Zobrazeno 1 - 10
of 119
pro vyhledávání: '"Martin Kürster"'
Autor:
Trifon Trifonov, Rafael Brahm, Andrés Jordán, Christian Hartogh, Thomas Henning, Melissa J. Hobson, Martin Schlecker, Saburo Howard, Finja Reichardt, Nestor Espinoza, Man Hoi Lee, David Nesvorny, Felipe I. Rojas, Khalid Barkaoui, Diana Kossakowski, Gavin Boyle, Stefan Dreizler, Martin Kürster, René Heller, Tristan Guillot, Amaury H. M. J. Triaud, Lyu Abe, Abdelkrim Agabi, Philippe Bendjoya, Nicolas Crouzet, Georgina Dransfield, Thomas Gasparetto, Maximilian N. Günther, Wenceslas Marie-Sainte, Djamel Mékarnia, Olga Suarez, Johanna Teske, R. Paul Butler, Jeffrey D. Crane, Stephen Shectman, George R. Ricker, Avi Shporer, Roland Vanderspek, Jon M. Jenkins, Bill Wohler, Karen A. Collins, Kevin I. Collins, David R. Ciardi, Thomas Barclay, Ismael Mireles, Sara Seager, Joshua N. Winn
Publikováno v:
The Astronomical Journal, Vol 165, Iss 4, p 179 (2023)
The K-type star TOI-2525 has an estimated mass of M = ${0.849}_{-0.033}^{+0.024}$ M _⊙ and radius of R = ${0.785}_{-0.007}^{+0.007}$ R _⊙ observed by the TESS mission in 22 sectors (within sectors 1 and 39). The TESS light curves yield significan
Externí odkaz:
https://doaj.org/article/8bca647556104094acecf0b967a78331
Autor:
Trifon Trifonov, Anna Wollbold, Martin Kürster, Jan Eberhardt, Stephan Stock, Thomas Henning, Sabine Reffert, R. Paul Butler, Steven S. Vogt, Ansgar Reiners, Man Hoi Lee, Bertram Bitsch, Mathias Zechmeister, Florian Rodler, Volker Perdelwitz, Lev Tal-Or, Jan Rybizki, Paul Heeren, Davide Gandolfi, Oscar Barragán, Olga Zakhozhay, Paula Sarkis, Marcelo Tala Pinto, Diana Kossakowski, Vera Wolthoff, Stefan S. Brems, Vera Maria Passegger
Based on recently-taken and archival HARPS, FEROS and HIRES radial velocities (RVs), we present evidence for a new planet orbiting the first ascent red giant star HD33142 (with an improved mass estimate of 1.52$\pm$0.03 M$_\odot$), already known to h
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::39d55f7565f675529e3b23b02bc6ebe7
http://arxiv.org/abs/2206.03899
http://arxiv.org/abs/2206.03899
Autor:
Olga V. Zakhozhay, Ralf Launhardt, Trifon Trifonov, Martin Kürster, Sabine Reffert, Thomas Henning, Rafael Brahm, José I. Vinés, Gabriel-Dominique Marleau, Jayshil A. Patel
Aiming to detect planetary companions to young stars with debris disks via the radial velocity method, we observed HD114082 during April 2018 - August 2022 as one of the targets of our RVSPY program (Radial Velocity Survey for Planets around Young st
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::68041721b18352dcc0eb78124c0d3f41
https://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&origin=inward&scp=85145255772
https://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&origin=inward&scp=85145255772
Autor:
Néstor Espinoza, Enric Pallé, Jonas Kemmer, Rafael Luque, José A. Caballero, Carlos Cifuentes, Enrique Herrero, Víctor J. Sánchez Béjar, Stephan Stock, Karan Molaverdikhani, Giuseppe Morello, Diana Kossakowski, Martin Schlecker, Pedro J. Amado, Paz Bluhm, Miriam Cortés-Contreras, Thomas Henning, Laura Kreidberg, Martin Kürster, Marina Lafarga, Nicolas Lodieu, Juan Carlos Morales, Mahmoudreza Oshagh, Vera M. Passegger, Alexey Pavlov, Andreas Quirrenbach, Sabine Reffert, Ansgar Reiners, Ignasi Ribas, Eloy Rodríguez, Cristina Rodríguez López, Andreas Schweitzer, Trifon Trifonov, Priyanka