Zobrazeno 1 - 10
of 149
pro vyhledávání: '"Víctor J. S. Béjar"'
Gliese 12 b: A Temperate Earth-sized Planet at 12 pc Ideal for Atmospheric Transmission Spectroscopy
Autor:
Masayuki Kuzuhara, Akihiko Fukui, John H. Livingston, José A. Caballero, Jerome P. de Leon, Teruyuki Hirano, Yui Kasagi, Felipe Murgas, Norio Narita, Masashi Omiya, Jaume Orell-Miquel, Enric Palle, Quentin Changeat, Emma Esparza-Borges, Hiroki Harakawa, Coel Hellier, Yasunori Hori, Kai Ikuta, Hiroyuki Tako Ishikawa, Takanori Kodama, Takayuki Kotani, Tomoyuki Kudo, Juan C. Morales, Mayuko Mori, Evangelos Nagel, Hannu Parviainen, Volker Perdelwitz, Ansgar Reiners, Ignasi Ribas, Jorge Sanz-Forcada, Bun’ei Sato, Andreas Schweitzer, Hugo M. Tabernero, Takuya Takarada, Taichi Uyama, Noriharu Watanabe, Mathias Zechmeister, Néstor Abreu García, Wako Aoki, Charles Beichman, Víctor J. S. Béjar, Timothy D. Brandt, Yéssica Calatayud-Borras, Ilaria Carleo, David Charbonneau, Karen A. Collins, Thayne Currie, John P. Doty, Stefan Dreizler, Gareb Fernández-Rodríguez, Izuru Fukuda, Daniel Galán, Samuel Geraldía-González, Josafat González-Rodríguez, Yuya Hayashi, Christina Hedges, Thomas Henning, Klaus Hodapp, Masahiro Ikoma, Keisuke Isogai, Shane Jacobson, Markus Janson, Jon M. Jenkins, Taiki Kagetani, Eiji Kambe, Yugo Kawai, Kiyoe Kawauchi, Eiichiro Kokubo, Mihoko Konishi, Judith Korth, Vigneshwaran Krishnamurthy, Takashi Kurokawa, Nobuhiko Kusakabe, Jungmi Kwon, Andrés Laza-Ramos, Florence Libotte, Rafael Luque, Alberto Madrigal-Aguado, Yuji Matsumoto, Dimitri Mawet, Michael W. McElwain, Pedro Pablo Meni Gallardo, Giuseppe Morello, Sara Muñoz Torres, Jun Nishikawa, Stevanus K. Nugroho, Masahiro Ogihara, Alberto Peláez-Torres, David Rapetti, Manuel Sánchez-Benavente, Martin Schlecker, Sara Seager, Eugene Serabyn, Takuma Serizawa, Monika Stangret, Aoi Takahashi, Huan-Yu Teng, Motohide Tamura, Yuka Terada, Akitoshi Ueda, Tomonori Usuda, Roland Vanderspek, Sébastien Vievard, David Watanabe, Joshua N. Winn, Maria Rosa Zapatero Osorio
Publikováno v:
The Astrophysical Journal Letters, Vol 967, Iss 2, p L21 (2024)
Recent discoveries of Earth-sized planets transiting nearby M dwarfs have made it possible to characterize the atmospheres of terrestrial planets via follow-up spectroscopic observations. However, the number of such planets receiving low insolation i
Externí odkaz:
https://doaj.org/article/135ed81aa2bf4c638b0d61cbb2f6cc8b
Autor:
Yasunori Hori, Akihiko Fukui, Teruyuki Hirano, Norio Narita, Jerome P. de Leon, Hiroyuki Tako Ishikawa, Joel D. Hartman, Giuseppe Morello, Nestor Abreu García, Leticia Álvarez Hernández, Víctor J. S. Béjar, Yéssica Calatayud-Borras, Ilaria Carleo, Gareb Enoc, Emma Esparza-Borges, Izuru Fukuda, Daniel Galán, Samuel Geraldía-González, Yuya Hayashi, Masahiro Ikoma, Kai Ikuta, Keisuke Isogai, Taiki Kagetani, Yugo Kawai, Kiyoe Kawauchi, Tadahiro Kimura, Takanori Kodama, Judith Korth, Nobuhiko Kusakabe, Andrés Laza-Ramos, John H. Livingston, Rafael Luque, Kohei Miyakawa, Mayuko Mori, Felipe Murgas, Jaume Orell-Miquel, Enric Palle, Hannu Parviainen, Alberto Peláez-Torres, Marta Puig-Subirà, Manuel Sánchez-Benavente, Paula Sosa-Guillén, Monika Stangret, Yuka Terada, Sara Muñoz Torres, Noriharu Watanabe, Gaspar Á. Bakos, Khalid Barkaoui, Charles Beichman, Zouhair Benkhaldoun, Andrew W. Boyle, David R. Ciardi, Catherine A. Clark, Karen A. Collins, Kevin I. Collins, Dennis M. Conti, Ian J.M. Crossfield, Mark E. Everett, Elise Furlan, Mourad Ghachoui, Michaël Gillon, Erica J. Gonzales, Jesus Higuera, Keith Horne, Steve B. Howell, Emmanuël Jehin, Kathryn V. Lester, Michael