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pro vyhledávání: '"F. Mallia"'
Akademický článek
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Akademický článek
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Autor:
Roland Vanderspek, Michele L. Silverstein, Danielle Dineen, Ethan Kruse, Stephen A. Rinehart, Matthew S. Clement, Emily A. Gilbert, Jessie L. Christiansen, Courtney D. Dressing, Joseph E. Rodriguez, Tansu Daylan, Christopher Lam, Keivan G. Stassun, Tianjun Gan, Sebastian Zieba, Nikole K. Lewis, Mario Di Sora, Veselin B. Kostov, Jonathan Brande, Jennifer G. Winters, George R. Ricker, Eric T. Wolf, Teresa Monsue, Eric D. Lopez, Karen A. Collins, Laura Kreidberg, Wei-Chun Jao, Stephen R. Kane, Naylynn Tañón Reyes, Andrew Couperus, Carl Ziegler, F. Mallia, Benjamin J. Shappee, Gabrielle Suissa, Kelsey Hoffman, Giovanni Covone, Laura D. Vega, Jeffrey C. Smith, Allison Youngblood, Bárbara Rojas-Ayala, Knicole D. Colón, Patricia T. Boyd, Fred C. Adams, Sean N. Raymond, Joel D. Hartman, Todd J. Henry, Geronimo L. Villanueva, Ravi Kumar Kopparapu, Avi Mandell, Christopher J. Burke, Giada Arney, Brianna Galgano, Mark E. Everett, Peter Tenenbaum, Gáspár Á. Bakos, Cesar Briceno, Samuel N. Quinn, Elisa V. Quintana, Mackenna L. Wood, Eve J. Lee, Alex R. Howe, Sarah E. Logsdon, Thomas Fauchez, Zahra Essack, Dennis M. Conti, Andrew W. Mann, Nora L. Eisner, Rishi R. Paudel, Jack J. Lissauer, Quadry Chance, Peter Plavchan, Lucianne M. Walkowicz, Fergal Mullally, Vladimir Airapetian, Eliot Halley Vrijmoet, Eric L. N. Jensen, David W. Latham, Thomas Barclay, Benjamin J. Hord, Joshua E. Schlieder, Nicholas M. Law, Jon M. Jenkins, Joshua N. Winn, Steve B. Howell, Susan E. Mullally, Andrew Vanderburg, David R. Ciardi, Lisa Kaltenegger, Jason F. Rowe, Luca Cacciapuoti, Giovanni Isopi, Sara Seager, Rachel A. Matson, Ryan Cloutier, Daria Pidhorodetska
Publikováno v:
The Astronomical Journal
The Astronomical Journal, American Astronomical Society, 2020, 160 (3), pp.116. ⟨10.3847/1538-3881/aba4b2⟩
The Astronomical Journal, American Astronomical Society, 2020, 160 (3), pp.116. ⟨10.3847/1538-3881/aba4b2⟩
We present the discovery and validation of a three-planet system orbiting the nearby (31.1 pc) M2 dwarf star TOI-700 (TIC 150428135). TOI-700 lies in the TESS continuous viewing zone in the Southern Ecliptic Hemisphere; observations spanning 11 secto
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c8bcb0cbe4b07772e10cfd6829967098
https://hal.archives-ouvertes.fr/hal-02997986
https://hal.archives-ouvertes.fr/hal-02997986
Autor:
Sharon X. Wang, Diana Dragomir, Étienne Artigau, Pedro Figueira, Z. Essack, Andrés Jordán, David R. Anderson, Stéphane Udry, Nicholas M. Law, Thomas Henning, Roland Vanderspek, Rhodes Hart, Howard M. Relles, T. Forveille, C. Ziegler, C. Lovis, J. Villasenor, Pascal Torres, Jon M. Jenkins, Johanna Teske, Rodrigo F. Díaz, Joshua N. Winn, J. R. De Medeiros, David Charbonneau, Ryan Cloutier, Ian J. M. Crossfield, Jose-Manuel Almenara, Fabo Feng, Daniel A. Nusdeo, Keivan G. Stassun, S. Shectman, Nuno C. Santos, Dennis M. Conti, Damien Ségransan, Jennifer G. Winters, Ana Glidden, James S. Jenkins, N. Guerrero, François Bouchy, Misty Davies, Sara Seager, Andrew W. Mann, C. Melo, Avi Shporer, Tianjun Gan, Coel Hellier, Giovanni Isopi, Néstor Espinoza, René Doyon, Elliott P. Horch, Rafael Brahm, Jason D. Eastman, Xavier Bonfils, Jeffrey C. Smith, Francesco Pepe, David W. Latham, John F. Kielkopf, Karen A. Collins, Nicola Astudillo-Defru, R. P. Butler, Cesar Briceno, X. Delfosse, Felipe Murgas, Mark E. Rose, George Zhou, Ronald E. Mennickent, L. Mignon, George R. Ricker, F. Mallia, Jeffrey D. Crane