Chaturvedi, Stefan Dreizler, Sandra V. Jeffers, Adrian Kaminski, María José López-González, Jorge Lillo-Box, David Montes, Grzegorz Nowak, Santos Pedraz, Siegfried Vanaverbeke, Maria R. Zapatero Osorio, Mathias Zechmeister, Karen A. Collins, Eric Girardin, Pere Guerra, Ramon Naves, Ian J. M. Crossfield, Elisabeth C. Matthews, Steve B. Howell, David R. Ciardi, Erica Gonzales, Rachel A. Matson, Charles A. Beichman, Joshua E. Schlieder, Thomas Barclay, Michael Vezie, Jesus Noel Villaseñor, Tansu Daylan, Ismael Mireies, Diana Dragomir, Joseph D. Twicken, Jon Jenkins, Joshua N. Winn, David Latham, George Ricker, Sara Seager
Publikováno v:
The Astronomical Journal
E-Prints Complutense. Archivo Institucional de la UCM
instname
Digital.CSIC. Repositorio Institucional del CSIC
E-Prints Complutense. Archivo Institucional de la UCM
instname
Digital.CSIC. Repositorio Institucional del CSIC
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___::fd19817213d222654942245ae783d216
https://hdl.handle.net/21.11116/0000-000C-B17B-2
https://hdl.handle.net/21.11116/0000-000C-B17B-2
Autor:
Olga V. Zakhozhay, Ralf Launhardt, Andre Müller, Stefan S. Brems, Paul Eigenthaler, Mario Gennaro, Angela Hempel, Maren Hempel, Thomas Henning, Grant M. Kennedy, Sam Kim, Martin Kürster, Régis Lachaume, Yashodhan Manerikar, Jayshil A. Patel, Alexey Pavlov, Sabine Reffert, Trifon Trifonov
Context. The occurrence rate and period distribution of (giant) planets around young stars is still not as well constrained as for older main-sequence stars. This is mostly due to the intrinsic activity-related complications and the avoidance of youn
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::477c5ca140d60003d1107a2dcc38cd91
http://wrap.warwick.ac.uk/168911/7/WRAP-RVSPY-Radial-Velocity-Survey-for-Planets-around-Young-Stars-Target-characterization-high-cadence-survey-2022.pdf
http://wrap.warwick.ac.uk/168911/7/WRAP-RVSPY-Radial-Velocity-Survey-for-Planets-around-Young-Stars-Target-characterization-high-cadence-survey-2022.pdf
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:
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:
D. Galadí-Enríquez, Ignasi Ribas, Enric Palle, M. Lafarga, Stefan Dreizler, Cristina Rodríguez-López, Víctor J. S. Béjar, Jose A. Caballero, Andreas Quirrenbach, Ansgar Reiners, Andreas Schweitzer, M. R. Zapatero Osorio, S. V. Jeffers, Adrian Kaminski, Mathias Zechmeister, Manuel Perger, Martin Kürster, A. P. Hatzes, Guillem Anglada-Escudé, D. Montes, Pedro J. Amado, Juan Carlos Morales, Thomas Henning
Publikováno v:
Digital.CSIC: Repositorio Institucional del CSIC
Consejo Superior de Investigaciones Científicas (CSIC)
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
instname
E-Prints Complutense. Archivo Institucional de la UCM
Digital.CSIC. Repositorio Institucional del CSIC
Consejo Superior de Investigaciones Científicas (CSIC)
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
instname
E-Prints Complutense. Archivo Institucional de la UCM
Digital.CSIC. Repositorio Institucional del CSIC
Context. The interaction between Earth-like exoplanets and the magnetic field of low-mass host stars are considered to produce weak emission signals at radio frequencies. A study using LOFAR data announced the detection of radio emission from the mid
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d5be4dd6e2211a439461a3a0c6fbea92