dc.contributor.author | Hernán Caballero, Antonio | |
dc.contributor.author | Alonso Herrero, Almudena | |
dc.contributor.author | Pérez-González, Pablo G. | |
dc.contributor.author | Cardiel, Nicolás | |
dc.contributor.author | Cava, Antonio | |
dc.contributor.author | Ferreras, Ignacio | |
dc.contributor.author | Barro, Guillermo | |
dc.contributor.author | Tresse, Laurence | |
dc.contributor.author | Daddi, Emanuele | |
dc.contributor.author | Cenarro, Javier | |
dc.contributor.author | Conselice, Christopher J. | |
dc.contributor.author | Guzmán, Rafael | |
dc.contributor.author | Gallego, Jesús | |
dc.contributor.other | Universidad de Cantabria | es_ES |
dc.date.accessioned | 2014-06-10T13:13:11Z | |
dc.date.available | 2014-06-10T13:13:11Z | |
dc.date.issued | 2013-09 | |
dc.identifier.issn | 0035-8711 | |
dc.identifier.issn | 1365-2966 | |
dc.identifier.uri | http://hdl.handle.net/10902/4806 | |
dc.description.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. | es_ES |
dc.format.extent | 17 p. | es_ES |
dc.language.iso | eng | es_ES |
dc.publisher | Oxford University Press | es_ES |
dc.publisher | Royal Astronomical Society | es_ES |
dc.rights | © 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society | * |
dc.source | Monthly Notices of the Royal Astronomical Society, vol. 434, iss.3, Pp.2136-2152 (2013) | es_ES |
dc.subject.other | Galaxies: evolution | es_ES |
dc.subject.other | Galaxies: fundamental parameters | es_ES |
dc.subject.other | Galaxies: high-redshift | es_ES |
dc.subject.other | Galaxies: statistics | es_ES |
dc.subject.other | Galaxies: stellar content | es_ES |
dc.subject.other | Infrared: galaxies | es_ES |
dc.title | SHARDS: stellar populations and star formation histories of a mass-selected sample of 0.65 < z < 1.1 galaxies | es_ES |
dc.type | info:eu-repo/semantics/article | es_ES |
dc.relation.publisherVersion | http://dx.doi.org/10.1093/mnras/stt1165 | es_ES |
dc.rights.accessRights | openAccess | es_ES |
dc.identifier.DOI | 10.1093/mnras/stt1165 | |
dc.type.version | publishedVersion | es_ES |