Zobrazeno 1 - 10
of 29
pro vyhledávání: '"Margaret C. Turnbull"'
Autor:
Margaret C. Turnbull, Stephen R. Kane, Zhexing Li, Julien Girard, S. R. Hildebrandt, Neil Zimmerman, Junellie Gonzalez-Quiles
Future direct imaging missions will primarily observe planets that have been previously detected, mostly via the radial velocity (RV) technique, to characterize planetary atmospheres. In the meantime, direct imaging may discover new planets within ex
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5716cf7ab14d2d764f6ef71a0632141f
https://resolver.caltech.edu/CaltechAUTHORS:20210610-100556900
https://resolver.caltech.edu/CaltechAUTHORS:20210610-100556900
Publikováno v:
The Astrophysical Journal. 933:62
A set of simulations with a 3D global climate model are performed to investigate the roles of obliquity and rotation period in the habitability of Earthlike exoplanets. The simulations cover the obliquity–rotation parameter space, from 0° to 90°
Starshade Imaging Simulation Toolkit for Exoplanet Reconnaissance (SISTER) is a versatile tool designed to provide accurate models of the images of exoplanet systems when observed with a starshade positioned to block the light from the host star. SIS
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b7bb6a16d31d26f60e44a67d329514f0
https://resolver.caltech.edu/CaltechAUTHORS:20210821-150837966
https://resolver.caltech.edu/CaltechAUTHORS:20210821-150837966
Autor:
Daniel Huber, Paul A. Dalba, Sara Seager, Tara Fetherolf, Margaret C. Turnbull, Stephen R. Kane, Tiago L. Campante, Colby Ostberg, William J. Chaplin, Joshua Pepper, Jacob L. Bean, George R. Ricker, Roland Vanderspek, Teo Mocnik, David W. Latham, Joshua N. Winn, Jon M. Jenkins, E. Simpson
Publikováno v:
Kane, S R, Bean, J L, Campante, T L, Dalba, P A, Fetherolf, T, Mocnik, T, Ostberg, C, Pepper, J, Simpson, E R, Turnbull, M C, Ricker, G R, Vanderspek, R, Latham, D W, Seager, S, Winn, J N, Jenkins, J M, Huber, D & Chaplin, W J 2021, ' Science extraction from TESS observations of known exoplanet hosts ', Publications of the Astronomical Society of the Pacific, vol. 133, no. 1019, 014402 . https://doi.org/10.1088/1538-3873/abc610
arXiv
arXiv
The transit method of exoplanet discovery and characterization has enabled numerous breakthroughs in exoplanetary science. These include measurements of planetary radii, mass-radius relationships, stellar obliquities, bulk density constraints on inte
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6e0400954bd9890b9c6f804099b0e503
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:
Filipe Pereira, S. G. Sousa, Daniel Huber, S. Stock, James S. Kuszlewicz, Marc Hon, Mário J. P. F. G. Monteiro, Stephen R. Kane, Rafael A. García, Vardan Adibekyan, Tiago L. Campante, Sabine Reffert, Dennis Stello, Zeynep Çelik Orhan, Guy R. Davies, Martin Bo Nielsen, Timothy R. Bedding, Mutlu Yildiz, Benard Nsamba, Jørgen Christensen-Dalsgaard, Elisa Delgado Mena, H. M. Antia, Sibel Örtel, Maria Tsantaki, Victor Silva Aguirre, Rasmus Handberg, Miles Lucas, Margarida S. Cunha, Sarbani Basu, Savita Mathur, Enrico Corsaro, Nicolas Nardetto, William J. Chaplin, Warrick H. Ball, Mathieu Vrard, Hans Kjeldsen, Jacob L. Bean, Travis S. Metcalfe, Benoit Mosser, Keivan G. Stassun, Aldo Serenelli, Steven D. Kawaler, Margaret C. Turnbull, Mikkel N. Lund, Marc H. Pinsonneault, Dimitri Veras, Andrea Miglio, Diego Bossini
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2019, 885 (1), pp.31. ⟨10.3847/1538-4357/ab44a8⟩
