Zobrazeno 1 - 10
of 28
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:
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:
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:
David W. Latham, Rhodes Hart, Richard P. Schwarz, Matías R. Díaz, Ryan Cloutier, George Zhou, Matthew W. Mengel, Felipe Rojas, George R. Ricker, Jeffrey D. Crane, Andrés Jordán, Joshua N. Winn, Jennifer Burt, Thomas Henning, Lizhou Sha, Brett C. Addison, Erin Snoddy, Jonathan Horner, Eric L. N. Jensen, Jack Okumura, Rafael Brahm, Christopher E. Henze, Holger Drass, Norio Narita, Ian J. M. Crossfield, Benjamin T. Montet, Peter Plavchan, Michael Vezie, John H. Livingston, Hui Zhang, Roland Vanderspek, Keivan G. Stassun, Carl Ziegler, Allyson Bieryla, Karen A. Collins, David Nespral, Thiam-Guan Tan, Stephen R. Kane, Kaloyan Penev, Louise D. Nielsen, Steven Villanueva, Akshata Krishnamurthy, Luigi Mancini, Robert A. Wittenmyer, Joel D. Hartman, Eric B. Ting, Andrew Vanderburg, G. Ottoni, Johanna Teske, John F. Kielkopf, Sara Seager, Knicole D. Colón, Janis Hagelberg, Mauro Barbieri, A. Zapata, Duncan J. Wright, Chelsea X. Huang, François Bouchy, Stéphane Udry, Elisabeth Matthews, Andrew W. Mann, Paula Sarkis, Sharon X. Wang, Jon M. Jenkins, Diana Dragomir, Motohide Tamura, Pascal Torres, Gáspár Á. Bakos, Joseph E. Rodriguez, Daniel Bayliss, Avi Shporer, Néstor Espinoza, Adina D. Feinstein
We report the discovery of two short-period Saturn-mass planets, one transiting the G subgiant TOI-954 (TIC 44792534, $ V = 10.343 $, $ T = 9.78 $) observed in TESS sectors 4 and 5, and one transiting the G dwarf K2-329 (EPIC 246193072, $ V = 12.70 $
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::809d8342209eed9fc89e926d9f607a49
Autor:
William J. Chaplin, Sibel Örtel, Stephen R. Kane, Tiago L. Campante, Rafael A. García, Savita Mathur, Jakob Rørsted Mosumgaard, Joel Ong, Warrick H. Ball, B. Mosser, M. Deal, M. S. Cunha, Amalie Stokholm, Keivan G. Stassun, Ângela R. G. Santos, Sarbani Basu, Daniel Huber, Martin Bo Nielsen, Victor Silva Aguirre, Benard Nsamba, Derek Buzasi, Z. Çelik Orhan, L. González-Cuesta, Mutlu Yildiz
Publikováno v:
Ball, W H, Chaplin, W J, Nielsen, M B, González-Cuesta, L, Mathur, S, Santos, Â R G, García, R, Buzasi, D, Mosser, B, Deal, M, Stokholm, A, Mosumgaard, J R, Silva Aguirre, V, Nsamba, B, Campante, T, Cunha, M S, Ong, J, Basu, S, Örtel, S, Çelik Orhan, Z, Yıldız, M, Stassun, K, Kane, S R & Huber, D 2020, ' Robust asteroseismic properties of the bright planet host HD 38529 ', Monthly Notices of the Royal Astronomical Society, vol. 499, no. 4, pp. 6084-6093 . https://doi.org/10.1093/mnras/staa3190
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 499 (4), pp.6084-6093. ⟨10.1093/mnras/staa3190⟩
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2020, 499 (4), pp.6084-6093. ⟨10.1093/mnras/staa3190⟩
The Transiting Exoplanet Survey Satellite (TESS) is recording short-cadence, high duty-cycle timeseries across most of the sky, which presents the opportunity to detect and study oscillations in interesting stars, in particular planet hosts. We have
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7d3be976253369b27eda989be81db6e9
https://pure.au.dk/ws/files/206006105/2010.07323
https://pure.au.dk/ws/files/206006105/2010.07323
Autor:
Matthew A. Kenworthy, Russel J. White, Keivan G. Stassun, Jason J. Wang, John P. Doty, Andrew Cancino, Joshua Pepper, Sara Seager, Sharon X. Wang, David W. Latham, Bernie Walp, Daniel Foreman-Mackey, John F. Kielkopf, Perri Zilberman, Dax L. Feliz, Ben Tieu, Mark Clampin, Matthew W. Mengel, Frank Giddens, Denise Weigand, Joshua E. Schlieder, David Berardo, Jon M. Jenkins, Roland Vanderspek, Ian J. M. Crossfield, Thomas Barclay, Ryan Hall, Joshua N. Winn, Fred C. Adams, Guillem Anglada-Escudé, Andrew Vanderburg, Patrick J. Lowrance, Hui Zhang, Bertrand Mennesson, S. N. Quinn, Akshata