Zobrazeno 1 - 10
of 154
pro vyhledávání: '"Stephen R. Kane"'
Autor:
Eric L. N. Jensen, Sara Seager, Brett C. Addison, Jack Okumura, Stephen R. Kane, Martin Paegert, Gavin Wang, J. Dittman, Guillermo Torres, David W. Latham, Thomas Barclay, Karen A. Collins, Laura Kreidberg, Sharon X. Wang, Matthew W. Mengel, Jeffrey C. Smith, Jonathan Horner, C. G. Tinney, Sarah Ballard, Keivan G. Stassun, Edward H. Morgan, John F. Kielkopf, Ian Crossfield, H. P. Osborn, Avi Shporer, Tianjun Gan, Roland Vanderspek, Hui Zhang, Nicholas M. Law, Shude Mao, Lorenzo Spina, Robert A. Wittenmyer, Peter Plavchan, Richard P. Schwarz, Cesar Briceno, C. Ziegler, Jacob L. Bean, Bernie Shiao, Joshua N. Winn, Jon M. Jenkins, Steve B. Howell, Coel Hellier, Daniel Foreman-Mackey, Andrew W. Mann, Megan Bedell, Brendan P. Bowler, Michael Vezie, Duncan J. Wright, George R. Ricker, Jorge Melendez, Joseph D. Twicken
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 507:2220-2240
We report the discovery and characterization of a transiting warm sub-Neptune planet around the nearby bright ($V=8.75$ mag, $K=7.15$ mag) solar twin HD 183579, delivered by the Transiting Exoplanet Survey Satellite (TESS). The host star is located $
Autor:
Stephen R. Kane, Cullen H. Blake, Robert A. Wittenmyer, Samson A. Johnson, David H. Sliski, Jason T. Wright, Audrey Houghton, Maurice Wilson, Mark R. Giovinazzi, Jonathan Horner, Nate McCrady, Joseph P. Glaser, John Asher Johnson, Peter Plavchan, Jason D. Eastman, Juliana Garcia-Mejia
Publikováno v:
Astronomische Nachrichten. 341:870-878
The hot Jupiter HD 217107 b was one of the first exoplanets detected using the radial velocity (RV) method, originally reported in the literature in 1999. Today, precise RV measurements of this system span more than 20 years, and there is clear evide
Autor:
Jack Lubin, Judah Van Zandt, Rae Holcomb, Lauren M. Weiss, Erik A Petigura, Paul Robertson, Joseph M. Akana Murphy, Nicholas Scarsdale, Konstantin Batygin, Alex S. Polanski, Natalie M. Batalha, Ian J. M. Crossfield, Courtney Dressing, Benjamin Fulton, Andrew W. Howard, Daniel Huber, Howard Isaacson, Stephen R. Kane, Arpita Roy, Corey Beard, Sarah Blunt, Ashley Chontos, Fei Dai, Paul A. Dalba, Kaz Gary, Steven Giacalone, Michelle L. Hill, Andrew Mayo, Teo Močnik, Molly R. Kosiarek, Malena Rice, Ryan A. Rubenzahl, David W. Latham, S. Seager, Joshua N. Winn
Exoplanet systems with multiple transiting planets are natural laboratories for testing planetary astrophysics. One such system is HD 191939 (TOI-1339), a bright (V=9) and Sun-like (G9V) star, which TESS found to host three transiting planets (b, c,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fc6e0bee9b81790c21f626d4cc4a542e
https://resolver.caltech.edu/CaltechAUTHORS:20211018-185245786
https://resolver.caltech.edu/CaltechAUTHORS:20211018-185245786
Autor:
Andrew W. Mayo, Jorge Lillo-Box, George R. Ricker, C. Moutou, Stephen R. Kane, René Tronsgaard, Ashley Chontos, Allyson Bieryla, Karen A. Collins, Nicola Astudillo-Defru, Luc Arnold, Rafael Luque, Andrew W. Howard, Xavier Dumusque, S. G. Sousa, V. Bourrier, Erik Petigura, Joshua N. Winn, Magali Deleuil, Lauren M. Weiss, Enric Palle, Nuno C. Santos, Steven Giacalone, J. Rey, Damien Ségransan, Courtney D. Dressing, Paul A. Dalba, Arpita Roy, Jack Lubin, Sara Seager, Corey Beard, Natalie M. Batalha, Daniel Huber, C. E. Brasseur, T. Lopez, Howard Isaacson, Teo Mocnik, Jason D. Eastman, Peter Tenenbaum, N. Heidari, Michelle L. Hill, P. Cortés-Zuleta, O. Mousis, E. Delgado Mena, Diana Dragomir, D. W. Latham, François Bouchy, Aida Behmard, David Ehrenreich, P. A. Strøm, Fei Dai, F. Vakili, T. Forveille, Tansu