, R F, Dumusque, X, Ehrenreich, D, Horner, J, Howard, A W, Isaacson, H, Jones, H R A, Kristiansen, M H, Lovis, C, Marcy, G W, Marmier, M, O'Toole, S J, Pepe, F, Ragozzine, D, Ségransan, D, Tinney, C G, Turnbull, M C, Wittenmyer, R A, Wright, D J & Wright, J T 2020, ' Transits of Known Planets Orbiting a Naked-eye Star ', Astrophysical Journal, vol. 160, no. 3, 129 . https://doi.org/10.3847/1538-3881/aba835
The Astronomical Journal, 2020, 160, ⟨10.3847/1538-3881/aba835⟩
Kane, S R, Yalçinkaya, S, Osborn, H P, Dalba, P A, Nielsen, L D, Vanderburg, A, Močnik, T, Hinkel, N R, Ostberg, C, Esmer, E M, Udry, S, Fetherolf, T, Baştürk, Ö, Ricker, G R, Vanderspek, R, Latham, D W, Seager, S, Winn, J N, Jenkins, J M, Allart, R, Bailey, J, Bean, J L, Bouchy, F, Butler, R P, Campante, T L, Carter, B D, Daylan, T, Deleuil, M, Diaz, R F, Dumusque, X, Ehrenreich, D, Horner, J, Howard, A W, Isaacson, H, Jones, H R A, Kristiansen, M H, Lovis, C, Marcy, G W, Marmier, M, O'Toole, S J, Pepe, F, Ragozzine, D, Ségransan, D, Tinney, C G, Turnbull, M C, Wittenmyer, R A, Wright, D J & Wright, J T 2020, ' Transits of Known Planets Orbiting a Naked-eye Star ', Astrophysical Journal, vol. 160, no. 3, 129 . https://doi.org/10.3847/1538-3881/aba835
Some of the most scientifically valuable transiting planets are those that were already known from radial velocity (RV) surveys. This is primarily because their orbits are well characterized and they preferentially orbit bright stars that are the tar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d108bbb329b643ec5447b3619391ebac
https://hal-insu.archives-ouvertes.fr/insu-03667072
https://hal-insu.archives-ouvertes.fr/insu-03667072
Autor:
Adam L. Kraus, Nicholas J. Scott, Jonathan Irwin, Jennifer Burt, Nicholas Mehrle, David W. Latham, Elisabeth Matthews, Joshua E. Schlieder, David Berardo, Joshua N. Winn, Karen A. Collins, Samuel Halverson, Chelsea X. Huang, Kristo Ment, Stephen R. Kane, Masayuki Kuzuhara, Ian J. M. Crossfield, Teruyuki Hirano, William Waalkes, Elisa V. Quintana, Jennifer G. Winters, Diana Dragomir, Takayuki Kotani, Daniel Huber, Noriharu Watanabe, Motohide Tamura, Erica J. Gonzales, Mark E. Everett, Ashley Chontos, Rachel A. Matson, David Charbonneau, Erik A. Petigura, Knicole D. Colón, Thomas Mikal-Evans, Paul A. Dalba, Douglas A. Caldwell, Björn Benneke, Joseph D. Twicken, Norio Narita, Howard Isaacson, Trent J. Dupuy, Molly R. Kosiarek, George R. Ricker, Merrin Peterson, Bárbara Rojas-Ayala, Andrew W. Howard, Courtney D. Dressing, Jon M. Jenkins, Sébastien Lépine, Benjamin J. Fulton, Steve B. Howell, Elisabeth R. Newton, Zachory K. Berta-Thompson, Veselin B. Kostov, Philip S. Muirhead, Sara Seager, Yasunori Hori, Aaron C. Rizzuto, Mark E. Rose, Teo Mocnik
Planets occur most frequently around cool dwarfs, but only a handful of specific examples are known to orbit the latest-type M stars. Using TESS photometry, we report the discovery of two planets transiting the low-mass star called LP 791-18 (identif
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::33bf86ef48d308ef1f9c2a55887fdf95
https://resolver.caltech.edu/CaltechAUTHORS:20190722-131718080
https://resolver.caltech.edu/CaltechAUTHORS:20190722-131718080
Autor:
Howard Isaacson, Makennah Bristow, Benjamin J. Fulton, Allyson Bieryla, Lynne A. Hillenbrand, Chas Beichman, Luisa Rebull, Ian J. M. Crossfield, Andrew W. Howard, David W. Latham, Marie Ygouf, Lea A. Hirsch, Eric E. Mamajek, Joshua E. Schlieder, Andrew Vanderburg, Erik A. Petigura, Erica J. Gonzales, David R. Ciardi, John R. Stauffer, Trevor J. David, Ann Marie Cody, Gautam Vasisht
