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Autor Gallego Maestro, Jesús |
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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[...]