Daylan, R. Vanderspek, Keivan G. Stassun, Alexandre Santerne, Melissa J. Hobson, X. Bonfils, Benjamin J. Fulton, G. Montagnier, M. Stalport, Francesco Pepe, Lars A. Buchhave, Flavien Kiefer, Nicholas Scarsdale, Lee J. Rosenthal, Vardan Adibekyan, Paul Robertson, Olivier Demangeon, J. M. Jenkins, A. Carmona, Nematollah Riazi, Stéphane Udry, Rodrigo F. Díaz, N. C. Hara, G. Gaisne, Thomas Barclay, Tara Fetherolf, X. Delfosse, L. Mignon, Sergio Hoyer, B. Courcol, J. Orell-Mique, S. Borgniet, Guillaume Hébrard, Ryan A. Rubenzahl, Lea A. Hirsch, S. Dalal, Ian J. M. Crossfield, Joseph M. Akana Murphy, L. Acuna, Isabelle Boisse
Publikováno v:
Heidari, N, Boisse, I, Orell-Miquel, J, Hébrard, G, Acuña, L, Hara, N C, Lillo-Box, J, Eastman, J D, Arnold, L, Astudillo-Defru, N, Adibekyan, V, Bieryla, A, Bonfils, X, Bouchy, F, Barclay, T, Brasseur, C E, Borgniet, S, Bourrier, V, Buchhave, L, Behmard, A, Beard, C, Batalha, N M, Courcol, B, Cortés-Zuleta, P, Collins, K, Carmona, A, Crossfield, I J M, Chontos, A, Delfosse, X, Dalal, S, Deleuil, M, Demangeon, O D S, Diáz, R F, Dumusque, X, Daylan, T, Dragomir, D, Delgado Mena, E, Dressing, C, Dai, F, Dalba, P A, Ehrenreich, D, Forveille, T, Fulton, B, Fetherolf, T, Gaisné, G, Giacalone, S, Riazi, N, Hoyer, S, Hobson, M J, Howard, A W, Huber, D, Hill, M L, Hirsch, L A, Isaacson, H, Jenkins, J, Kane, S R, Kiefer, F, Luque, R, Latham, D W, Lubin, J, Lopez, T, Mousis, O, Moutou, C, Montagnier, G, Mignon, L, Mayo, A, Močnik, T, Murphy, J M A, Palle, E, Pepe, F, Petigura, E A, Rey, J, Ricker, G, Robertson, P, Roy, A, Rubenzahl, R A, Rosenthal, L J, Santerne, A, Santos, N C, Sousa, S G, Stassun, K G, Stalport, M, Scarsdale, N, Strøm, P A, Seager, S, Segransan, D, Tenenbaum, P, Tronsgaard, R, Udry, S, Vanderspek, R, Vakili, F, Winn, J & Weiss, L M 2022, ' HD 207897 b : A dense sub-Neptune transiting a nearby and bright K-type star ', Astronomy and Astrophysics, vol. 658, A176 . https://doi.org/10.1051/0004-6361/202141429
aap
aap, 2022, 658, pp.A176. ⟨10.1051/0004-6361/20214142910.48550/arXiv.2110.08597⟩
A&A
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 658, pp.A176. ⟨10.1051/0004-6361/202141429⟩
aap
aap, 2022, 658, pp.A176. ⟨10.1051/0004-6361/20214142910.48550/arXiv.2110.08597⟩
A&A
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 658, pp.A176. ⟨10.1051/0004-6361/202141429⟩
We present the discovery and characterization of a transiting sub-Neptune orbiting with a 16.20 day period around a nearby (28 pc) and bright(V=8.37) K0V star HD207897 (TOI-1611). This discovery is based on photometric measurements from the Transitin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c45535bfbc2b44d80aa4ccfcf7e815bb
https://orbit.dtu.dk/en/publications/3d99a271-47b7-4a78-9949-fa7678314633
https://orbit.dtu.dk/en/publications/3d99a271-47b7-4a78-9949-fa7678314633
Autor:
Matias Diaz, Stephen R. Kane, Jose I. Vines, Mikko Tuomi, Diana Dragomir, Johanna Teske, Jeffrey D. Crane, Pamela Arriagada, M. G. Soto, Daniel Thorngren, Fabo Feng, James S. Jenkins, Stephen A. Shectman, Z. M. Berdinas, S. Villanueva, Sharon X. Wang, R. Paul Butler
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 496:4330-4341
We report the detection of a transiting, dense Neptune planet candidate orbiting the bright ($V=8.6$) K0.5V star HD 95338. Detection of the 55-day periodic signal comes from the analysis of precision radial velocities from the Planet Finder Spectrogr
Autor:
Enrico Corsaro, William J. Chaplin, James S. Kuszlewicz, Zhexing Li, Benjamin J. Fulton, S. N. Breton, Rafael A. García, Derek Buzasi, Tanda Li, Dennis Stello, J. M. Joel Ong, Timothy D. Brandt, Paul A. Dalba, Marc Hon, Savita Mathur, Keivan G. Stassun, Aldo Serenelli, Timothy R. White, Timothy R. Bedding, Margarida S. Cunha, Chen Jiang, Benjamin J. S. Pope, Daniel Huber, Cenk Kayhan, Michelle L. Hill, Stephen R. Kane, Tiago L. Campante, Diego Bossini
Publikováno v:
Hill, M L, Kane, S R, Campante, T L, Li, Z, Dalba, P A, Brandt, T D, White, T R, Pope, B J S, Stassun, K G, Fulton, B J, Corsaro, E, Li, T, Ong, J M J, Bedding, T R, Bossini, D, Buzasi, D L, Chaplin, W J, Cunha, M S, García, R A, Breton, S N, Hon, M, Huber, D, Jiang, C, Kayhan, C, Kuszlewicz, J S, Mathur, S, Serenelli, A & Stello, D 2021, ' Asteroseismology of iota Draconis and Discovery of an Additional Long-period Companion ', Astronomical Journal, vol. 162, no. 5, 211 . https://doi.org/10.3847/1538-3881/ac1b31
The Astronomical Journal
Digital.CSIC. Repositorio Institucional del CSIC
instname
The Astronomical Journal
Digital.CSIC. Repositorio Institucional del CSIC
instname
Hill, Michelle L., et al.
Giant stars as known exoplanet hosts are relatively rare due to the potential challenges in acquiring precision radial velocities and the small predicted transit depths. However, these giant host stars are also some of
Giant stars as known exoplanet hosts are relatively rare due to the potential challenges in acquiring precision radial velocities and the small predicted transit depths. However, these giant host stars are also some of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bcebdd18163113aea676a5a0dbc175c5
https://avesis.erciyes.edu.tr/publication/details/7e2fd1ff-4746-4eb6-9028-ba33af12ee78/oai
https://avesis.erciyes.edu.tr/publication/details/7e2fd1ff-4746-4eb6-9028-ba33af12ee78/oai
Autor:
Andrés Jordán, Sara Seager, Brett C. Addison, Maximilian N. Günther, Monika Lendl, Jack Okumura, Jorge Lillo-Box, Jon M. Jenkins, Roland Vanderspek, C. G. Tinney, Benjamin J. Fulton, Peter J. Wheatley, Erik A. Petigura, Beth A. Henderson, C. Stibbard, P. Figueira, Rafael Brahm, Eric L. N. Jensen, Michael Reefe, Cesar Briceno, Chris Stockdale, S. Hojjatpanah, Farisa Y. Morales, Alexis M. S. Smith, Caroline Dorn, Thomas Henning, Vardan Adibekyan, George W. King, Lauren M. Weiss, David R. Ciardi, Howard Isaacson, Richard P. Schwarz, Thomas Barclay, Stephen R. Kane, Keivan G. Stassun, David W. Latham, Malcolm Fridlund, Jack S. Acton, Ravit Helled, Sharon X. Wang, John Berberian, Joseph D. Twicken, J. F. Otegi, David R. Anderson, Sarah L. Casewell, Elise Furlan, Elisabeth Matthews, Johanna Teske, Rodrigo F. Díaz, Samuel Gill, Daniel Bayliss, Ian Crossfield, Peter Plavchan, Matthew W. Mengel, Joshua E. Schlieder, John F. Kielkopf, Stéphane Udry, E. Delgado Mena, H. P. Osborn, Avi Shporer, R. Cloutier, J. Villasenor, Duncan J. Wright, E. Gaidos, A. Osborn, K. I. Collins, Angelle Tanner, Nicholas M. Law, Björn Benneke, Joshua N. Winn, Fei Dai, Nicholas J. Scott, Erica J. Gonzales, Courtney D. Dressing, Sarah Ballard, Don Pollacco, Coel Hellier, Michael R. Goad, David J. Armstrong, Varoujan Gorjian, Paula Sarkis, Richard C. Kidwell, F. Zohrabi, Nuno C. Santos, David Barrado, Matthew R. Burleigh, Sergio Hoyer, Claire Geneser, Christopher J. Burke, Richard G. West, James McCormac, P. A. Strøm, Daniel Huber, Aleisha Hogan, Paul Robertson, Natalie M. Batalha, Edward M. Bryant, Liam Raynard, Karen A. Collins, Robert A. Wittenmyer, Mark E. Rose, Rachel A. Matson, Steve B. Howell, James S. Jenkins, Jose I. Vines, S. C. C. Barros, Néstor Espinoza, B. Cale, Andrew W. Howard, Diana Dragomir, Alexandre Santerne, M. Lund, Olivier Demangeon, Brendan P. Bowler, Benjamin F. Cooke, Xavier Dumusque, Andrew W. Mann, Hui Zhang, Carl Ziegler, Arpita Roy, Rosanna H. Tilbrook, Sérgio F. Sousa, George R. Ricker, Jonathan Horner, Elisa V. Quintana, Thiam-Guan Tan, Louise D. Nielsen, François Bouchy