The role of stellar age in the measured properties and occurrence rates of exoplanets is not well understood. This is in part due to a paucity of known young planets and the uncertainties in age-dating for most exoplanet host stars. Exoplanets with w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a9d8c40fccb7ca104a7c1e3178a9e150
https://resolver.caltech.edu/CaltechAUTHORS:20180817-160130573
https://resolver.caltech.edu/CaltechAUTHORS:20180817-160130573
Autor:
Simon Albrecht, Kento Masuda, Molly R. Kosiarek, Erik A. Petigura, Joshua N. Winn, Howard Isaacson, Andrew W. Howard, Emma M. Louden
Publikováno v:
Louden, E M, Winn, J N, Petigura, E A, Isaacson, H, Howard, A W, Masuda, K, Albrecht, S & Kosiarek, M R 2021, ' Hot stars with kepler planets have high obliquities ', Astronomical Journal, vol. 161, no. 2, 68 . https://doi.org/10.3847/1538-3881/abcebd
It has been known for a decade that hot stars with hot Jupiters tend to have high obliquities. Less is known about the degree of spin-orbit alignment for hot stars with other kinds of planets. Here, we re-assess the obliquities of hot Kepler stars wi
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:
Howard Isaacson, Stephen R. Kane, Margaret C. Turnbull, Andrew W. Howard, Benjamin J. Fulton, Geoffrey W. Marcy, Lee J. Rosenthal, Lauren M. Weiss
Publikováno v:
The Astronomical Journal. 160:81
Uncovering the occurrence rate of terrestrial planets within the Habitable Zone (HZ) of their host stars has been a particular focus of exoplanetary science in recent years. The statistics of these occurrence rates have largely been derived from tran
Autor:
George R. Ricker, Jon M. Jenkins, Songhu Wang, Benjamin J. Fulton, David W. Latham, Hodari-Sadiki James, Matias I. Jones, Rafael Brahm, Keduse Worku, Jessie L. Christiansen, Howard Isaacson, Allen B. Davis, Bryndis Cruz, Eric B. Ting, Florian Rodler, Martin Paegert, Patricia T. Boyd, Todd J. Henry, Gábor Fűrész, Xian-Yu Wang, Seth Redfield, John M. Brewer, Martin Kürster, Sabine Reffert, Erik A. Petigura, A. M. Levine, Samuel N. Quinn, Timothy M. Brown, Gregory Laughlin, Sara Seager, Brett C. Addison, Maximilian N. Günther, L. A. Paredes, Robert J. Siverd, Sarah Millholland, En-Si Liang, Trifon Trifonov, Tsevi Mazeh, Keivan G. Stassun, René Tronsgaard, Christopher E. Henze, David R. Ciardi, Olga V. Zakhozhay, Avi Shporer, Gilbert A. Esquerdo, Allyson Bieryla, Karen A. Collins, Laura Kreidberg, Darryl Seligman, Andrew W. Howard, Jason D. Eastman, Sahar Shahaf, Michael Vezie, Roland Vanderspek, Debra A. Fischer, Joshua N. Winn, Hui Zhang, Charles Beichman, Chelsea X. Huang, Diana Kossakowski, Robert L. Morris
Publikováno v:
The Astronomical Journal, vol 157, iss 2
The Astronomical Journal
Wang, S, Jones, M, Shporer, A, Fulton, B J, Paredes, L A, Trifonov, T, Kossakowski, D, Eastman, J, Redfield, S, Günther, M N, Kreidberg, L, Huang, C X, Millholland, S, Seligman, D, Fischer, D, Brahm, R, Wang, X-Y, Cruz, B, Henry, T, James, H-S, Addison, B, Liang, E-S, Davis, A B, Tronsgaard, R, Worku, K, Brewer, J M, Kürster, M, Zhang, H, Beichman, C A, Bieryla, A, Brown, T M, Christiansen, J L, Ciardi, D R, Collins, K A, Esquerdo, G A, Howard, A W, Isaacson, H, Latham, D W, Mazeh, T, Petigura, E A, Quinn, S N, Shahaf, S, Siverd, R J, Rodler, F, Reffert, S, Zakhozhay, O, Ricker, G R, Vanderspek, R, Seager, S, Winn, J N, Jenkins, J M, T. Boyd, P, Fűrész, G, Henze, C, M. Levine, A, Morris, R, Paegert, M, G. Stassun, K, B. Ting, E, Vezie, M & Laughlin, G 2019, ' HD 202772A b: A Transiting Hot Jupiter around a Bright, Mildly Evolved Star in a Visual Binary Discovered by TESS ', Astrophysical Journal, vol. 157, no. 2, 51 . https://doi.org/10.3847/1538-3881/aaf1b7
