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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
We analyze the outburst experienced by the September ?-Perseid meteor shower on 9 September 2013. As a result of our monitoring the atmospheric trajectory of 60 multistation events observed over Spain was obtained and accurate orbital data were [...]texto impreso
Arrabal Haro, P. ; Rodríguez Espinosa, J.M. ; Muñoz Tuñón, C. ; Sobral, D. ; Lumbreras Calle, A. ; Boquien, M. ; Hernán Caballero, A. ; Rodríguez Muñoz, L. ; Alcalde Pampliega, Belén | Oxford University Press. | 2020-06Lyman alpha emitters (LAEs) and Lyman break galaxies (LBGs) represent the most common groups of star-forming galaxies at high z, and the differences between their inherent stellar populations (SPs) are a key factor in understanding early galaxy [...]texto impreso
This is an erratum to the paper ‘The Herschel PEP/HerMES Luminosity Function – I: Probing the Evolution of PACS selected Galaxies to z ? 4’, by Gruppioni et al., published in MNRAS, 432, 23 (2013).texto impreso
The next generation of galaxy surveys will allow us to test one of the most fundamental assumptions of the standard cosmology, i.e. that gravity is governed by the general theory of relativity (GR). In this paper, we investigate the ability of t[...]texto impreso
Barrio Uña, Juan Abel ; Bonnefoy, Simon ; Contreras González, José Luis ; Domínguez Díaz, Alberto ; Fonseca González, Mª Victoria ; Fidalgo, David ; López Moya, Marcos ; Nievas Rosillo, Mireia ; Barres de Almeida, U. ; Barrio, J.A. ; otros, ... | Oxford University Press. | 2017-10The microquasar V404 Cygni underwent a series of outbursts in 2015, June 15-31, during which its flux in hard X-rays (20-40 keV) reached about 40 times the Crab nebula flux. Because of the exceptional interest of the flaring activity from this s[...]texto impreso
Bará, Salvador ; Aubé, Martin ; Barentine, John ; Zamorano Calvo, Jaime | Oxford University Press. | 2020-04The visual brightness of the night sky is not a single-valued function of its brightness in other photometric bands, because the transformations between photometric systems depend on the spectral power distribution of the skyglow. We analyze the[...]texto impreso
García Vargas, M. L. ; Carrasco, E. ; Mollá, M. ; Gil de Paz, Armando ; Berlanas, S.R. ; Cardiel López, Nicolás ; Gómez Álvarez, P. ; Gallego Maestro, Jesús ; Iglesias Páramo, J. ; Cedazo, R. ; Pascual Ramírez, Sergio ; Castillo Morales, África ; Pérez Calpena, A. ; Martínez Delgado, I. | Oxford University Press. | 2020-03MEGARA (Multi Espectrografo en GTC de Alta Resolucion para Astronomia) is an optical (3650-9750 Å), fibre-fed, medium-high spectral resolution (R = 6000, 12 000 and 20 000) instrument for the Gran Telescopio CANARIAS (GTC) 10.4-m telescope, comm[...]texto impreso
Gil de Paz, Armando ; Gallego Maestro, Jesús ; Castillo Morales, África ; Pascual Ramírez, Sergio ; Cardiel López, Nicolás | Oxford University Press. | 2020-04We present our analysis of high-resolution (R ? 20 000) GTC/MEGARA integral-field unit spectroscopic observations, obtained during the commissioning run, in the inner region (12.5 arcsec × 11.3 arcsec) of the active galaxy NGC 7469, at spatial s[...]texto impreso
Barrio Uña, Juan Abel ; Bonnefoy, Simon ; Contreras González, José Luis ; Domínguez Díaz, Alberto ; Fidalgo, David Friedrich Carreto ; Fonseca González, Mª Victoria ; López Moya, Marcos ; Nievas Rosillo, Mireia ; Ahnen, L.M. ; Ansoldi, S. ; otros, ... | Oxford University Press. | 2017-10Spontaneous breaking of Lorentz symmetry at energies on the order of the Planck energy or lower is predicted by many quantum gravity theories, implying non-trivial dispersion relations for the photon in vacuum. Consequently, gamma-rays of differ[...]texto impreso
Rodríguez Muñoz, L. ; Rodighiero, G. ; Mancini, C. ; Pérez González, Pablo Guillermo ; Rawle, T.D. ; Egami, E. ; Mercurio, A. ; Rosati, P. ; Puglisi, A. ; Franceschini, A. ; Balestra, I. ; Baronchelli, I. ; Biviano, A. ; Ebeling, H. ; Edge, A,C ; Enia, A.F.M. ; Grillo, C. ; Haines, C.P. ; Iani, E. ; Jones, T. ; Nonino, M. ; Valtchanov, I. ; Vulcani, B. ; Zemcov, M. | Oxford University Press. | 2019-05We quantify the star formation (SF) in the inner cores (R/R_(200) ?0.3) of 24 massive galaxy clusters at 0.2texto impreso
Gómez Marfil, Emilio ; Tabernero, H.M. ; Montes Gutiérrez, David ; Caballero, J. A. ; Soto, M.G. ; González Hernández, J. I. ; Kaminski, A. ; Nagel, E. ; Jeffers, S.V. ; Reiners, A. ; Ribas, I. ; Quirrenbach, A. ; Amado, P.J. | Oxford University Press. | 2020-03With the purpose of assessing classic spectroscopic methods on high-resolution and high signal-to-noise ratio spectra in the near-infrared wavelength region, we selected a sample of 65 F-, G-, and K-type stars observed with CARMENES, the new, ul[...]
