J. Cabrera-Caño

Membrana metropolitana costera. Estrategias para proyectar una ciudad híbrida

Luisa Acosta Scandela, Juan Carlos Arismendi, J. Cabrera-Caño, Stephany Sánchez

Muchas de nuestras ciudades latinoamericanas se caracterizan por ser espacios fragmentados en continua expansión, no sólo en términos urbanos, sino también en lo social, económico y político. Tal es el caso de Maracaibo, una ciudad en el occidente venezolano cuyo borde costero …

es (code pays fourni par la source)

Stellar populations of galaxies in the ALHAMBRA survey up to z ∼ 1

L. A. Díaz-García, A. J. Cenarro, C. López-Sanjuán, Ignacio Ferreras et autres

Aims.Our aim is to determine the distribution of stellar population parameters (extinction, age, metallicity, and star formation rates) of quiescent galaxies within the rest-frame stellar mass–colour diagrams andUVJcolour–colour diagrams corrected for extinction up toz ∼ 1. These novel diagrams reduce the contamination …

tw, es, gb, br, cl (code pays fourni par la source)

VizieR Online Data Catalog: Stellar populations of quiescent galaxies (Diaz-Garcia+, 2019)

L. A. Díaz-García, A. J. Cenarro, C. López-Sanjuán, Ignacio Ferreras et autres

Stellar populations of galaxies in the ALHAMBRA survey up toz ∼ 1

L. A. Díaz-García, A. J. Cenarro, C. López-Sanjuán, Ignacio Ferreras et autres

Aims.We aim at constraining the stellar population properties of quiescent galaxies. These properties reveal how these galaxies evolved and assembled sincez ∼ 1 up to the present time. Methods.Combining the ALHAMBRA multi-filter photo-spectra with the fitting code for spectral energy distribution MUFFIT …

tw, es, gb, br, cl (code pays fourni par la source)

Stellar populations of galaxies in the ALHAMBRA survey up to z ¿ 1. III. The stellar content of the quiescent galaxy population during the last 8 Gyr

L. A. Díaz-García, A. J. Cenarro, C. López-Sanjuán, Ignacio Ferreras et autres

Aims. We aim at constraining the stellar population properties of quiescent galaxies. These properties reveal how these galaxies evolved and assembled since z similar to 1 up to the present time. Methods. Combining the ALHAMBRA multi-filter photo-spectra with the fitting code for …

tw, es, gb, br (code pays fourni par la source)

Stellar populations of galaxies in the ALHAMBRA survey up to z ~ 1. II. Stellar content of quiescent galaxies within the dust-corrected stellar mass-colour and the UVJ colour-colour diagrams

L. A. Díaz-García, A. J. Cenarro, C. López-Sanjuán, Ignacio Ferreras et autres

Aims. Our aim is to determine the distribution of stellar population parameters (extinction, age, metallicity, and star formation rates) of quiescent galaxies within the rest-frame stellar mass-colour diagrams and UVJ colour-colour diagrams corrected for extinction up to z similar to 1. These …

es (code pays fourni par la source)

High redshift galaxies in the ALHAMBRA survey

K. Viironen, C. López-Sanjuán, C. Hernández–Monteagudo, J. Chaves-Montero et autres

Context.Knowing the exact shape of the ultraviolet (UV) luminosity function (LF) of high-redshift galaxies is important to understand the star formation history of the early Universe. However, the uncertainties, especially at the faint and bright ends of the LFs, remain significant. Aims.In …

es, fr, Éthiopie, br, cl (code pays fourni par la source)

Stellar populations of galaxies in the ALHAMBRA survey up to $z \sim 1$. III. The stellar content of the quiescent galaxy population during the last $8$ Gyr

L. A. Díaz-García, A. J. Cenarro, C. López-Sanjuán, Ignacio Ferreras et autres

We aim at constraining the stellar population properties of quiescent galaxies. These properties reveal how these galaxies evolved and assembled since $z\sim1$ up to the present time. Combining the ALHAMBRA multi-filter photo-spectra with the SED-fitting code MUFFIT, we build a complete catalogue …

The ALHAMBRA survey: 2D analysis of the stellar populations in massive early-type galaxies at z < 0.3

I. San Roman, A. J. Cenarro, L. A. Díaz-García, C. López-Sanjuán et autres

We present a technique that permits the analysis of stellar population gradients in a relatively low-cost way compared to integral field unit (IFU) surveys. We developed a technique to analyze unresolved stellar populations of spatially resolved galaxies based on photometric multi-filter surveys. …

es, fr, Éthiopie, cl (code pays fourni par la source)

High redshift galaxies in the ALHAMBRA survey. II. Strengthening the evidence of bright-end excess in UV luminosity functions at 2.5 <= z<= 4.5 by PDF analysis

K. Viironen, C. López-Sanjuán, C. Hernández–Monteagudo, J. Chaves-Montero et autres

Context. Knowing the exact shape of the ultraviolet (UV) luminosity function (LF) of high-redshift galaxies is important to understand the star formation history of the early Universe. However, the uncertainties, especially at the faint and bright ends of the LFs, remain significant. …

es, fr, br (code pays fourni par la source)

Stellar populations of galaxies in the ALHAMBRA survey up to $z \sim 1$. II. Stellar populations of quiescent galaxies within the stellar mass- and the $UVJ$ colour-colour diagrams

L. A. Díaz-García, A. J. Cenarro, C. López-Sanjuán, Ignacio Ferreras et autres

We aim at discerning the distribution of stellar population parameters (extinction, age, metallicity, and sSFR) of quiescent galaxies within the rest-frame stellar mass- and $UVJ$ colour-colour diagrams up to $z\sim1$ and down to $I=23$ AB, as well as the development of new …

Stellar populations of galaxies in the ALHAMBRA survey up to $z \sim 1$. II. Stellar content of quiescent galaxies within the dust-corrected stellar mass$-$colour and the $UVJ$ colour$-$colour diagrams

L. A. Díaz-García, A. J. Cenarro, C. López-Sanjuán, Ignacio Ferreras et autres

Our aim is to determine the distribution of stellar population parameters (extinction, age, metallicity, and star formation rate) of quiescent galaxies within the rest-frame stellar mass$-$colour and $UVJ$ colour$-$colour diagrams corrected for extinction up to $z\sim1$. These novel diagrams reduce the contamination …