Krishnamurthy, Karen A. Collins, Norio Narita, Robert A. Wittenmyer, Bryson Cale, Todd J. Henry, Natasha Latouf, Elise Furlan, Dennis Afanasev, Joseph Huber, Ethan Kruse, Elisabeth R. Newton, Cassy Davison, C. G. Tinney, Chas Beichman, Jack Okumura, Coel Hellier, Allison Youngblood, David M. Kipping, Aki Roberge, Andrew W. Howard, America Nishimoto, Kaspar von Braun, Stephen R. Kane, Diana Dragomir, Timothy D. Morton, Peter Plavchan, Brendan P. Bowler, Peter Gao, Angelle Tanner, Eric Gaidos, George R. Ricker, Veronica Roccatagliata, William Matzko, Enric Palle, Emily A. Gilbert, Jonathan Gagné, Stephen A. Rinehart, Jake T. Clark, Duncan J. Wright, Chelsea X. Huang, Sean M. Mills, Michael Bottom, David R. Ciardi, Carolyn Brinkworth, Johanna Teske, Chris Klenke, Scott Dynes, Claire Geneser, Jonathan Horner, Carolyn Brown, Elisa V. Quintana
Publikováno v:
Nature, vol 582, iss 7813
Nature
Nature, 582, 497-500
Nature
Nature, 582, 497-500
AU Microscopii (AU Mic) is the second closest pre main sequence star, at a distance of 9.79 parsecs and with an age of 22 million years. AU Mic possesses a relatively rare and spatially resolved3 edge-on debris disk extending from about 35 to 210 ast
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f847eb05b7de1b3f7c7522184d319653
https://escholarship.org/uc/item/1qd287dk
https://escholarship.org/uc/item/1qd287dk
Autor:
Dennis Stello, Duncan J. Wright, Sven Buder, Martin Asplund, Andrew R. Casey, Kenneth C. Freeman, Lorenzo Spina, Klemen Čotar, Joss Bland-Hawthorn, Jonathan Horner, Tomaz Zwitter, Jeffrey D. Simpson, Jake T. Clark, Robert A. Wittenmyer, Sanjib Sharma, Valentina D'Orazi, Catherine Stevens, Janez Kos, Gayandhi M. De Silva, Sarah L. Martell, Stephen R. Kane, Geraint F. Lewis, Daniel B. Zucker, Jane Lin, Karin Lind
Accurate and precise radius estimates of transiting exoplanets are critical for understanding their compositions and formation mechanisms. To know the planet, we must know the host star in as much detail as possible. We present complete results for p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a00d62307604a258b8103486ee224384
http://hdl.handle.net/20.500.12386/31089
http://hdl.handle.net/20.500.12386/31089
Autor:
J. Villasenor, Zachory K. Berta-Thompson, Eric D. Lopez, Jon M. Jenkins, Douglas A. Caldwell, Courtney D. Dressing, Patricia T. Boyd, Joseph D. Twicken, Emily A. Gilbert, Jason D. Eastman, David W. Latham, Sara Seager, Stephen R. Kane, Ryan Cloutier, Joshua E. Schlieder, Natalia Guerrero, Elisa V. Quintana, Joshua N. Winn, Eugene Chiang, Andrew W. Mann, Karen A. Collins, George R. Ricker, Maximilian N. Günther, Caroline V. Morley, Philip S. Muirhead, Thomas Barclay, John P. Doty, Gabrielle Suissa, Chelsea X. Huang, Alan M. Levine, Roland Vanderspek, Eve J. Lee, Andrew Vanderburg, David Charbonneau, Knicole D. Colón, Laura Kreidberg, David R. Ciardi, Elisabeth R. Newton, Alton Spencer, Mark E. Rose, Joseph E. Rodriguez, Tianjun Gan, Sebastian Zieba, Jessie L. Christiansen, Samuel N. Quinn, Ravi Kumar Kopparapu
We present $Spitzer$ 4.5$��$m observations of the transit of TOI-700 d, a habitable zone Earth-sized planet in a multiplanet system transiting a nearby M-dwarf star (TIC 150428135, 2MASS J06282325-6534456). TOI-700 d has a radius of $1.144^{+0.06
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2e43216146356525a0962901013b2eab
Autor:
Veselin B. Kostov, Stephen R. Kane, Ravi Kumar Kopparapu, Eric T. Wolf, Jacob Haqq-Misra, Wolf Cukier, William F. Welsh
We use a one-dimensional (1-D) cloud-free climate model to estimate habitable zone (HZ) boundaries for terrestrial planets of masses 0.1 M$_{E}$ and 5 M$_{E}$ around circumbinary stars of various spectral type combinations. Specifically, we consider
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7275f615614f64993fa6f09f84d7e01a
http://arxiv.org/abs/1911.02983
http://arxiv.org/abs/1911.02983