Información del autor
Autor Gallego Maestro, Jesús |
Documentos disponibles escritos por este autor (176)
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López Sanjuan, C. ; Balcells, M. ; Pérez González, Pablo Guillermo ; Barro, Guillermo ; García Dabó, C. E. ; Gallego Maestro, Jesús ; Zamorano Calvo, Jaime | EDP Sciencies | 2009-07Aims. The importance of disc-disc major mergers in galaxy evolution remains uncertain. We study the major merger fraction in a SPITZER/IRAC-selected catalogue in the GOODS-S field up to z ~ 1 for luminosity- and mass-limited samples. Methods. We[...]texto impreso
Bouquin, Alexandre Y. K. ; Gil de Paz, Armando ; Muñoz Mateos, Juan Carlos ; Boissier, Samuel ; Sheth, Kartik ; Zaritsky, Dennis ; Peletier, Reynier F. ; Knapen, Johan H. ; Gallego Maestro, Jesús | University Chicago Press | 2018-02We present new spatially resolved surface photometry in the far-ultraviolet (FUV) and near-ultraviolet (NUV) from images obtained by the Galaxy Evolution Explorer (GALEX) and IRAC1 (3.6 mu m) photometry from the Spitzer Survey of Stellar Structu[...]texto impreso
Bouquin, Alexandre Y. K. ; Gil de Paz, Armando ; Boissier, Samuel ; Muñoz Mateos, Juan Carlos ; Sheth, Kartik ; Zaritsky, Dennis ; Laine, Jarkko ; Gallego Maestro, Jesús ; Peletier, Reynier F. ; Roeck, Benjamin R. ; Knapen, Johan H. | IOP Publishing | 2015-02-10We obtained GALEX FUV, NUV, and Spitzer/ IRAC 3.6 ?m photometry for > 2000 galaxies, available for 90% of the S^(4)G sample. We find a very tight. GALEX blue sequence (GBS) in the (FUV- NUV) versus (NUV-[3.6]) color- color diagram, which is pop[...]texto impreso
Pisano, D. J. ; Kobulnicky, Henry A. ; Guzmán, Rafael ; Gallego Maestro, Jesús ; Bershady, Matthew A. | IOP publishing ltd | 2001-09We present Arecibo 21 cm spectroscopy, Keck HIRES H? spectroscopy, and WIYN R-band imaging of 11 nearby blue compact galaxies with effective B-band surface brightnesses of SBe = 19.4–21.2 mag arcsec^2 and effective radii of R_ eff = 0.6–1.9 kpc.[...]texto impreso
Villar, Víctor ; Gallego Maestro, Jesús ; Pérez González, Pablo Guillermo ; Pascual, Sergio ; Noeske, Kai ; Koo, David C. ; Barro, Guillermo ; Zamorano Calvo, Jaime | American Astronomical Society | 2008-04-10We present the results of an H? near-infrared narrowband survey searching for star-forming galaxies at redshift z = 0.84. This work is an extension of our previous narrowband studies in the optical at lower redshifts. After removal of stars and [...]texto impreso
Villar, V. ; Gallego Maestro, Jesús ; Pascual Ramírez, Sergio ; Zamorano Calvo, Jaime ; Noeske, K. ; Koo, D.C. | Instituto de Astronomía de la UNAM. Universidad Nacional Autónoma de México | 2007We presen there the results of a survey searching for current-star forming galaxies at at z ?0.83. Objects are selected by their emission in the H? line through the narrow band filter technique.texto impreso
López Sanjuan, Carlos ; Balcells, Marc ; Pérez González, Pablo Guillermo ; Barro, Guillermo ; García Dabó, César Enrique ; Gallego Maestro, Jesús ; Zamorano Calvo, Jaime | American Astronomical Society | 2010-02-20We study the evolution of galaxy structure since z ~ 1 to the present. From a Great Observatories Origins Deep Survey South (GOODS-S) multi-band catalog, we define (blue) luminosity- and mass-weighted samples, limited by MB ? –20 and M sstarf ?[...]texto impreso
Sánchez de Miguel, Alejandro ; Kyba, Christopher C. M. ; Zamorano Calvo, Jaime ; Gallego Maestro, Jesús ; Gaston, Kevin J. | Nature Publishing Group | 2020-05-08Difuse glow has been observed around brightly lit cities in nighttime satellite imagery since at least the frst publication of large scale maps in the late 1990s. In the literature, this has often been assumed to be an error related to the senso[...]texto impreso