B. Lund, Rachel Matson, Elisabeth C. Matthews, Francisco J. Pozuelos, Boris S. Safonov, Joshua E. Schlieder, Richard P. Schwarz, Ramotholo Sefako, Gregor Srdoc, Ivan A. Strakhov, Mathilde Timmermans, William C. Waalkes, Carl Ziegler, David Charbonneau, Zahra Essack, Natalia M. Guerrero, Hiroki Harakawa, Christina Hedges, Masato Ishizuka, Jon M. Jenkins, Mihoko Konishi, Takayuki Kotani, Tomoyuki Kudo, Takashi Kurokawa, Masayuki Kuzuhara, Jun Nishikawa, Masashi Omiya, George R. Ricker, Sara Seager, Takuma Serizawa, Stephanie Striegel, Motohide Tamura, Akitoshi Ueda, Roland Vanderspek, Sébastien Vievard, Joshua N. Winn
Publikováno v:
The Astronomical Journal, Vol 167, Iss 6, p 289 (2024)
Sub-Neptunes with radii of 2–3 R _⊕ are intermediate in size between rocky planets and Neptune-sized planets. The orbital properties and bulk compositions of transiting sub-Neptunes provide clues to the formation and evolution of close-in small p
Externí odkaz:
https://doaj.org/article/e90e706d0f7942389d0887e8f3b38aa6
Autor:
Akihiko Fukui, Tadahiro Kimura, Teruyuki Hirano, Norio Narita, Takanori Kodama, Yasunori Hori, Masahiro Ikoma, Enric Pallé, Felipe Murgas, Hannu Parviainen, Kiyoe Kawauchi, Mayuko Mori, Emma Esparza-Borges, Allyson Bieryla, Jonathan Irwin, Boris S Safonov, Keivan G Stassun, Leticia Alvarez-Hernandez, Víctor J S Béjar, Núria Casasayas-Barris, Guo Chen, Nicolas Crouzet, Jerome P de Leon, Keisuke Isogai, Taiki Kagetani, Peter Klagyivik, Judith Korth, Seiya Kurita, Nobuhiko Kusakabe, John Livingston, Rafael Luque, Alberto Madrigal-Aguado, Giuseppe Morello, Taku Nishiumi, Jaume Orell-Miquel, Mahmoudreza Oshagh, Manuel Sánchez-Benavente, Monika Stangret, Yuka Terada, Noriharu Watanabe, Yujie Zou, Motohide Tamura, Takashi Kurokawa, Masayuki Kuzuhara, Jun Nishikawa, Masashi Omiya, Sébastien Vievard, Akitoshi Ueda, David W Latham, Samuel N Quinn, Ivan S Strakhov, Alexandr A Belinski, Jon M Jenkins, George R Ricker, Sara Seager, Roland Vanderspek, Joshua N Winn, David Charbonneau, David R Ciardi, Karen A Collins, John P Doty, Etienne Bachelet, Daniel Harbeck
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Publications of Astronomical Society of Japan, 74(1), L1-L8
instname
Publications of Astronomical Society of Japan, 74(1), L1-L8
This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the origina
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7b45873c2385329cd150ecf3fc601b66
Autor:
Steve Boudreault, M. R. Zapatero-Osorio, Víctor J. S. Béjar, Elena Manjavacas, Nicolas Lodieu, Mickael Bonnefoy
Publikováno v:
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
instname
Digital.CSIC. Repositorio Institucional del CSIC
Instituto Nacional de Técnica Aeroespacial (INTA)
instname
Digital.CSIC. Repositorio Institucional del CSIC
Instituto Nacional de Técnica Aeroespacial (INTA)
In the past years, some extremely red brown dwarfs were found. They were believed to have low surface gravity, but many of their spectral characteristics were similar to those of high surface gravity brown dwarfs, showing that youth (or low surface g
Autor:
Ignasi Ribas, Enric Palle, Martin Kürster, Th. Henning, Mathias Zechmeister, Stefan Dreizler, Cristina Rodríguez-López, Víctor J. S. Béjar, D. Fabbian, Sandra V. Jeffers, M. Cortés-Contreras, Pedro J. Amado, Andreas Quirrenbach, Hugo M. Tabernero, Emilio Marfil, Juan Carlos Morales, Adrian Kaminski, Andreas Schweitzer, D. Montes, V. M. Passegger, Ansgar Reiners, Jose A. Caballero, Y. Shan, M. Lafarga, A. P. Hatzes, Jesús Aceituno, Evangelos Nagel
Publikováno v:
E-Prints Complutense. Archivo Institucional de la UCM
