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Stellar populations of over one 1000 z ∼ 0.8 galaxies from LEGA-C : ages and star formation histories from Dn4000 and Hδ

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Date
12/03/2018
Author
Wu, Po-Feng
van der Wel, Arjen
Gallazzi, Anna
Bezanson, Rachel
Pacifici, Camilla
Straatman, Caroline
Franx, Marijn
Barišić, Ivana
Bell, Eric F.
Brammer, Gabriel B.
Calhau, Joao
Chauke, Priscilla
van Houdt, Josha
Maseda, Michael V.
Muzzin, Adam
Rix, Hans-Walter
Sobral, David
Spilker, Justin
van de Sande, Jesse
van Dokkum, Pieter
Wild, Vivienne
Keywords
Galaxies: evolution
Galaxies: high-redshift
Galaxies: stellar content
QB Astronomy
QC Physics
NDAS
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Abstract
Drawing from the LEGA-C data set, we present the spectroscopic view of the stellar population across a large volume- and mass-selected sample of galaxies at large look-back time. We measure the 4000Å break (Dn4000) and Balmer absorption line strengths (probed by Hδ) from 1019 high-quality spectra of z = 0.6−1.0 galaxies with M∗ = 2 x 1010M⊙−3×1011M⊙. Our analysis serves as a first illustration of the power of high-resolution, high-S/N continuum spectroscopy at intermediate redshifts as a qualitatively new tool to constrain galaxy formation models. The observed Dn4000-EW(Hδ) distribution of our sample overlaps with the distribution traced by present-day galaxies, but z∼0.8 galaxies populate that locus in a fundamentally different manner. While old galaxies dominate the present-day population at all stellar masses > 2 x 1010M⊙, we see a bimodal Dn4000-EW(Hδ) distribution at z∼0.8, implying a bimodal light-weighted age distribution. The light-weighted age depends strongly on stellar mass, with the most massive galaxies > 1 x 1011M⊙ being almost all older than 2 Gyr. At the same time we estimate that galaxies in this high mass range are only ∼3 Gyr younger than their z∼0.1 counterparts, at odd with pure passive evolution given a difference in lookback time of > 5 Gyr; younger galaxies must grow to > 1011M⊙ in the meantime, and/or small amounts of young stars must keep the light-weighted ages young. Star-forming galaxies at z ∼ 0.8 have stronger Hδ absorption than present-day galaxies with the same Dn4000, implying larger short-term variations in star-formation activity.
Citation
Wu , P-F , van der Wel , A , Gallazzi , A , Bezanson , R , Pacifici , C , Straatman , C , Franx , M , Barišić , I , Bell , E F , Brammer , G B , Calhau , J , Chauke , P , van Houdt , J , Maseda , M V , Muzzin , A , Rix , H-W , Sobral , D , Spilker , J , van de Sande , J , van Dokkum , P & Wild , V 2018 , ' Stellar populations of over one 1000 z ∼ 0.8 galaxies from LEGA-C : ages and star formation histories from D n 4000 and Hδ ' , Astrophysical Journal , vol. 855 , no. 2 , 85 . https://doi.org/10.3847/1538-4357/aab0a6
Publication
Astrophysical Journal
Status
Peer reviewed
DOI
https://doi.org/10.3847/1538-4357/aab0a6
ISSN
0004-637X
Type
Journal article
Rights
© 2018 The American Astronomical Society. All rights reserved. This work is made available online in accordance with the publisher’s policies. This is the final published version of the work, which was originally published at: https://doi.org/10.3847/1538-4357/aab0a6
Description
Funding: VW acknowledges funding from the ERC (starting grant SEDmorph, PI. Wild).
Collections
  • University of St Andrews Research
URL
http://adsabs.harvard.edu/abs/2018arXiv180206799W
URI
http://hdl.handle.net/10023/13048

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