Gallego Maestro, Jesús ; García Dabó, C. E. ; Zamorano Calvo, Jaime ; Aragón Salamanca, A. ; Rego Fernández, Manuel | American Astronomical Society | 2002-05-01The measurement of the star formation rate density of the universe is of prime importance in understanding the formation and evolution of galaxies. The [O II] ?3727 emission-line flux, easy to measure up to z ? 1.4 within deep redshift surveys i[...]texto impreso
Gallego Maestro, Jesús ; García Dabó, C. E. ; Zamorano Calvo, Jaime ; Aragón Salamanca, A. ; Rego Fernández, Manuel | Univ. Chicago Press | 2002-05-01The measurement of the star formation rate density of the universe is of prime importance in understanding the formation and evolution of galaxies. The [O ii] ?3727 emission-line flux, easy to measure up to z ? 1.4 within deep redshift surveys i[...]texto impreso
Context. The OSIRIS Tunable Filter Emission Line Object (OTELO) survey is a very deep, blind exploration of a selected region of the Extended Groth Strip and is designed for finding emission-line sources (ELSs). The survey design, observations, [...]texto impreso
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Context. The evolution of galaxies through cosmic time is studied observationally by means of extragalactic surveys. The usefulness of these surveys is greatly improved by increasing the cosmological volume, in either depth or area, and by obser[...]texto impreso
Ramón-Pérez, Marina ; Bongiovanni, Ángel ; Pérez García, Ana María ; Cepa, Jordi ; Nadolny, Jakup ; Pintos-Castro, Irene ; Lara-López, Maritza A. ; Alfaro, Emilio J. ; Castañeda, Héctor O. ; Cerviño, Miguel ; Diego, José A. ; Fernández-Lorenzo, Mirian ; Gallego Maestro, Jesús ; González, J. Jesús ; González-Serrano, J. Ignacio ; Oteo Gómez, Iván ; Pérez Martínez, Ricardo ; Povic, Mirjana ; Sánchez-Portal, Miguel | EDP Sciencies | 2019-10-14Aims. We take advantage of the capability of the OTELO survey to obtain the H? luminosity function (LF) at z ? 0.40. Because of the deepest coverage of OTELO, we are able to determine the faint end of the LF, and thus better constrain the star f[...]texto impreso
Ramón-Pérez, Marina ; Bongiovanni, Ángel ; Pérez García, Ana María ; Cepa, Jordi ; Nadolny, Jakup ; Pintos-Castro, Irene ; Lara-López, Maritza A. ; Alfaro, Emilio J. ; Castañeda, Héctor O. ; Cerviño, Miguel ; Diego, José A. ; Fernández-Lorenzo, Mirian ; Gallego Maestro, Jesús ; González, J. Jesús ; González-Serrano, J. Ignacio ; Oteo Gómez, Iván ; Pérez Martínez, Ricardo ; Povic, Mirjana ; Sánchez-Portal, Miguel | EDP Sciencies | 2019-10-14Aims. We take advantage of the capabilities of the OSIRIS Tunable Emission Line Object (OTELO) survey to select and study the AGN population in the field. In particular, we aim to perform an analysis of the properties of these objects, including[...]texto impreso
Pérez González, Pablo Guillermo ; Rieke, George H.;, George H. ; Villar, Víctor ; Barro, Guillermo ; Blaylock, Myra ; Egami, Eiichi ; Gallego Maestro, Jesús ; Gil de Paz, Armando ; Pascual, Sergio ; Zamorano Calvo, Jaime ; Donley, Jennifer L. | American Astronomical Society | 2008-03-01Using a sample of ~28,000 sources selected at 3.6-4.5 ?m with Spitzer observations of the Hubble Deep Field North, the Chandra Deep Field South, and the Lockman Hole (surveyed area ~664 arcmin^2), we study the evolution of the stellar mass conte[...]texto impreso
Klose, S. ; Henden, A. A. ; Greiner, J. ; Hartmann, D. H. ; Cardiel López, Nicolás ; Castro Tirado, A. J. ; Cerón, J. M. C. ; Gallego Maestro, Jesús ; Gorosabel, J. ; Stecklum, B. ; Tanvir, N. ; Thiele, U. ; Vrba, F. J. ; Zeh, A. | IOP Publishing | 2003-08-01We report rapid follow-up K'-band observations of the error box of the bright High Energy Transient Explorer burst GRB 020819. We find that any afterglow was fainter than K' = 19 only 9 hr after the burst. Because no optical afterglow was found,[...]texto impreso