Campante, T L, Corsaro, E, Lund, M N, Mosser, B, Serenelli, A, Veras, D, Adibekyan, V, Antia, H M, Ball, W, Basu, S, Bedding, T R, Bossini, D, Davies, G R, Mena, E D, García, R A, Handberg, R, Hon, M, Kane, S R, Kawaler, S D, Kuszlewicz, J S, Lucas, M, Mathur, S, Nardetto, N, Nielsen, M B, Pinsonneault, M H, Reffert, S, Aguirre, V S, Stassun, K G, Stello, D, Stock, S, Vrard, M, Yildiz, M, Chaplin, W J, Huber, D, Bean, J L, Çelik Orhan, Z, Cunha, M S, Christensen-Dalsgaard, J, Kjeldsen, H, Metcalfe, T S, Miglio, A, Monteiro, M J P F G, Nsamba, B, Örtel, S, Pereira, F, Sousa, S G, Tsantaki, M & Turnbull, M C 2019, ' TESS Asteroseismology of the Known Red-giant Host Stars HD 212771 and HD 203949 ', Astrophysical Journal, vol. 885, no. 1, 31 . https://doi.org/10.3847/1538-4357/ab44a8
The Astrophysical Journal, 2019, 885 (1), pp.31. ⟨10.3847/1538-4357/ab44a8⟩
The Astrophysical Journal, American Astronomical Society, 2019, 885 (1), pp.31. ⟨10.3847/1538-4357/ab44a8⟩
Campante, T L, Corsaro, E, Lund, M N, Mosser, B, Serenelli, A, Veras, D, Adibekyan, V, Antia, H M, Ball, W, Basu, S, Bedding, T R, Bossini, D, Davies, G R, Mena, E D, García, R A, Handberg, R, Hon, M, Kane, S R, Kawaler, S D, Kuszlewicz, J S, Lucas, M, Mathur, S, Nardetto, N, Nielsen, M B, Pinsonneault, M H, Reffert, S, Aguirre, V S, Stassun, K G, Stello, D, Stock, S, Vrard, M, Yildiz, M, Chaplin, W J, Huber, D, Bean, J L, Çelik Orhan, Z, Cunha, M S, Christensen-Dalsgaard, J, Kjeldsen, H, Metcalfe, T S, Miglio, A, Monteiro, M J P F G, Nsamba, B, Örtel, S, Pereira, F, Sousa, S G, Tsantaki, M & Turnbull, M C 2019, ' TESS Asteroseismology of the Known Red-giant Host Stars HD 212771 and HD 203949 ', Astrophysical Journal, vol. 885, no. 1, 31 . https://doi.org/10.3847/1538-4357/ab44a8
The Astrophysical Journal, 2019, 885 (1), pp.31. ⟨10.3847/1538-4357/ab44a8⟩
Orhan, Zeynep Celik/0000-0002-9424-2339; Serenelli, Aldo/0000-0001-6359-2769; Monteiro, Mario J. P. F. G./0000-0003-0513-8116; Huber, Daniel/0000-0001-8832-4488; Adibekyan, Vardan/0000-0002-0601-6199; Reffert, Sabine/0000-0002-0460-8289; Stock, Steph
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ce47f685bd0523ed86f224b81a00582e
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:
Kerri Cahoy, Ewan S. Douglas, N. Jeremy Kasdin, Margaret C. Turnbull, Ashley Carlton, Bruce Macintosh
Publikováno v:
Modeling, Systems Engineering, and Project Management for Astronomy VIII.
The coronagraphic instrument (CGI) on the Wide-Field Infrared Survey Telescope (WFIRST) will demonstrate technologies and methods for high-contrast direct imaging and spectroscopy of exoplanet systems in reflected light, including polarimetry of circ
Autor:
Margaret C. Turnbull, Joshua Pepper, Paul A. Dalba, Stephen R. Kane, Tiago L. Campante, Thomas Barclay, Darin Ragozzine, Jacob L. Bean
Radial velocity (RV) surveys have detected hundreds of exoplanets through their gravitational interactions with their host stars. Some will be transiting, but most lack sufficient follow-up observations to confidently detect (or rule out) transits. W
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cf49805b7e5077d4f23699517a9fd859
Direct imaging of exoplanets presents both significant challenges and significant gains. The advantages primarily lie in receiving emitted and, with future instruments, reflected photons at phase angles not accessible by other techniques, enabling th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::316c1225afc4935575f5c64de32791b6