@book {181,
	title = {{The Spanish Square Kilometre Array White Book}},
	series = {ArXiv e-prints},
	year = {2015},
	keywords = {Astrophysics - Instrumentation and Methods for Astrophysics},
	url = {http://adsabs.harvard.edu/abs/2015arXiv150603474A},
	author = {Acosta-Pulido, J.~A. and Agudo, I. and Alberdi, A. and Alcolea, J. and Alfaro, E.~J. and Alonso-Herrero, A. and Anglada, G. and Arnalte-Mur, P. and Ascasibar, Y. and Ascaso, B. and Azulay, R. and Bachiller, R. and Baez-Rubio, A. and Battaner, E. and Blasco, J. and Brook, C.~B. and Bujarrabal, V. and Busquet, G. and Caballero-Garcia, M.~D. and Carrasco-Gonzalez, C. and Casares, J. and Castro-Tirado, A.~J. and Colina, L. and Colomer, F. and de Gregorio-Monsalvo, I. and del Olmo, A. and Desmurs, J.-F. and Diego, J.~M. and Dominguez-Tenreiro, R. and Estalella, R. and Fernandez-Soto, A. and Florido, E. and Font, J. and Font, J.~A. and Fuente, A. and Garc{\'\i}a-Benito, R. and Garcia-Burillo, S. and Garc{\'\i}a-Lorenzo, B. and Gil de Paz, A. and Girart, J.~M. and Goicoechea, J.~R. and G{\'o}mez, J.~F. and Gonzalez-Garcia, M. and Gonz{\'a}lez-Mart{\'\i}n, O. and Gonzalez-Serrano, J.~I. and Gorgas, J. and Gorosabel, J. and Guijarro, A. and Guirado, J.~C. and Hern{\'a}ndez-Garc{\'\i}a, L. and Hernandez-Monteagudo, C. and Herranz, D. and R. Herrero-Illana and Hu, Y.-D. and Huelamo, N. and Huertas-Company, M. and Iglesias-Paramo, J. and Jeong, S. and Jimenez-Serra, I. and Knapen, J.~H. and Lineros, R.~A. and Lisenfeld, U. and Marcaide, J.~M. and Marquez, I. and Marti, J. and Marti, J.~M. and Mart{\'\i}-Vidal, I. and Martinez-Gonzalez, E. and Martin-Pintado, J. and Masegosa, J. and Mayen-Gijon, J.~M. and Mezcua, M. and Migliari, S. and Mimica, P. and Mold{\'o}n, J. and Morata, O. and Negueruela, I. and Oates, S.~R. and Osorio, M. and Palau, A. and Paredes, J.~M. and Perea, J. and P{\'e}rez-Gonz{\'a}lez, P.~G. and Perez-Montero, E. and M. A. P{\'e}rez-Torres and Perucho, M. and Planelles, S. and Pons, J.~A. and Prieto, A. and Quilis, V. and Ramirez-Moreta, P. and Ramos Almeida, C. and Rea, N. and Rib{\'o}, M. and Rioja, M.~J. and Rodriguez Espinosa, J.~M. and Ros, E. and Rubi{\~n}o-Martin, J.~A. and Ruiz-Granados, B. and Sabater, J. and Sanchez, S. and Sanchez-Contreras, C. and Sanchez-Monge, A. and Sanchez-Ramirez, R. and Sintes, A.~M. and Solanes, J.~M. and Sopuerta, C.~F. and Tafalla, M. and Tello, J.~C. and Tercero, B. and Toribio, M.~C. and Torrelles, J.~M. and Torres, M.~A.~P. and Usero, A. and Verdes-Montenegro, L. and Vidal-Garcia, A. and Vielva, P. and Vilchez, J. and Zhang, B.-B.}
}
@article {2014MNRAS.444L..68R,
	title = {{Episodic star formation in a group of LAEs at z = 5.07}},
	journal = {Monthly Notices of the Royal Astronomical Society},
	volume = {444},
	year = {2014},
	pages = {L68-L72},
	abstract = {We are undertaking a search for high-redshift low-luminosity Lyman Alpha sources in the SHARDS (Survey for High-z Absorption Red and Dead Sources) survey. Among the pre-selected Lyman Alpha sources two candidates were spotted, located 3.19 arcsec apart, and tentatively at the same redshift. Here, we report on the spectroscopic confirmation with Gran Telescopio Canarias of the Lyman Alpha emission from this pair of galaxies at a confirmed spectroscopic redshifts of z=5.07. Furthermore, one of the sources is interacting/merging with another close companion that looks distorted. Based on the analysis of the spectroscopy and additional photometric data, we infer that most of the stellar mass of these objects was assembled in a burst of star formation 100 Myr ago. A more recent burst (2 Myr old) is necessary to account for the measured Lyman Alpha flux. We claim that these two galaxies are good examples of Lyman Alpha sources undergoing episodic star formation. Besides, these sources very likely constitute a group of interacting Lyman Alpha emitters (LAEs).},