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Astronomy & Astrophysics
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 636, pp.A58. ⟨10.1051/0004-6361/201937179⟩
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Astronomy & Astrophysics
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 636, pp.A58. ⟨10.1051/0004-6361/201937179⟩
We report the detection of a transiting super-Earth-sized planet (R=1.39+-0.09 Rearth) in a 1.4-day orbit around L 168-9 (TOI-134),a bright M1V dwarf (V=11, K=7.1) located at 25.15+-0.02 pc. The host star was observed in the first sector of the Trans
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7473a803ec8849aa4d3a54d65db9a297
Autor:
Todd C. Klaus, Jose I. Vines, Ruth Titz-Weider, Motohide Tamura, Jessie L. Christiansen, Samuel N. Quinn, M. G. Soto, J. Villasenor, Pablo Rojas, George R. Ricker, Simon R. Walker, Maximiliano Moyano, Nicolás T. Kurtovic, Sara Seager, Sean McCauliff, Maximilian N. Günther, Andrés Jordán, Juan Cabrera, Pascal Torres, Michael R. Goad, Jerome de Leon, Giovanni Isopi, David R. Ciardi, Daniel Bayliss, K. I. Collins, Peter J. Wheatley, Jack J. Lissauer, Norio Narita, David W. Latham, François Bouchy, Sarah L. Casewell, Oliver Turner, Mayuko Mori, Andrea Ercolino, Cristobal Petrovich, Richard G. West, E. Foxell, Claudia Belardi, Philipp Eigmüller, James McCormac, Tom Louden, Eric D. Lopez, Liam Raynard, Benjamin F. Cooke, Edward Gillen, George W. King, Allyson Bieryla, Karen A. Collins, Matias Diaz, Heike Rauer, David J. Armstrong, Jack S. Acton, James A. G. Jackman, Don Pollacco, Anders Erikson, Néstor Espinoza, Michael Vezie, Samuel Gill, Nicholas M. Law, Carl Ziegler, Jon M. Jenkins, Edward M. Bryant, Rafael Brahm, Alexis M. S. Smith, Charles Beichman, Boris T. Gänsicke, Roland Vanderspek, Andrew W. Mann, Taku Nishiumi, Pía Cortés-Zuleta, Didier Queloz, Rosanna H. Tilbrook, Matthew J. Hooton, Louise D. Nielsen, Joshua N. Winn, Christopher J. Burke, Alexander Chaushev, Matthew R. Burleigh, Enric Palle, James S. Jenkins, Christopher E. Henze, Stéphane Udry, F. Mallia, Christopher A. Watson
Publikováno v:
Jenkins, J S, Díaz, M R, Kurtovic, N T, Espinoza, N, Vines, J I, Rojas, P A P, Brahm, R, Torres, P, Cortés-Zuleta, P, Soto, M G, Lopez, E D, King, G W, Wheatley, P J, Winn, J N, Ciardi, D R, Ricker, G, Vanderspek, R, Latham, D W, Seager, S, Jenkins, J M, Beichman, C A, Bieryla, A, Burke, C J, Christiansen, J L, Henze, C E, Klaus, T C, McCauliff, S, Mori, M, Narita, N, Nishiumi, T, Tamura, M, Leon, J P D, Quinn, S N, Villaseñor, J N, Vezie, M, Lissauer, J J, Collins, K A, Collins, K I, Isopi, G, Mallia, F, Ercolino, A, Petrovich, C, Jordán, A, Acton, J S, Armstrong, D J, Bayliss, D, Bouchy, F, Claudia~Belardi, Bryant, E M, Burleigh, M R, Cabrera, J, Casewell, S L, Chaushev, A, Cooke, B F, Eigmüller, P, Erikson, A, Foxell, E, Gänsicke, B T, Gill, S, Gillen, E, Günther, M N, Goad, M R, Hooton, M J, Jackman, J A G, Louden, T, McCormac, J, Moyano, M, Nielsen, L D, Pollacco, D, Queloz, D, Rauer, H, Raynard, L, Smith, A M S, Tilbrook, R H, Titz-Weider, R, Turner, O, Udry, S, Walker, S R, Watson, C A, West, R G, Palle, E, Ziegler, C, Law, N & Mann, A W 2020, ' An Ultra-Hot Neptune in the Neptune desert ', Nature Astronomy . https://doi.org/10.1038/s41550-020-1142-z
