Información del autor
Autor Gallego Maestro, Jesús |
Documentos disponibles escritos por este autor (176)
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Gil de Paz, Armando ; Silich, S. A. ; Madore, B. F. ; Sánchez Contreras, C. ; Zamorano Calvo, Jaime ; Gallego Maestro, Jesús | Univ. Chicago Press | 2002-07-10We have mapped the ^(12)CO J = 1-0 and J = 2-1 line emission in Markarian 86, one of the most metal- deficient blue compact dwarf galaxies so far detected in ^(12)CO. The ^(12)CO emission is distributed in a horseshoelike structure that follows [...]texto impreso
Barro, G. ; Gallego Maestro, Jesús ; Villar, V. ; Zamorano Calvo, Jaime | Instituto de Astronomía de la UNAM. Universidad Nacional Autónoma de México | 2007The 3C Database aims to provide complete multi-wavelength information over different cosmological fields, such as GOODS, Groth or Sa68 allowing detailed studies on wide samples of galaxies.texto impreso
Pérez Gallego, J. ; Guzmán, R. ; Castillo Morales, África ; Castander, F. J. ; Gallego Maestro, Jesús ; Garland, C. A. ; Gruel, N. ; Pisano, D. J. ; Sánchez, S. F. ; Zamorano Calvo, Jaime | Wiley | 2010-02-21The kinematic properties of the ionized gas of local luminous compact blue galaxy NGC 7673 are presented using three-dimensional data taken with the PPAK integral field unit at the 3.5-m telescope in the Centro Astronomico Hispano Aleman. Our da[...]texto impreso
The following authors should be included in the author list of this article: E. Alfaro, J. Gallego, J. J. González, and J. I. González-Serrano. All of them are part of the OTELO project and were not listed in the original version of the article [...]texto impreso
Povi?, M. ; Sánchez Portal, M. ; Pérez García, A. M. ; Bongiovanni, A. ; Cepa, J. ; Huertas Company, M. ; Lara López, M. A. ; Fernández Lorenzo, M. ; Ederoclite, A. ; Alfaro, E. ; Castañeda, H. ; Gallego Maestro, Jesús ; González Serrano, J. I. ; González, J. J. | EDP Sciencies | 2012-05Context. The connection between active galactic nuclei (AGN) and their host galaxies has been widely studied and found to be of great importance for providing answers to some fundamental questions related to AGN fuelling mechanisms, and both the[...]texto impreso
Alonso, O. ; Zamorano Calvo, Jaime ; Rego Fernández, Manuel ; Gallego Maestro, Jesús ; Vitores, A.G. | Kluwer Academic Publ. | 1994The most unambiguous way to discover new emission-line galaxies (ELGs) is directly by the presence of their lines, using objective-prism plates of adequate resolution. The first survey using this technique was developed by Smith in 1975 with the[...]texto impreso
Rodríguez Espinosa, J.M. ; Mas-Hesse, J.M. ; Salvador-Solé, E. ; Calvi, R. ; Manrique, A. ; Chanchaiworawit, K. ; Guzmán, R. ; Gallego Maestro, Jesús ; Herrero, A. ; Marín Franch, A. | Oxford University Press. | 2020-06We show herein that a proto-cluster of Ly ? emitting galaxies, spectroscopically confirmed at redshift 6.5, produces a remarkable number of ionizing continuum photons. We start from the Ly ? fluxes measured in the spectra of the sources detected[...]texto impreso
Aims. Long gamma-ray bursts (LGRBs) are associated with the deaths of massive stars and might therefore be a potentially powerful tool for tracing cosmic star formation. However, especially at low redshifts (ztexto impreso
