The vandels survey: The star-formation histories of massive quiescent galaxies at 1.0 < z < 1.3

dc.contributor.authorDavé, Romeel
dc.contributor.authorCarnall, A. C.
dc.contributor.authorMcLure, R. J.
dc.date.accessioned2023-01-12T07:38:18Z
dc.date.available2023-01-12T07:38:18Z
dc.date.issued2019
dc.description.abstractWe present a Bayesian full-spectral-fitting analysis of 75 massive (⁠M∗>1010.3M⊙⁠) UVJ-selected galaxies at redshifts of 1.0 < z < 1.3, combining extremely deep rest-frame ultraviolet spectroscopy from VANDELS with multiwavelength photometry. By the use of a sophisticated physical plus systematic uncertainties model, constructed within the BAGPIPES code, we place strong constraints on the star-formation histories (SFHs) of individual objects. We first constrain the stellar mass versus stellar age relationship, finding a steep trend towards earlier average formation time with increasing stellar mass (downsizing) of 1.48+0.34−0.39 Gyr per decade in mass, although this shows signs of flattening at M∗>1011M⊙⁠en_US
dc.identifier.citationCarnall, A. C. et al. (2019). The vandels survey: The star-formation histories of massive quiescent galaxies at 1.0 < z < 1.3. Monthly Notices of the Royal Astronomical Society, 490(1), 417–439. https://doi.org/10.1093/mnras/stz2544en_US
dc.identifier.issn2331-8422
dc.identifier.urihttp://hdl.handle.net/10566/8298
dc.language.isoen_USen_US
dc.publisherOxford Academicsen_US
dc.subjectmethods: statisticalen_US
dc.subjectgalaxies: star formationen_US
dc.subjectgalaxies: evolutionen_US
dc.subjectAstrophysicsen_US
dc.subjectAstronomyen_US
dc.titleThe vandels survey: The star-formation histories of massive quiescent galaxies at 1.0 < z < 1.3en_US
dc.typeArticleen_US

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