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

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    Identificadores
    URI: http://hdl.handle.net/10902/4806
    DOI: 10.1093/mnras/stt1165
    ISSN: 0035-8711
    ISSN: 1365-2966
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    Autoría
    Hernán Caballero, Antonio; Alonso Herrero, Almudena; Pérez-González, Pablo G.; Cardiel, Nicolás; Cava, Antonio; Ferreras, Ignacio; Barro, Guillermo; Tresse, Laurence; Daddi, Emanuele; Cenarro, Javier; Conselice, Christopher J.; Guzmán, Rafael; Gallego, Jesús
    Fecha
    2013-09
    Derechos
    © 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
    Publicado en
    Monthly Notices of the Royal Astronomical Society, vol. 434, iss.3, Pp.2136-2152 (2013)
    Editorial
    Oxford University Press
    Royal Astronomical Society
    Enlace a la publicación
    http://dx.doi.org/10.1093/mnras/stt1165
    Palabras clave
    Galaxies: evolution
    Galaxies: fundamental parameters
    Galaxies: high-redshift
    Galaxies: statistics
    Galaxies: stellar content
    Infrared: galaxies
    Resumen/Abstract
    We report on results from the analysis of a stellar mass-selected (log (M*/M⊙) ≥ 9.0) sample of 1644 galaxies at 0.65 < z < 1.1 with ultradeep (mAB < 26.5) optical medium-band (R ∼ 50) photometry from the Survey for High-z Absorption Red and Dead Sources (SHARDS). The spectral resolution of SHARDS allows us to consistently measure the strength of the 4000 Å spectral break [Dn(4000), an excellent age indicator for the stellar populations of quiescent galaxies] for all galaxies at z ∼ 0.9 down to log (M*/M⊙) ∼ 9. The Dn(4000) index cannot be resolved from broad-band photometry, and measurements from optical spectroscopic surveys are typically limited to galaxies at least 10 times more massive. When combined with the rest-frame U − V colour, (U − V)r, Dn(4000) provides a powerful diagnostic of the extinction affecting the stellar population that is relatively insensitive to degeneracies with age, metallicity or star formation history. We use this novel approach to estimate de-reddened colours and light-weighted stellar ages for individual sources. We explore the relationships linking stellar mass, (U − V)r, and Dn(4000) for the sources in the sample, and compare them to those found in local galaxies. The main results are: (a) both Dn(4000) and (U − V)r correlate with M*. The dispersion in Dn(4000) values at a given M* increases with M*, while the dispersion for (U − V)r decreases due to the higher average extinction prevalent in massive star-forming galaxies. (b) For massive galaxies, we find a smooth transition between the blue cloud and red sequence in the intrinsic U − V colour, in contrast with other recent results. (c) At a fixed stellar age, we find a positive correlation between extinction and stellar mass. (d) The fraction of sources with declining or halted star formation increases steeply with the stellar mass, from ∼5 per cent at log (M*/M⊙) = 9.0–9.5 to ∼80 per cent at log (M*/M⊙) > 11, in agreement with downsizing scenarios.
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    UNIVERSIDAD DE CANTABRIA

    Repositorio realizado por la Biblioteca Universitaria utilizando DSpace software
    Contacto | Sugerencias
    Metadatos sujetos a:licencia de Creative Commons Reconocimiento 4.0 España