instname
Digital.CSIC. Repositorio Institucional del CSIC
instname
Digital.CSIC. Repositorio Institucional del CSIC
Context. M-dwarf spectra are complex and notoriously difficult to model, posing challenges to understanding their photospheric properties and compositions in depth. Vanadium (V) is an iron-group element whose abundance supposedly closely tracks that
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::505c503b81ba379719e54489284a1822
http://hdl.handle.net/10261/261151
http://hdl.handle.net/10261/261151
Autor:
Víctor J. S. Béjar, D. Baroch, Carlos Cardona Guillén, Curtis McCully, Daniel Harbeck, Pier-Emmanuel Tremblay, Felipe Murgas, Nicolas Lodieu, Matthew J. Hoskin, P. Schöfer, S. V. Jeffers, D. Montes
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
E-Prints Complutense. Archivo Institucional de la UCM
instname
E-Prints Complutense. Archivo Institucional de la UCM
Context. Double-lined spectroscopic (SB2) binaries allow us to obtain a direct determination of the masses of their components, which is essential to test stellar models. Although these objects only provide a lower limit for the mass, they are more a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ff35f35503673b7bc1f7e50ddacd5e1e
http://arxiv.org/abs/2109.01624
http://arxiv.org/abs/2109.01624
Autor:
Diana Kossakowski, Roland Vanderspek, Norio Narita, Martin Kürster, E. González-Álvarez, A. P. Hatzes, Felipe Murgas, V. M. Passegger, John F. Kielkopf, David Lafrenière, Eric L. N. Jensen, P. Bluhm, R. Cloutier, Adrian Kaminski, Enric Palle, George R. Ricker, Stefan Dreizler, Víctor J. S. Béjar, Jorge Lillo-Box, P. Schöfer, K. I. Collins, S. V. Jeffers, D. Montes, Pedro J. Amado, S. Stock, A. Fukui, Motohide Tamura, Sabine Reffert, Peyton Brown, Rafael Luque, Charles Cadieux, Juan Carlos Morales, J. Kemmer, Karan Molaverdikhani, Jon M. Jenkins, Karen A. Collins, Trifon Trifonov, M. G. Soto, N. Kusakabe, René Doyon, Ansgar Reiners, Sara Seager, Jose A. Caballero, Keith Horne, Andreas Schweitzer, Mathias Zechmeister, Andreas Quirrenbach, Richard P. Schwarz, Néstor Espinoza, Joshua N. Winn, Ignasi Ribas, Th. Henning, M. R. Zapatero Osorio, M. Cortés-Contreras
Publikováno v:
E-Prints Complutense. Archivo Institucional de la UCM
instname
Digital.CSIC: Repositorio Institucional del CSIC
Consejo Superior de Investigaciones Científicas (CSIC)
Astronomy & Astrophysics
Digital.CSIC. Repositorio Institucional del CSIC
instname
Digital.CSIC: Repositorio Institucional del CSIC
Consejo Superior de Investigaciones Científicas (CSIC)
Astronomy & Astrophysics
Digital.CSIC. Repositorio Institucional del CSIC
Full list of authors: Bluhm, P.; Pallé, E.; Molaverdikhani, K.; Kemmer, J.; Hatzes, A. P.; Kossakowski, D.; Stock, S.; Caballero, J. A.; Lillo-Box, J.; Béjar, V. J. S.; Soto, M. G.; Amado, P. J.; Brown, P.; Cadieux, C.; Cloutier, R.; Collins, K. A.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7a3541e5eab3f6ac1ed295383fb2ad80
https://eprints.ucm.es/id/eprint/67934/
https://eprints.ucm.es/id/eprint/67934/
Autor:
Enric Palle, E. Rodríguez, Sabine Reffert, A. Kaminski, Don Pollacco, M. Lafarga, D. Baroch, P. Schöfer, Mathias Zechmeister, J. A. Caballero, J. Colomé, D. Montes, D. Galadí-Enríquez, Martin Kürster, P. J. Amado, Lev Tal-Or, C. Cardona Guillén, Ansgar Reiners, Guillem Anglada-Escudé, A. Rosich, Th. Henning, Andreas Quirrenbach, Ignasi Ribas, Y. Shan, M. Cortés-Contreras, Artie P. Hatzes, Juan Carlos Morales, S. V. Jeffers, Andreas Schweitzer, M. J. López-González, Stefan Dreizler, Cristina Rodríguez-López, Víctor J. S. Béjar, Nicolas Lodieu, Enrique Herrero, M. Perger
