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The NIRVANDELS Survey: a robust detection of α-enhancement in star-forming galaxies at z ≃ 3.4

  • F. Cullen*
  • , A. E. Shapley
  • , R. J. McLure
  • , J. S. Dunlop
  • , R. L. Sanders
  • , M. W. Topping
  • , N. A. Reddy
  • , R. Amorin
  • , R. Begley
  • , M. Bolzonella
  • , A. Calabro
  • , A. C. Carnall
  • , M. Castellano
  • , A. Cimatti
  • , M Cirasuolo
  • , G. Cresci
  • , A. Fontana
  • , F. Fontanot
  • , B. Garilli
  • , L. Guaita
  • M. Hamadouche, N. P. Hathi, F. Mannucci, D. J. McLeod, L. Pentericci, A. Saxena, M. Talia, G. Zamorani
*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

Abstract

We present results from the NIRVANDELS survey on the gas-phase metallicity (Zg, tracing O/H) and stellar metallicity (Z, tracing Fe/H) of 33 star-forming galaxies at redshifts 2.95 < z < 3.80. Based on a combined analysis of deep optical and near-IR spectra, tracing the rest-frame far-ultraviolet (FUV; 1200–2000 Å) and rest-frame optical (3400–5500 Å), respectively, we present the first simultaneous determination of the stellar and gas-phase mass–metallicity relationships (MZRs) at z ≃ 3.4. In both cases, we find that metallicity increases with increasing stellar mass (M) and that the power-law slope at M ≲ 1010M of both MZRs scales as Z∝M0.3⋆⁠. Comparing the stellar and gas-phase MZRs, we present direct evidence for super-solar O/Fe ratios (i.e. α-enhancement) at z > 3, finding (O/Fe) = 2.54 ± 0.38 × (O/Fe), with no clear dependence on M.
Original languageEnglish
Pages (from-to)903-920
Number of pages18
JournalMonthly Notices of the Royal Astronomical Society
Volume505
Issue number1
Early online date12 May 2021
DOIs
Publication statusPublished - 1 Jul 2021

Keywords / Materials (for Non-textual outputs)

  • astro-ph.GA

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