About one out of 200 Sun-like stars has a planet with an orbital period shorter than one day: an ultra-short-period planet (Sanchis-ojeda et al. 2014; Winn et al. 2018). All of the previously known ultra-short-period planets are either hot Jupiters,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bd71a0a3787ce478c1aff403cd637b07
Autor:
David R. Ciardi, Emmanuel Jehin, Giovanni Isopi, Robert F. Goeke, K. I. Collins, Jessica E. Libby-Roberts, Bárbara Rojas-Ayala, Jacob L. Bean, Khalid Barkaoui, Francisco J. Pozuelos, M. L. Silverstein, George R. Ricker, David W. Latham, F. Mallia, Joshua N. Winn, Alan M. Levine, William Waalkes, Jessie L. Christiansen, Carl Ziegler, Zachory K. Berta-Thompson, Sara Seager, Elisabeth R. Newton, Joseph D. Twicken, Roland Vanderspek, Tianjun Gan, S. A. Rinehart, Dennis M. Conti, Benjamin M. Tofflemire, Benjamin T. Montet, Karen A. Collins, Michaël Gillon, Mark E. Rose, Adina D. Feinstein, Eric L. N. Jensen, Andrew W. Mann, H. P. Osborn, Nicholas M. Law, Jon M. Jenkins, Cesar Briceno, Eric B. Ting, John F. Kielkopf, Howard M. Relles
We report the discovery and validation of TOI 122b and TOI 237b, two warm planets transiting inactive M dwarfs observed by \textit{TESS}. Our analysis shows TOI 122b has a radius of 2.72$\pm$0.18 R$_\rm{e}$ and receives 8.8$\pm$1.0$\times$ Earth's bo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::18f7deffdd9c353705a394000c432be1
Autor:
Sigfried Vanaverbeke, Jan Subjak, John H. Livingston, D. Hidalgo, Martin Kürster, Peter Plavchan, M. R. Zapatero Osorio, Malcolm Fridlund, Savita Mathur, Grzegorz Nowak, Pedro J. Amado, William D. Cochran, Juan Carlos Morales, Sara Seager, Lev Tal-Or, George R. Ricker, S. Pedraz, Mathias Zechmeister, Jose A. Caballero, Ignasi Ribas, Carlos Cifuentes, E. González-Álvarez, D. Montes, Th. Henning, Y. Shan, R. A. Garcia, Giovanni Isopi, Vincent Van Eylen, L. González-Cuesta, Diana Kossakowski, M. Lafarga, Karen A. Collins, Roland Vanderspek, P. Guerra, J. Kemmer, Heike Rauer, Jorge Lillo-Box, A. R. G. Santos, J. Wittrock, Trifon Trifonov, Néstor Espinoza, M. Cortés-Contreras, B. Cale, P. Schöfer, David Barrado, Enric Palle, Sz. Csizmadia, K. I. Collins, Stefan Dreizler, F. Mallia, Cristina Rodríguez-López, Víctor J. S. Béjar, Eric L. N. Jensen, Maria Morales-Calderon, Andrea Ercolino, S. Stock, Norio Narita, Andreas Quirrenbach, Rafael Luque, E. Herrero, Seth Redfield, P. Bluhm, Andreas Schweitzer, Martin Schlecker, Ansgar Reiners, M. G. Soto, Judith Korth, Sabine Reffert, E. Gaidos, S. V. Jeffers, Carina M. Persson, Petr Kabath, M. El Mufti, Felipe Murgas, Iskra Georgieva, Adrian Kaminski, Eric D. Lopez, Priyanka Chaturvedi, A. P. Hatzes, F. Zohrabi, Mahmoudreza Oshagh, Jon M. Jenkins, V. M. Passegger, E. Díez Alonso
Publikováno v:
Astronomy & Astrophysics, 639, A132
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
Astronomy & Astrophysics
Digital.CSIC. Repositorio Institucional del CSIC
instname
E-Prints Complutense. Archivo Institucional de la UCM
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
Astronomy & Astrophysics
Digital.CSIC. Repositorio Institucional del CSIC
