Zobrazeno 1 - 10
of 44
pro vyhledávání: '"Howard Isaacson"'
Autor:
Teo Mocnik, Daniel Huber, Howard Isaacson, Stephen R. Kane, S. Giacalone, Lee J. Rosenthal, Paul A. Dalba, Douglas A. Caldwell, Michelle L. Hill, Nicholas Scarsdale, Roland Vanderspek, Martti H. Kristiansen, Jon M. Jenkins, Andrew W. Mayo, Edward H. Morgan, Benjamin J. Fulton, Andrew W. Howard, Andrew W. Mann, Arpita Roy, Ashley Chontos, Samuel N. Quinn, Ryan A. Rubenzahl, George R. Ricker, David Charbonneau, Paul Robertson, Courtney D. Dressing, J. Lubin, Ian Crossfield, Fei Dai, Joseph M. Akana Murphy, Simon Albrecht, Aida Behmard, Jeffrey C. Smith, Erik A. Petigura, Natalie M. Batalha, Mark E. Rose, Lea A. Hirsch, Tansu Daylan, Sara Seager, Maximilian N. Günther, David W. Latham, Corey Beard, Judah Van Zandt, Joshua N. Winn, Molly R. Kosiarek, Lauren M. Weiss
Publikováno v:
Dai, F, Roy, A, Fulton, B, Robertson, P, Hirsch, L, Isaacson, H, Albrecht, S, Mann, A W, Kristiansen, M H, Batalha, N M, Beard, C, Behmard, A, Chontos, A, Crossfield, I J M, Dalba, P A, Dressing, C, Giacalone, S, Hill, M, Howard, A W, Huber, D, Kane, S R, Kosiarek, M, Lubin, J, Mayo, A, Mocnik, T, Akana Murphy, J M, Petigura, E A, Rosenthal, L, Rubenzahl, R A, Scarsdale, N, Weiss, L M, van Zandt, J, Ricker, G R, Vanderspek, R, Latham, D W, Seager, S, Winn, J N, Jenkins, J M, Caldwell, D A, Charbonneau, D, Daylan, T, Günther, M N, Morgan, E, Quinn, S N, Rose, M E & Smith, J C 2020, ' The TESS-keck survey. III : A stellar obliquity measurement of TOI-1726 c ', Astronomical Journal, vol. 160, no. 4, abb3bd . https://doi.org/10.3847/1538-3881/abb3bd
Dai, F, Roy, A, Fulton, B, Robertson, P, Hirsch, L, Isaacson, H, Albrecht, S, Mann, A W, Kristiansen, M H, Beard, C, Behmard, A, Chontos, A, Crossfield, I J M, Dalba, P A, Dressing, C, Giacalone, S, Hill, M, Howard, A W, Huber, D, Kane, S R, Kosiarek, M, Lubin, J, Mayo, A, Mocnik, T, Akana Murphy, J M, Petigura, E A, Rosenthal, L, Rubenzahl, R A, Scarsdale, N, Weiss, L M, Zandt, J V, Ricker, G R, Vanderspek, R, Latham, D W, Seager, S, Winn, J N, Jenkins, J M, Caldwell, D A, Charbonneau, D, Daylan, T, Günther, M N, Morgan, E, Quinn, S N, Rose, M E & Smith, J C 2020, ' The TESS-Keck Survey. III. A Stellar Obliquity Measurement of TOI-1726 c ', Astrophysical Journal, vol. 160, no. 4, 193 . https://doi.org/10.3847/1538-3881/abb3bd
Dai, F, Roy, A, Fulton, B, Robertson, P, Hirsch, L, Isaacson, H, Albrecht, S, Mann, A W, Kristiansen, M H, Beard, C, Behmard, A, Chontos, A, Crossfield, I J M, Dalba, P A, Dressing, C, Giacalone, S, Hill, M, Howard, A W, Huber, D, Kane, S R, Kosiarek, M, Lubin, J, Mayo, A, Mocnik, T, Akana Murphy, J M, Petigura, E A, Rosenthal, L, Rubenzahl, R A, Scarsdale, N, Weiss, L M, Zandt, J V, Ricker, G R, Vanderspek, R, Latham, D W, Seager, S, Winn, J N, Jenkins, J M, Caldwell, D A, Charbonneau, D, Daylan, T, Günther, M N, Morgan, E, Quinn, S N, Rose, M E & Smith, J C 2020, ' The TESS-Keck Survey. III. A Stellar Obliquity Measurement of TOI-1726 c ', Astrophysical Journal, vol. 160, no. 4, 193 . https://doi.org/10.3847/1538-3881/abb3bd
We report the measurement of a spectroscopic transit of TOI-1726c, one of two planets transiting a G-type star with V = 6.9 in the Ursa Major Moving Group (∼400 Myr). With a precise age constraint from cluster membership, TOI-1726 provides a great
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::aa0cfdcff3dbb54f4a230f960242ff3c
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:
Courtney D. Dressing, Daniel Huber, Steven Giacalone, Ryan A. Rubenzahl, Stephen R. Kane, Howard Isaacson, Ian J. M. Crossfield, Arpita Roy, Natalie M. Batalha, Ashley Chontos, Paul Robertson, Lee J. Rosenthal, Nicholas Scarsdale, Erik A. Petigura, Andrew W. Mayo, Andrew W. Howard, Lauren M. Weiss, Teo Mocnik, Corey Beard, Jack Lubin, Fei Dai, Benjamin J. Fulton, Michelle L. Hill, Joseph M. Akana Murphy
Publikováno v:
The Astronomical Journal. 161:119
We measured the Rossiter-McLaughlin effect of WASP-107b during a single transit with Keck/HIRES. We found the sky-projected inclination of WASP-107b's orbit, relative to its host star's rotation axis, to be $|\lambda| = {118}^{+38}_{-19}$ degrees. Th
Autor:
Edward W. Schwieterman, Andrew W. Howard, Andrew Vanderburg, Steven Giacalone, Paul A. Dalba, Jason D. Eastman, Stephen R. Kane, Adam L. Kraus, Joseph E. Rodriguez, Howard Isaacson, Trent J. Dupuy, Lauren M. Weiss
Publikováno v:
The Astronomical Journal. 161:103
Despite the severe bias of the transit method of exoplanet discovery toward short orbital periods, a modest sample of transiting exoplanets with orbital periods greater than 100 days is known. Long-term radial velocity (RV) surveys are pivotal to con
Tidal forces in eccentric binary stars known as heartbeat stars excite detectable oscillations that shed light on the processes of tidal synchronization and circularization. We examine the pulsation phases of tidally excited oscillations (TEOs) in he
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::26afc65662b1e22d450c4b465eb46593
Autor:
E. O. Cadena Zepeda, David Barrado, Howard Isaacson, Daniel Huber, R. Petrucci, Paul Robertson, Abderahmane Soubkiou, Alan M. Watson, Allyson Bieryla, Prajwal Niraula, Karen A. Collins, Kevin Heng, V. Maigne, Lionel Garcia, Maria Morales-Calderon, Joshua N. Winn, Z. Essack, Amaury H. M. J. Triaud, G. Guisa, James McCormac, Brice-Olivier Demory, David W. Latham, Courtney D. Dressing, Arjun B. Savel, Khalid Barkaoui, Roberto Zambelli, J. D. Twicken, E. E. Lugo-Ibarra, Jon M. Jenkins, Mourad Ghachoui, Juan C. Suárez, Steven Giacalone, Jorge Lillo-Box, Y. Gómez Maqueo Chew, Marko Sestovic, George R. Ricker, Stephen R. Kane, L. Figueroa, U. Schroffenegger, Andrew Vanderburg, J. A. Franco Herrera, J. Haldemann, Lauren M. Weiss, Willy Benz, Simon L. Grimm, Arpita Roy, Brett M. Morris, Laurence Sabin, Leticia Carigi, Keivan G. Stassun, Didier Queloz, E. Colorado, Chelsea X. Huang, Fei Dai, P. Guerra, Christoph Mordasini, Zouhair Benkhaldoun, Benjamin V. Rackham, J. de Wit, G. Srdoc, Jack J. Lissauer, Francisco J. Pozuelos, Emmanuel Jehin, Sara Seager, Artem Burdanov, E. Jofre, Michaël Gillon, Ashley Chontos, T. Calvario-Velasquez, François Bouchy, G. Sierra Diaz, J. Herrera, Natalie M. Batalha
Publikováno v:
Digibug: Repositorio Institucional de la Universidad de Granada
Universidad de Granada (UGR)
Digital.CSIC. Repositorio Institucional del CSIC
instname
Digibug. Repositorio Institucional de la Universidad de Granada
Consejo Superior de Investigaciones Científicas (CSIC)
Universidad de Granada (UGR)
Digital.CSIC. Repositorio Institucional del CSIC
instname
Digibug. Repositorio Institucional de la Universidad de Granada
Consejo Superior de Investigaciones Científicas (CSIC)
We report the discovery and characterisation of a super-Earth and a sub-Neptune transiting the bright (K = 8:8), quiet, and nearby (37 pc) M3V dwarf TOI-1266. We validate the planetary nature of TOI-1266 b and c using four sectors of TESS photometry
Autor:
Howard Isaacson, Matthew J. Payne, Eric B. Ford, Seth Pritchard, Paul Robertson, Katherine M. Deck, Jason T. Wright, Benjamin E. Nelson
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 455:2484-2499
We report constraints on the three-dimensional orbital architecture for all four planets known to orbit the nearby M dwarf Gliese 876 based solely on Doppler measurements and demanding long-term orbital stability. Our dataset incorporates publicly av
Autor:
Molly R. Kosiarek, Lea A. Hirsch, Andrew W. Howard, Samuel W. Yee, Lauren M. Weiss, Heather Knutson, Benjamin J. Fulton, Erik A. Petigura, Gáspár Á. Bakos, Konstantin Batygin, Howard Isaacson, Joel D. Hartman, Evan Sinukoff
Publikováno v:
BASE-Bielefeld Academic Search Engine
HAT-P-11 is a mid-K dwarf that hosts one of the first Neptune-sized planets found outside the solar system. The orbit of HAT-P-11b is misaligned with the star's spin --- one of the few known cases of a misaligned planet orbiting a star less massive t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::05d31d24eb8428e9c8d3dcbbb08825e6
https://resolver.caltech.edu/CaltechAUTHORS:20180525-092851253
https://resolver.caltech.edu/CaltechAUTHORS:20180525-092851253
Autor:
Howard Isaacson, John M. Brewer, Gregory Laughlin, Songhu Wang, Debra A. Fischer, Brett C. Addison, Andrew W. Howard
We present spectroscopic measurements of the Rossiter-McLaughlin effect for the planet b of Kepler-9 multi-transiting planet system. The resulting sky-projected spin-orbit angle is $\lambda=-13^{\circ} \pm 16^{\circ}$, which favors an aligned system
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0eacdcffc3d1c630dd4229af3727741f
https://resolver.caltech.edu/CaltechAUTHORS:20180118-145948077
https://resolver.caltech.edu/CaltechAUTHORS:20180118-145948077
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