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dc.contributor.authorWild, Vivienne
dc.contributor.authorTaj Aldeen, Laith
dc.contributor.authorCarnall, Adam
dc.contributor.authorMaltby, David
dc.contributor.authorAlmaini, Omar
dc.contributor.authorWerle, Ariel
dc.contributor.authorWilkinson, Aaron
dc.contributor.authorRowlands, Kate
dc.contributor.authorBolzonella, Micol
dc.contributor.authorCastellano, Marco
dc.contributor.authorGargiulo, Adriana
dc.contributor.authorMcLure, Ross
dc.contributor.authorPentericci, Laura
dc.contributor.authorPozzetti, Lucia
dc.identifier.citationWild , V , Taj Aldeen , L , Carnall , A , Maltby , D , Almaini , O , Werle , A , Wilkinson , A , Rowlands , K , Bolzonella , M , Castellano , M , Gargiulo , A , McLure , R , Pentericci , L & Pozzetti , L 2020 , ' The star formation histories of z ∼ 1 post-starburst galaxies ' , Monthly Notices of the Royal Astronomical Society , vol. 494 , no. 1 , pp. 529-548 .
dc.identifier.otherPURE: 266312495
dc.identifier.otherPURE UUID: 3dea6efd-9833-4e1a-9ae5-fb64ee699ab7
dc.identifier.otherBibCode: 2020arXiv200109154W
dc.identifier.otherBibCode: 2020MNRAS.494..529W
dc.identifier.otherScopus: 85085387414
dc.identifier.otherWOS: 000535885900041
dc.descriptionFunding: LTA acknowledges support from the Ministry of Higher Education and Scientific Research (MOHESR), Iraq. AW acknowledges financial support from the Royal Society Newton Fund (grant NAF/R1/180403, PI Natalia Vale Asari) and Fundação de à Amparo Pesquisa do Estado de São Paulo (FAPESP) process number 2019/01768-6.en
dc.description.abstractWe present the star formation histories of 39 galaxies with high-quality rest-frame optical spectra at 0.5 <z <1.3 selected to have strong Balmer absorption lines and/or Balmer break, and compare to a sample of spectroscopically selected quiescent galaxies at the same redshift. Photometric selection identifies a majority of objects that have clear evidence for a recent short-lived burst of star formation within the last 1.5 Gyr, i.e. 'post-starburst' galaxies, however we show that good quality continuum spectra are required to obtain physical parameters such as burst mass fraction and burst age. Dust attenuation appears to be the primary cause for misidentification of post-starburst galaxies, leading to contamination in spectroscopic samples where only the [O II] emission line is available, as well as a small fraction of objects lost from photometric samples. The 31 confirmed post-starburst galaxies have formed 40-90 per cent of their stellar mass in the last1-1.5 Gyr. We use the derived star formation histories to find that the post-starburst galaxies are visible photometrically for 0.5-1 Gyr. This allows us to update a previous analysis to suggest that 25-50 per cent of the growth of the red sequence at z ∼ 1 could be caused by a starburst followed by rapid quenching. We use the inferred maximum historical star formation rates of several 100-1000 M⊙yr-1 and updated visibility times to confirm that sub-mm galaxies are likely progenitors of post-starburst galaxies. The short quenching time-scales of 100-200 Myr are consistent with cosmological hydrodynamic models in which rapid quenching is caused by the mechanical expulsion of gas due to an acive galactic neucleus.
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.rightsCopyright © 2020 the Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. This work has been made available online in accordance with publisher policies or with permission. Permission for further reuse of this content should be sought from the publisher or the rights holder. This is the final published version of the work, which was originally published at
dc.subjectGalaxies: evolutionen
dc.subjectGalaxies: formationen
dc.subjectGalaxies: starbursten
dc.subjectGalaxies: stellar contenten
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.titleThe star formation histories of z ∼ 1 post-starburst galaxiesen
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.contributor.institutionUniversity of St Andrews. University of St Andrewsen
dc.description.statusPeer revieweden

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