	keywords = {galaxies: high-redshift},
	doi = {10.1093/mnrasl/slu099},
	url = {http://adsabs.harvard.edu/abs/2014MNRAS.444L..68R},
	author = {Rodr{\'\i}guez-Espinosa, J.~M. and Gonz{\'a}lez-Mart{\'\i}n, O. and Castro-Rodr{\'\i}guez, N. and P. P{\'e}rez-Gonz{\'a}lez and Mas-Hesse, J.~M. and Mu{\~n}oz-Tu{\~n}{\'o}n, C. and Cava, A. and Cardiel, N. and Cabrera-Lavers, A. and Gallego, J. and Hern{\'a}n-Caballero, A. and Herrera-Ruiz, N. and N. Ram{\'\i}rez-Olivencia}
}
@article {2011MNRAS.410.2556D,
	title = {{Extragalactic background light inferred from AEGIS galaxy-SED-type fractions}},
	journal = {Monthly Notices of the Royal Astronomical Society},
	volume = {410},
	year = {2011},
	month = {feb},
	pages = {2556-2578},
	abstract = {The extragalactic background light (EBL) is of fundamental importance both for understanding the entire process of galaxy evolution and for {$\gamma$}-ray astronomy, but the overall spectrum of the EBL between 0.1 and 1000 {$μ$}m has never been determined directly from galaxy spectral energy distribution (SED) observations over a wide redshift range. The evolving, overall spectrum of the EBL is derived here utilizing a novel method based on observations only. This is achieved from the observed evolution of the rest-frame K-band galaxy luminosity function up to redshift 4, combined with a determination of galaxy-SED-type fractions. These are based on fitting Spitzer Wide-Area Infrared Extragalactic Survey (SWIRE) templates to a multiwavelength sample of about 6000 galaxies in the redshift range from 0.2 to 1 from the All-wavelength Extended Groth Strip International Survey (AEGIS). The changing fractions of quiescent galaxies, star-forming galaxies, starburst galaxies and active galactic nucleus (AGN) galaxies in that redshift range are estimated, and two alternative extrapolations of SED types to higher redshifts are considered. This allows calculation of the evolution of the luminosity densities from the ultraviolet (UV) to the infrared (IR), the evolving star formation rate density of the Universe, the evolving contribution to the bolometric EBL from the different galaxy populations including AGN galaxies and the buildup of the EBL. Our EBL calculations are compared with those from a semi-analytic model, another observationally based model and observational data. The EBL uncertainties in our modelling based directly on the data are quantified, and their consequences for attenuation of very-high-energy {$\gamma$}-rays due to pair production on the EBL are discussed. It is concluded that the EBL is well constrained from the UV to the mid-IR, but independent efforts from IR and {$\gamma$}-ray astronomy are needed in order to reduce the uncertainties in the far-IR.},
	keywords = {cosmology: observations, diffuse radiation, galaxies: evolution, galaxies: formation, infrared: diffuse background},
	doi = {10.1111/j.1365-2966.2010.17631.x},
	url = {http://adsabs.harvard.edu/abs/2011MNRAS.410.2556D},
	author = {Dom{\'\i}nguez, A. and Primack, J.~R. and Rosario, D.~J. and Prada, F. and Gilmore, R.~C. and Faber, S.~M. and Koo, D.~C. and Somerville, R.~S. and M. A. P{\'e}rez-Torres and P. P{\'e}rez-Gonz{\'a}lez and Huang, J.-S. and Davis, M. and Guhathakurta, P. and Barmby, P. and Conselice, C.~J. and Lozano, M. and Newman, J.~A. and Cooper, M.~C.}
}