Pelló, R. ; Hudelot, P. ; Laporte, N. ; Mellier, Y. ; McCraken, H.J. ; Balcells, M. ; Boone, F. ; Cardiel López, Nicolás ; Gallego Maestro, Jesús ; Garzón, F. ; Guzmán, R.G. ; Le Borgne, J.F. ; Prieto, M. ; Richard, J. ; Schaerer, D. ; Tresse, L. ; Arnouts, S. ; Cuby, J.G. ; Disseau, K. ; Hayes, M. | EDP SCIENCES S A | 2018-11-29The aim of this paper is to introduce the WIRCam Ultra Deep Survey (WUDS), a near-IR photometric survey carried out at the CFH Telescope in the field of the CFHTLS-D3 field (Groth Strip). WUDS includes four near-IR bands (Y, J, H and Ks) over a [...]texto impreso
Pérez Gallego, J. ; Guzmán, R. ; Castillo Morales, África ; Gallego Maestro, Jesús ; Castander, F. J. ; Garland, C. A. ; Gruel, N. ; Pisano, D. J. ; Zamorano Calvo, Jaime | Wiley | 2011-12We use three-dimensional optical spectroscopy observations of a sample of 22 local luminous compact blue galaxies (LCBGs) to create kinematic maps. By means of these, we classify the kinematics of these galaxies into three different classes: rot[...]texto impreso
Zamorano Calvo, Jaime ; Gallego Maestro, Jesús ; Rego Fernández, Manuel ; Vitores, A. G. ; González Riestra, R. | IOP publishing ltd | 1992-09Multiwavelength observations of the galaxy UCM 2257+2438 found in the Universidad Complutense of Madrid (UCM) objective-prism survey are reported. The optic spectroscopy, CCD imaging, near-infrared and IRAS photometric data suggest that this obj[...]texto impreso
Rego Fernández, Manuel ; Cordero Gracia, M. ; Gallego Maestro, Jesús ; Zamorano Calvo, Jaime | EDP Sciencies | 1998-02UCM1612+1308 is a new emission-line galaxy identified in the context of the Universidad Complutense de Madrid (UCM) survey. This object was classified as Blue Compact Galaxy (BCG) from photometric data. A detailed spectroscopic study from new op[...]texto impreso
Barro, Guillermo ; Pérez González, Pablo Guillermo ; Gallego Maestro, Jesús ; Ashby, M. L. N. ; Kajisawa, M. ; Miyazaki, S. ; Villar, V. ; Yamada, T. ; Zamorano, J. | University Chicago Press | 2011-03We present an IRAC 3.6+4.5 ?m selected catalog in the Extended Groth Strip (EGS) containing photometry from the ultraviolet to the far-infrared and stellar parameters derived from the analysis of the multi-wavelength data. In this paper, we desc[...]texto impreso
Barro, Guillermo ; Pérez González, Pablo Guillermo ; Gallego Maestro, Jesús ; Ashby, M. L. N. ; Kajisawa, M. ; Miyazaki, S. ; Villar, V. ; Yamada, T. ; Zamorano Calvo, Jaime | University Chicago Press | 2011-04Based on the ultraviolet to far-infrared photometry already compiled and presented in a companion paper (Paper I), we present a detailed spectral energy distribution (SED) analysis of nearly 80,000 IRAC 3.6 + 4.5 ? m selected galaxies in the Ext[...]texto impreso
We present Gran-Telescopio-Canarias/OSIRIS optical spectra of four of the most compact and massive early-type galaxies (ETGs) in the Groth Strip Survey at redshift z ~ 1, with effective radii R e = 0.5-2.4 kpc and photometric stellar masses M [...]texto impreso
García Vargas, M. L. ; Pérez Calpena, A. ; Gallego Maestro, Jesús ; Gil de Paz, Armando ; Sánchez Blanco, E. ; Martínez Delgado, I. ; Maldonado Medina, M. ; Zamorano Calvo, Jaime | Spie-Int Soc Optical Engineering | 2012The goal of VIENTOS project is to analyze pupil innovative systems that could be used in the new generation of instruments for the large telescopes. This study tries to identify the current scientific needs, to understand why some of them have n[...]texto impreso
Luminosity functions are one of the most important observational clues when studying galaxy evolution over cosmic time. In this paper we present the X-ray luminosity functions for X-ray detected AGN in the SXDS and GWS fields. The limiting fluxe[...]