Zobrazeno 1 - 10
of 22
pro vyhledávání: '"B. López-Martí"'
Autor:
E. Racero, Bruno Merín, Deborah Baines, J. González Núñez, P. Rodriguez, M. López-Caniego, Sebastien Besse, I. de la Calle, Elena Puga, Fabrizio Giordano, Th. Müller, Michael Küppers, N. Álvarez Crespo, Benoit Carry, S. Kruk, Max Mahlke, B. López-Martí, M. Wrangblad, Ivan Valtchanov, Henrik Norman, J. Berthier
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 659, ⟨10.1051/0004-6361/202140899⟩
Astronomy and Astrophysics-A&A, 2022, 659, ⟨10.1051/0004-6361/202140899⟩
We introduce in this work the Solar System Object Search Service (SSOSS), a service aimed at providing the scientific community with a search service for all potential detections of SSOs among the ESA astronomy archival imaging data. We illustrate it
Autor:
Ben Burningham, M. C. Gálvez-Ortiz, Derek Homeier, Hugh R. A. Jones, M. R. Zapatero Osorio, Richard L. Smart, Rafael Rebolo, F. Allard, B. López Martí, D. J. Pinfield, Zhenyu Zhang, Nicolas Lodieu, Adam J. Burgasser, E. L. Martín
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2018, 479 (1), pp.1383-1391. ⟨10.1093/mnras/sty1352⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2018, 479 (1), pp.1383-1391. ⟨10.1093/mnras/sty1352⟩
Monthly Notices of the Royal Astronomical Society, 2018, 479 (1), pp.1383-1391. ⟨10.1093/mnras/sty1352⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2018, 479 (1), pp.1383-1391. ⟨10.1093/mnras/sty1352⟩
We report the discovery of an esdL3 subdwarf, ULAS J020858.62+020657.0, and a usdL4.5 subdwarf, ULAS J230711.01+014447.1. They were identified as L subdwarfs by optical spectra obtained with the Gran Telescopio Canarias, and followed up by optical-to
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::222faf944eb63d3659737f1fcc99945d
https://hal.science/hal-02280897
https://hal.science/hal-02280897
Autor:
B. López Martí, Adam J. Burgasser, Nicolas Lodieu, M. R. Zapatero Osorio, Leigh C. Smith, F. Allard, Ben Burningham, Richard L. Smart, Zhenyu Zhang, D. J. Pinfield, Hugh R. A. Jones, Rafael Rebolo, Federico Marocco, E. L. Martín, M. C. Gálvez-Ortiz, Derek Homeier
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2018, 480 (4), pp.5447-5474. ⟨10.1093/mnras/sty2054⟩
Monthly Notices of the Royal Astronomical Society, 2018, 480 (4), pp.5447-5474. ⟨10.1093/mnras/sty2054⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2018, 480 (4), pp.5447-5474. ⟨10.1093/mnras/sty2054⟩
Monthly Notices of the Royal Astronomical Society, 2018, 480 (4), pp.5447-5474. ⟨10.1093/mnras/sty2054⟩
We present 27 new L subdwarfs and classify five of them as esdL and 22 as sdL. Our L subdwarf candidates were selected with the UKIRT Infrared Deep Sky Survey and Sloan Digital Sky Survey. Spectroscopic follow-up was carried out primarily with the OS
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::afc27405c75b3c934de1f5dd82fef4c2
http://arxiv.org/abs/1807.10560
http://arxiv.org/abs/1807.10560
Publikováno v:
Astronomy & Astrophysics. 500:1045-1063
Context. Most studies of the stellar and substellar populations of star-forming regions rely on using the signatures of accretion, outflows, disks, or activity characterizing the early stages of stellar evolution. However, these signatures rapidly de
Autor:
E. De Filippis, F. Comerón, Anna Pasquali, Vallery Stanishev, B. López Martí, Giulia Rodighiero, A. Stankov, M. C. Gálvez Ortiz, Roland Gredel
Publikováno v:
Scopus-Elsevier
We present a near-infrared spectroscopic survey of a large area centered on the Cygnus OB2 association aimed at constraining its massive star contents. Our goal is to establish a nearly complete list of O-type members of the association, both to exam
Autor:
Mercedes Lopez-Morales, F. F. Bauer, Javier López-Santiago, Johana Panduro, E. Mirabet, M. Fernandez, J. Guàrdia, Ana Pérez-Calpena, H. Martínez-Rodríguez, Pedro J. Amado, P. Rhode, M. Kehr, Ansgar Reiners, Mauro López del Fresno, K. F. Huber, E. de Juan, Otmar Stahl, R. G. Ulbrich, David Barrado, M. A. C. Perryman, Enric Palle, Cristina Rodríguez-López, Víctor J. S. Béjar, J. Stürmer, R.-R. Rohloff, D. Benítez, A. Garcia-Piquer, J. Helmling, R. Antona Jiménez, E. Rodríguez-Pérez, B. López Martí, Clemens Storz, Josep Colomé, G. Holgado, D. Galadí, C. Feiz, Sebastian Schafer, W. Xu, R. Morales Muñoz, Ulrich Mall, Werner Laun, A. Ramón, E. de Guindos, R. Garrido, Simon Tulloch, F. J. Alonso-Floriano, A. P. Hatzes, Jesús Aceituno, J. I. González Hernández, S. Dreizler, C. Schmidt, V. Gómez Galera, C. J. Marvin, A. Rosich, A. Claret, Juan Carlos Morales, Mathias Zechmeister, J. H. M. M. Schmitt, Juan Carlos Suárez, S. Reinhardt, Walter Seifert, Rainer Lenzen, C. del Burgo, M. Doellinger, Miguel Abril, Florian Rodler, H. W. Rix, D. Montes, V. M. Passegger, Eike W. Guenther, M. C. Gálvez-Ortiz, Ernesto Sánchez-Blanco, P. Redondo, M. L. García-Vargas, S. Becerril, Holger Mandel, E. González Álvarez, A. Moya, H. Anwand-Heerwart, Vianak Naranjo, Martin Kürster, A. Quirrenbach, Susana Martín-Ruiz, J. Schiller, D. Hidalgo, M. Pluto, D. Hermann, A. Klutsch, D. Pérez Medialdea, Rafael Rebolo, Armin Huber, J. L. Lizon, M. Ammler-von Eiff, E. Rodriguez, M. R. Zapatero Osorio, M. Azzaro, A. Lamert, Guillem Anglada-Escudé, M. A. Sánchez Carrasco, Ralf Klein, Aviv Ofir, Karl Wagner, H. J. Hagen, Eduardo L. Martín, Z. M. Berdiñas, Sandra V. Jeffers, R. Oreiro, L. F. Sarmiento, M. C. Cárdenas, U. Lemke, Ulrich Grözinger, Sabine Reffert, Richard J. Mathar, Jorge Sanz-Forcada, Peter H. Hauschildt, E. Solano, J. Winkler, Manuel Perger, Ignasi Ribas, Th. Henning, S. Lalitha, Juan Gutiérrez-Soto, M. Cortés-Contreras, Lluis Gesa, Jose A. Caballero, L. Hernández Castaño, F. J. Abellán de Paco, E. Herrero, G. Veredas, E. Casal, Viki Joergens, Reinhard Mundt, S. Czesla
Publikováno v:
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
E-Prints Complutense. Archivo Institucional de la UCM
instname
Universidad Complutense de Madrid
E-Prints Complutense. Archivo Institucional de la UCM
instname
This paper gives an overview of the CARMENES instrument and of the survey that will be carried out with it during the first years of operation. CARMENES (Calar Alto high-Resolution search for M dwarfs with Exoearths with Near-infrared and optical Ech
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3f08f87f78b1301a2c8784a478c2b5fc
https://eprints.ucm.es/id/eprint/32540/1/cortescontreras01libre.pdf
https://eprints.ucm.es/id/eprint/32540/1/cortescontreras01libre.pdf
Akademický článek
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Publikováno v:
López Martí, Belén ; Eislöffel, J. ; Scholz, A. ; Mundt, R., 2004, The brown dwarf population in the Chamaeleon I cloud, Astronomy and Astrophysics, vol. 416, no. 2, p. 555-576
RODERIC. Repositorio Institucional de la Universitat de Valéncia
instname
RODERIC. Repositorio Institucional de la Universitat de Valéncia
instname
We present the results of a multiband survey for brown dwarfs in the Chamaeleon I dark cloud with the Wide Field Imager (WFI) camera at the ESO/MPG 2.2-m telescope on La Silla (Chile). The survey has revealed a substantial population of brown dwarfs
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::db55f3ebfc5b0d29cfc368560c8b2742
http://hdl.handle.net/10550/14025
http://hdl.handle.net/10550/14025
Autor:
B. López Martí, M. R. Zapatero Osorio
Publikováno v:
Astronomy & Astrophysics. 568:A87
(abridged) We perform photometric time-series analysis of a sample of ten early to mid-L dwarfs in the field over three years of $K_s$-band observations with the OMEGA 2000 infrared camera of the 3.5m telescope on Calar Alto Observatory between Janua
Publikováno v:
Astronomy & Astrophysics. 554:A86
Context. Many star forming regions are known to have associated dispersed populations, whose members are located away from known current star forming sites. Their origin is unclear, and the identification of the members through relatively short-lived