Alonso, O. ; Zamorano Calvo, Jaime ; Rego Fernández, Manuel ; Gallego Maestro, Jesús | EDP Sciences | 1995-10A full set of algorithms for the automatic analysis of low-resolution objective-prism spectra has been developed with the aim of finding new emission-line galaxies (ELGs) candidates from the Universidad Complutense de Madrid (UCM) survey prism p[...]texto impreso
Ramos Almeida, C. ; Rodríguez Espinosa, J. M. ; Barro, Guillermo ; Gallego Maestro, Jesús ; Pérez González, Pablo Guillermo | IOP publishing ltd | 2009-01We have employed a reliable technique of classification of active galactic nuclei (AGNs) based on the fit of well sampled spectral energy distributions (SEDs) with a complete set of AGN and starburst galaxy templates. We have compiled UV, optica[...]texto impreso
Gil de Paz, Armando ; Silich, S. A. ; Madore, B. F. ; Sánchez Contreras, C. ; Zamorano Calvo, Jaime ; Gallego Maestro, Jesús | American Astronomical Society | 2002-07-10We have mapped the CO^12 J = 1-0 and J = 2-1 line emission in Markarian 86, one of the most metal-deficient blue compact dwarf galaxies so far detected in CO^12. The CO^12 emission is distributed in a horseshoe-like structure that follows the lo[...]texto impreso
Gómez Guijarro, Carlos ; González Martín, Omaira ; Ramos Almeida, Cristina ; Miguel Rodríguez-Espinosa, José ; Gallego Maestro, Jesús | Wiley | 2017-08Several studies of nearby active galactic nuclei (AGNs) have shown that the soft X-ray emission presents a size and morphology resembling that of the narrow-line region (NLR) traced by [O III]. Since the NLR is mainly constituted by gas photoion[...]texto impreso
The Galaxy Origins and Young Assembly (GOYA) survey is designed to study the formation and evolution of 1texto impreso
Salvador Solé, Eduard ; Manrique, Alberto ; Guzmán, Rafael ; Rodríguez Espinosa, José Miguel ; Gallego Maestro, Jesús ; Herrero, Artemio ; Mas-Hesse, J. Miguel ; Marín Franch, Antonio | American Astronomical Society | 2017-01-01We combine observational data on a dozen independent cosmic properties at high-z with the information on reionization drawn from the spectra of distant luminous sources and the cosmic microwave background (CMB) to constrain the interconnected ev[...]texto impreso
Peralta de Arriba, L. ; Balcells, M. ; Trujillo, I. ; Falcón Barroso, J. ; Tapia, T. ; Cardiel López, Nicolás ; Gallego Maestro, Jesús ; Guzmán, R. ; Hempel, A. ; Martín Navarro, I. ; Pérez González, Pablo Guillermo ; Sánchez Blázquez, P. | Wiley | 2015-10-11Several authors have reported that the dynamical masses of massive compact galaxies (M_? ? 10^11?M_?, r_e ? 1?kpc), computed as M_dyn=5.0 ?_e^2r_e/GMdyn=5.0 ?e2re/G, are lower than their stellar masses M_?. In a previous study from our group, th[...]texto impreso
Sánchez de Miguel, Alejandro ; Zamorano Calvo, Jaime ; Gómez Castaño, José ; Pascual Ramírez, Sergio ; López Cayuela, Maria Angeles ; Gallego Maestro, Jesús ; Ocaña González, Francisco ; Martín Martínez, G. ; Larrodera, Carlos ; Tinao, B. ; Oré, S. ; Palos, M.F. ; Challupner, Peter | 2012-07-10The evolution of electric power consumption on public lighting in Spain is obtained from DMSP-OLS satellite data and compared with official data. We provide trends for each Spanish province. Radiance calibrated images for the Iberian peninsula f[...]texto impreso
Emission-line galaxies are an invaluable tool for understanding the evolution of galaxies in the universe. Imaging deep fields with narrowband filters allows not only the selection of these objects, but also inferences about the line flux and th[...]texto impreso