The Astronomical Journal
Wang, S, Jones, M, Shporer, A, Fulton, B J, Paredes, L A, Trifonov, T, Kossakowski, D, Eastman, J, Redfield, S, Günther, M N, Kreidberg, L, Huang, C X, Millholland, S, Seligman, D, Fischer, D, Brahm, R, Wang, X-Y, Cruz, B, Henry, T, James, H-S, Addison, B, Liang, E-S, Davis, A B, Tronsgaard, R, Worku, K, Brewer, J M, Kürster, M, Zhang, H, Beichman, C A, Bieryla, A, Brown, T M, Christiansen, J L, Ciardi, D R, Collins, K A, Esquerdo, G A, Howard, A W, Isaacson, H, Latham, D W, Mazeh, T, Petigura, E A, Quinn, S N, Shahaf, S, Siverd, R J, Rodler, F, Reffert, S, Zakhozhay, O, Ricker, G R, Vanderspek, R, Seager, S, Winn, J N, Jenkins, J M, T. Boyd, P, Fűrész, G, Henze, C, M. Levine, A, Morris, R, Paegert, M, G. Stassun, K, B. Ting, E, Vezie, M & Laughlin, G 2019, ' HD 202772A b: A Transiting Hot Jupiter around a Bright, Mildly Evolved Star in a Visual Binary Discovered by TESS ', Astrophysical Journal, vol. 157, no. 2, 51 . https://doi.org/10.3847/1538-3881/aaf1b7
We report the first confirmation of a hot Jupiter discovered by the Transiting Exoplanet Survey Satellite (TESS) mission: HD 202772A b. The transit signal was detected in the data from TESS Sector 1, and was confirmed to be of planetary origin throug
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6399d0a2b1101463f67e7fcdd6d13938
Autor:
C. G. Tinney, Z. Csubry, Kaloyan Penev, S. Durkan, Paula Sarkis, Joel D. Hartman, Duncan J. Wright, Néstor Espinoza, Waqas Bhatti, Gáspár Á. Bakos, Istvan Papp, Rafael Brahm, G. W. Marcy, J. Lázár, Andrés Jordán, Th. Henning, Benjamin J. Fulton, Andrew W. Howard, Daniel Bayliss, M. de Val-Borro, Luigi Mancini, S. Ciceri, P. Sári, Vincent Suc, Markus Rabus, Howard Isaacson, J. Bento, Thiam-Guan Tan, George Zhou
Publikováno v:
The Astronomical Journal
We report the discovery of four close-in transiting exoplanets, HATS-50 through HATS-53, discovered using the HATSouth three-continent network of homogeneous and automated telescopes. These new exoplanets belong to the class of hot Jupiters and orbit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6b28a7dafa0912c4798afe1ed3a8b58b
http://hdl.handle.net/2108/204979
http://hdl.handle.net/2108/204979
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:
Travis Barman, Björn Benneke, Chad F. Bender, Alexandra C. Lockwood, John Asher Johnson, John S. Carr, Debra A. Fischer, Marta L. Bryan, Howard Isaacson, Nathan R. Crockett, Andrew W. Howard, Geoffrey A. Blake, Danielle Piskorz
We target the thermal emission spectrum of the non-transiting gas giant HD 88133 b with high-resolution near-infrared spectroscopy, by treating the planet and its host star as a spectroscopic binary. For sufficiently deep summed flux observations of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0880af17c5af548b1e6df20b12f945a8
https://resolver.caltech.edu/CaltechAUTHORS:20161123-092049528
https://resolver.caltech.edu/CaltechAUTHORS:20161123-092049528