Publikováno v:
Monthly Notices of the Royal Astronomical Society
MNRAS
MNRAS, 2021, 507 (2), pp.2782-2803. ⟨10.1093/mnras/stab2313⟩
Monthly Notices of the Royal Astronomical Society, 507(2), 2782-2803
MNRAS
MNRAS, 2021, 507 (2), pp.2782-2803. ⟨10.1093/mnras/stab2313⟩
Monthly Notices of the Royal Astronomical Society, 507(2), 2782-2803
We present the bright (V$_{mag} = 9.12$), multi-planet system TOI-431, characterised with photometry and radial velocities. We estimate the stellar rotation period to be $30.5 \pm 0.7$ days using archival photometry and radial velocities. TOI-431b is
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6e6466f6b97f9534884a0fbc2c4a2504
https://resolver.caltech.edu/CaltechAUTHORS:20211008-175558303
https://resolver.caltech.edu/CaltechAUTHORS:20211008-175558303
Autor:
Xavier Bonfils, Michael W. Werner, Nicola Astudillo-Defru, Jon M. Jenkins, George R. Ricker, Ian J. M. Crossfield, Eric L. N. Jensen, David R. Ciardi, Emmanuel Jehin, Judith Korth, David W. Latham, Farisa Y. Morales, Ismael Mireles, Keivan G. Stassun, Étienne Artigau, Rodrigo F. Díaz, J. Orell-Miquel, Pedro Figueira, Stéphane Udry, René Doyon, X. Delfosse, Jack J. Lissauer, Francesco Pepe, Damien Ségransan, Nuno C. Santos, Christophe Lovis, Peter Tenenbaum, Elisa V. Quintana, Björn Benneke, Rachel A. Matson, Jose-Manuel Almenara, Felipe Murgas, Douglas A. Caldwell, Kevin I. Collins, Phil Evans, C. E. Brasseur, Stephen R. Kane, François Bouchy, David Charbonneau, G. Morello, Roland Vanderspek, Charles Beichman, Elisabeth Matthews, T. Forveille, Khalid Barkaoui, Sara Seager, Diana Dragomir, Erica J. Gonzales, Robert F. Goeke, G. Gaisne, Joshua E. Schlieder, John H. Livingston, Natalia Guerrero, Claudio Melo, Alan M. Levine, Joshua N. Winn, Steve B. Howell, Michaël Gillon, Francisco J. Pozuelos, Jason D. Eastman, Varoujan Gorjian, Karen A. Collins
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 653, pp.A60. ⟨10.1051/0004-6361/202140718⟩
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 653, pp.A60. ⟨10.1051/0004-6361/202140718⟩
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
We use TESS, Spitzer, ground-based light curves and HARPS spectrograph radial velocity measurements to establish the physical properties of the transiting exoplanet candidate TOI-674b. We perform a joint fit of the light curves and radial velocity ti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1b8dbf299b512c0ec69e07c72bfbe688
https://hal-insu.archives-ouvertes.fr/insu-03458387/file/aa40718-21.pdf
https://hal-insu.archives-ouvertes.fr/insu-03458387/file/aa40718-21.pdf
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
Autor:
Gregory W. Henry, Lauren M. Weiss, Howard Isaacson, Ryan A. Rubenzahl, Cayla M. Dedrick, Ilya A. Sherstyuk, Heather A. Knutson, Geoffrey W. Marcy, Lea A. Hirsch, Ian J. M. Crossfield, Ashley Chontos, Stephen R. Kane, Lee J. Rosenthal, Paul A. Dalba, Debra A. Fischer, Aida Behmard, Molly R. Kosiarek, Jason T. Wright, Justin R. Crepp, Erik A. Petigura, Sarah Blunt, Benjamin J. Fulton, Andrew W. Howard
We present a high-precision radial velocity (RV) survey of 719 FGKM stars, which host 164 known exoplanets and 14 newly discovered or revised exoplanets and substellar companions. This catalog updated the orbital parameters of known exoplanets and lo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::76732e1729874d6acb5e099890ba773b
https://resolver.caltech.edu/CaltechAUTHORS:20210715-145459591
https://resolver.caltech.edu/CaltechAUTHORS:20210715-145459591