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Your search keyword '"Cenarro, Javier"' showing total 4 results
Start Over Author "Cenarro, Javier" Publication Year Range Last 50 years Journal monthly notices of the royal astronomical society
4 results on '"Cenarro, Javier"'

1. The miniJPAS survey. Multiwavelength exploration of detected Extreme Emission Line Galaxies

Author

Breda, Iris, primary, Amarantidis, Stergios, additional, Vilchez, José M, additional, Pérez-Montero, Enrique, additional, Kehrig, Carolina, additional, Iglesias-Páramo, Jorge, additional, Arroyo-Polonio, Antonio, additional, Fernández-Ontiveros, Juan A, additional, Delgado, Rosa M González, additional, Díaz-García, Luis A, additional, Abramo, Raul, additional, Alcaniz, Jailson, additional, Benítez, Narciso, additional, Bonoli, Silvia, additional, Cenarro, Javier A, additional, Cristóbal-Hornillos, David, additional, Dupke, Renato, additional, Ederoclite, Alessandro, additional, Hernán-Caballero, Antonio, additional, López-Sanjuan, Carlos, additional, Marín-Franch, Antonio, additional, de Oliveira, Claudia Mendes, additional, Moles, Mariano, additional, Sodré, Laerte, additional, Taylor, Keith, additional, Varela, Jesús, additional, and Vázquez-Ramió, Héctor, additional

Published
2024
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2. Pathways to quiescence: SHARDS view on the star formation histories of massive quiescent galaxies at 1.0 < 1.5

Author

Domínguez Sánchez, Helena, primary, Pérez-González, Pablo G., additional, Esquej, Pilar, additional, Eliche-Moral, M. Carmen, additional, Barro, Guillermo, additional, Cava, Antonio, additional, Koekemoer, Anton M., additional, Alcalde Pampliega, Belén, additional, Alonso Herrero, Almudena, additional, Bruzual, Gustavo, additional, Cardiel, Nicolás, additional, Cenarro, Javier, additional, Ceverino, Daniel, additional, Charlot, Stéphane, additional, and Hernán Caballero, Antonio, additional

Published
2016
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3. SHARDS: stellar populations and star formation histories of a mass-selected sample of 0.65 < z < 1.1 galaxies

Author

Hernán-Caballero, Antonio, primary, Alonso-Herrero, Almudena, additional, Pérez-González, Pablo G., additional, Cardiel, Nicolás, additional, Cava, Antonio, additional, Ferreras, Ignacio, additional, Barro, Guillermo, additional, Tresse, Laurence, additional, Daddi, Emanuele, additional, Cenarro, Javier, additional, Conselice, Christopher J., additional, Guzmán, Rafael, additional, and Gallego, Jesús, additional

Published
2013
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4. Pathways to quiescence: SHARDS view on the star formation histories of massive quiescent galaxies at 1.0 < z < 1.5.

Author

Sánchez, Helena Domínguez, Pérez-González, Pablo G., Esquej, Pilar, Eliche-Moral, M. Carmen, Barro, Guillermo, Cava, Antonio, Koekemoer, Anton M., Pampliega, Belén Alcalde, Herrero, Almudena Alonso, Bruzual, Gustavo, Cardiel, Nicolás, Cenarro, Javier, Ceverino, Daniel, Charlot, Stéphane, and Caballero, Antonio Hernán

Subjects
STAR formation, MONTE Carlo method, GALACTIC redshift, STELLAR mass, SPECTRAL energy distribution, ULTRAVIOLET radiation, SUPERGIANT stars
Abstract

We present star formation histories (SFHs) for a sample of 104 massive (stellar mass M > 1010 M⊙) quiescent galaxies (MQGs) at z = 1.0-1.5 from the analysis of spectrophotometric data from the Survey for High-z Absorption Red and Dead Sources (SHARDS) and HST/WFC3 G102 and G141 surveys of the GOODS-North field, jointly with broad-band observations from ultraviolet (UV) to far-infrared (far-IR). The sample is constructed on the basis of rest-frame UVJ colours and specific star formation rates (sSFRs = SFR/Mass). The spectral energy distributions (SEDs) of each galaxy are compared to models assuming a delayed exponentially declining SFH. A Monte Carlo algorithm characterizes the degeneracies, which we are able to break taking advantage of the SHARDS data resolution, by measuring indices such as MgUV and D4000. The population of MQGs shows a duality in their properties. The sample is dominated (85 per cent) by galaxies with young mass-weighted ages, tM < 2 Gyr, short star formation time-scales, <τ> ~ 60-200 Myr, and masses log(M/M⊙) ~ 10.5. There is an older population (15 per cent) with tM = 2-4 Gyr, longer star formation time-scales, <τ> ~ 400 Myr, and larger masses, log(M/M⊙) ~ 10.7. The SFHs of our MQGs are consistent with the slope and the location of the main sequence of star-forming galaxies at z > 1.0, when our galaxies were 0.5-1.0 Gyr old. According to these SFHs, all the MQGs experienced a luminous infrared galaxy phase that lasts for ~500 Myr, and half of them an ultraluminous infrared galaxy phase for ~100 Myr. We find that the MQG population is almost assembled at z ~ 1, and continues evolving passively with few additions to the population. [ABSTRACT FROM AUTHOR]

Published
2016
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