instname
E-Prints Complutense. Archivo Institucional de la UCM
All authors: Bluhm, P.; Luque, R.; Espinoza, N.; Pallé, E.; Caballero, J. A.; Dreizler, S.; Livingston, J. H.; Mathur, S.; Quirrenbach, A.; Stock, S.; Van Eylen, V.; Nowak, G.; López, E. D.; Csizmadia, Sz.; Zapatero Osorio, M. R.; Schöfer, P.; Lil
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ce1bd4a6aafc92ef3b3d112ef1914e61
Akademický článek
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Autor:
Jon M. Jenkins, Steven Villeneuva, Mackenna L. Wood, Coel Hellier, Luke G. Bouma, John F. Kielkopf, Sara Seager, Jason J. Wang, Joseph E. Rodriguez, Christopher J. Burke, Thomas Barclay, Raquel A. Martinez, Joel Villasenor, Robert L. Morris, Adam L. Kraus, Pa Chia Thao, Gregory A. Feiden, Andrew W. Mann, Karen A. Collins, Eric L. Nielsen, Andrew Vanderburg, Robert J. De Rosa, Robert A. Wittenmyer, Misty Davies, Matthew W. Mengel, Jie Li, Chris Stockdale, Jack Okumura, Aaron C. Rizzuto, Logan A. Pearce, Jack J. Lissauer, David W. Latham, Rhodes Hart, Joshua N. Winn, Bruce Macintosh, Duncan J. Wright, Diana Dragomir, Koji Mukai, Rayna Rampalli, George R. Ricker, F. Mallia, Marshall C. Johnson, David R. Anderson, Jean-Baptiste Ruffio, Roland Vanderspek, Carolyn Brown, Peter F. Nelson, Giovanni Isopi, Benjamin M. Tofflemire, Ian A. Waite, Elisabeth R. Newton, Michael Fausnaugh
Young exoplanets are snapshots of the planetary evolution process. Planets that orbit stars in young associations are particularly important because the age of the planetary system is well constrained. We present the discovery of a transiting planet
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::62f0b24f015cd6dba0f6bd06cb74b56a
https://resolver.caltech.edu/CaltechAUTHORS:20190723-152802874
https://resolver.caltech.edu/CaltechAUTHORS:20190723-152802874
Autor:
Jon M. Jenkins, Francisco J. Pozuelos, Timothy D. Morton, Jennifer G. Winters, Khalid Barakoui, Ian A. Waite, Jennifer Burt, Elisabeth Matthews, Songhu Wang, Sébastien Lépine, Enric Palle, Steve B. Howell, Thiam-Guan Tan, Howard M. Relles, Eric B. Ting, Keith Horne, John F. Kielkopf, Diana Dragomir, Stephen R. Kane, Chelsea X. Huang, Roland Vanderspek, Avi Shporer, Tianjun Gan, Bárbara Rojas-Ayala, Tansu Daylan, Michaël Gillon, James D. Armstrong, Jacob L. Bean, Giovanni Isopi, David R. Ciardi, George R. Ricker, Ian J. M. Crossfield, Emmanuel Jehin, Adina D. Feinstein, F. Mallia, Rachel A. Matson, Sara Seager, Samuel N. Quinn, Natalie M. Batalha, Luke G. Bouma, Michael J. Ireland, Michael Fausnaugh, Juan C. Suárez, Jason A. Dittmann, Joshua E. Schlieder, Natalia Guerrero, Benjamin T. Montet, Douglas A. Caldwell, Kevin I. Collins, Joshua N. Winn, Joseph D. Twicken, Gabor Furesz, Ramotholo Sefako, A. Bonfanti, Andrew Vanderburg, Karen A. Collins, David W. Latham, Maximilian N. Günther, Jack J. Lissauer, G. Myers
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
arXiv
instname
arXiv
One of the primary goals of exoplanetary science is to detect small, temperate planets passing (transiting) in front of bright and quiet host stars. This enables the characterization of planetary sizes, orbits, bulk compositions, atmospheres and form
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b28438e2f478642552a5cab79af86141
http://hdl.handle.net/10261/194852
http://hdl.handle.net/10261/194852