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
E-Prints Complutense. Archivo Institucional de la UCM
Universidad Europea (UEM)
instname
E-Prints Complutense. Archivo Institucional de la UCM
Universidad Europea (UEM)
Context. M dwarfs are ideal targets for the search of Earth-size planets in the habitable zone using the radial velocity method, and are attracting the attention of many ongoing surveys. One of the expected results of these surveys is that new multip
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::59079b2accf5951d13315ea70b7fe64b
http://arxiv.org/abs/2105.14770
http://arxiv.org/abs/2105.14770
Autor:
Carlos Cifuentes, J. P. de Leon, Richard P. Schwarz, Joshua N. Winn, Hannu Parviainen, Christopher E. Henze, Thomas Henning, M. Lafarga, Courtney D. Dressing, Martin Kürster, Jorge Sanz-Forcada, Roland Vanderspek, A. Kaminski, Andreas Schweitzer, David W. Latham, Don Pollacco, Guillem Anglada-Escudé, Benjamin T. Montet, Eric L. N. Jensen, P. J. Amado, Jacob L. Bean, Ignasi Ribas, A. Fukui, P. Bluhm, C. Rodríguez López, Sara Seager, Enric Palle, Stefan Dreizler, Víctor J. S. Béjar, E. Esparza-Borges, Andrew W. Mann, Michael Fausnaugh, Rafael Luque, M. Stangret, Jose A. Caballero, Andreas Seifahrt, S. Stock, M. Cortés-Contreras, Karan Molaverdikhani, D. Montes, Núria Casasayas-Barris, Juan Carlos Morales, George R. Ricker, Artie P. Hatzes, Karen A. Collins, Thiam-Guan Tan, Felipe Murgas, Kevin I. Collins, Joseph D. Twicken, Enrique Herrero, Norio Narita, Avi Shporer, Mathias Zechmeister, Trifon Trifonov, Thomas Barclay, P. Tenenbaum, Dennis L. Kasper, Ansgar Reiners, Mahmoudreza Oshagh, Jon M. Jenkins, Julian Stürmer, Coel Hellier, Andreas Quirrenbach, Diana Kossakowski, Néstor Espinoza, V. M. Passegger, Samuel N. Quinn, S. V. Jeffers, M. Azzaro
Publikováno v:
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Universitat Pompeu Fabra
Digital.CSIC. Repositorio Institucional del CSIC
instname
E-Prints Complutense. Archivo Institucional de la UCM
arXiv
Digital.CSIC: Repositorio Institucional del CSIC
Consejo Superior de Investigaciones Científicas (CSIC)
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
Science
Universitat Pompeu Fabra
Digital.CSIC. Repositorio Institucional del CSIC
instname
E-Prints Complutense. Archivo Institucional de la UCM
arXiv
Digital.CSIC: Repositorio Institucional del CSIC
Consejo Superior de Investigaciones Científicas (CSIC)
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
Science
Spectroscopy of transiting exoplanets can be used to investigate their atmospheric properties and habitability. Combining radial velocity (RV) and transit data provides additional information on exoplanet physical properties. We detect a transiting r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4ba1530d15bdf4ceddb872388f6c653d
https://hdl.handle.net/20.500.12666/607
https://hdl.handle.net/20.500.12666/607
Autor:
I. M. Gómez Muñoz, Enrique Solano, Eduardo Martín, M. C. Gálvez-Ortiz, Víctor J. S. Béjar, Adam J. Burgasser, Hervé Bouy, Carlos Rodrigo, Nicolas Lodieu, Maria Morales-Calderon, Nuria Huélamo
Publikováno v:
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
instname
instname
This article is published and distributed under the terms of the Oxford University Press, Standard Journals Publication Model (https://academic.oup.com/journals/pages/open_access/funder_policies/chorus/standard_publication_model) Ultracool dwarfs (UC
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3af4aedab03cdb474ef87bc3d4b7a4f8
http://hdl.handle.net/20.500.12666/565
http://hdl.handle.net/20.500.12666/565