Querejeta, Miguel ; Eliche Moral, María del Carmen ; Tapia, Trinidad ; Borlaff, Alejandro ; Van de Ven, Glenn ; Lyubenova, Mariya ; Martig, Marie ; Falcón Barroso, Jesús ; Méndez Abreu, Jairo ; Zamorano Calvo, Jaime ; Gallego Maestro, Jesús | MDPI AG | 2015-12A number of simulators have argued that major mergers can sometimes preserve discs, but the possibility that they could explain the emergence of lenticular galaxies (S0s) has been generally neglected. In fact, observations of S0s reveal a strong[...]texto impreso
Castillo Domínguez, E. ; Ferrusca Rodríguez, D. ; Tulloch, S. ; Velázquez, M. ; Carrasco, E. ; Gallego Maestro, Jesús ; Gil de Paz, Armando ; Sánchez, F. M. ; Vílchez, J. M. | Spie-Int Soc Optical Engineering | 2012MEGARA (Multi-Espectrografo en GTC de Alta Resolucion para Astronomia) is the new integral field unit (IFU) and multi-object spectrograph (MOS) instrument for the GTC. The spectrograph subsystems include the pseudo-slit, the shutter, the collima[...]texto impreso
Pascual Ramírez, Sergio ; Gallego Maestro, Jesús ; Cardiel López, Nicolás | Universidad Nacional Autónoma México, Instituto Astronomía | 2007EMIR (Balcells et al. 2000) is a near-infrared wide-field camera and multi-object spectrograph being built for the GTC. The Data Reduction Pipeline (DRP) will be optimized for handling and reducing near-infrared data acquired with EMIR.texto impreso
Barro, Guillermo ; Gallego Maestro, Jesús ; Pérez González, Pablo Guillermo ; Eliche Moral, María del Carmen ; Balcells, M. ; Villar, V. ; Cardiel López, Nicolás ; Cristobal Hornillos, D. ; Gil de Paz, Armando ; Guzmán, R. ; Pelló, R. ; Prieto, M. ; Zamorano Calvo, Jaime | SPRINGER-VERLAG BERLIN | 2010We present a study that links the NCs to the rest-frame luminosity functions (LFs) at the passbands probed by the observed K-band at different epochs. Making use of a large K-band selected sample in the Groth Field, HDFN and CDFS (?0.27deg^(2)),[...]texto impreso
Gil de Paz, Armando ; Castillo Morales, África ; Sánchez Penim, Ainhoa ; Verdet Paredes, Antonio ; Pascual Ramírez, Sergio ; Curto, Andrés ; García, Oscar ; Gallego Maestro, Jesús ; otros, ... | Spie-Int Soc Optical Engineering | 2018MEGARA is an IFU & MOS medium-resolution spectrograph that finished its commissioning at the GTC 10m telescope on August 2017. MEGARA is a fiber-fed high-resolution spectrograph with two major units, Fiber-MOS & Spectrograph, that are now locate[...]texto impreso
We present the antireflection coatings of the optical elements of MEGARA, the new integral field and multi-object spectrograph for the Gran Telescopio Canarias. We describe the methodology for optimizing the solutions. We also present the result[...]texto impreso
Pascual Ramírez, Sergio ; Gallego Maestro, Jesús ; Cardiel López, Nicolás ; Eliche Moral, María del Carmen | Universidad Nacional Autónoma Mexico, Inst. de Astronomía | 2013The UCM Instrumentation Group (GUAIX) is developing currently Data Reduction Pipelines (DRP) for four instruments of the GTC: EMIR, FRIDA, MEGARA and MIRADAS. The purpose of the DRPs is to provide astronomers scientific quality data, removing in[...]texto impreso
Gallego Maestro, Jesús ; Zamorano Calvo, Jaime ; Rego Fernández, Manuel ; Vitores, A. G. | EDP Sciencies | 1994-10We analyze a rather interesting galaxy discovered during the UCM survey for new H? emission-line galaxies. The new galaxy UCM 2329+2500 presents a compact core that hosts a Seyfert 1 nucleus. The spectrum of the Seyfert nucleus presents broad co[...]