Linking gas and galaxies at high redshift: MUSE surveys the environments of six damped Lyα systems at z ≈ 3

Ruari Mackenzie, Michele Fumagalli, Tom Theuns, David J. Hatton, Thibault Garel, Sebastiano Cantalupo, Lise Christensen, Johan P.U. Fynbo, Nissim Kanekar, Palle Møller, John O'meara, J. Xavier Prochaska, Marc Rafelski, Tom Shanks, James Trayford

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Abstract

We present results from a survey of galaxies in the fields of six z ≥ 3 damped Lyman α (Lyα) systems (DLAs) using the Multi Unit Spectroscopic Explorer (MUSE) at the Very Large Telescope (VLT). We report a high detection rate of up to ≈80 per cent≈80 per cent of galaxies within 1000 km s−1 from DLAs and with impact parameters between 25 and 280 kpc. In particular, we discovered five high-confidence Lyα emitters associated with three DLAs, plus up to nine additional detections across five of the six fields. The majority of the detections are at relatively large impact parameters (>50 kpc) with two detections being plausible host galaxies. Among our detections, we report four galaxies associated with the most metal-poor DLA in our sample (Z/Z = −2.33 ± 0.22), which trace an overdense structure resembling a filament. By comparing our detections with predictions from the Evolution and Assembly of GaLaxies and their Environments (EAGLE) cosmological simulations and a semi-analytic model designed to reproduce the observed bias of DLAs at z > 2, we conclude that our observations are consistent with a scenario in which a significant fraction of DLAs trace the neutral regions within haloes with a characteristic mass of Mh≈1011−1012 M⊙Mh≈1011−1012 M⊙⁠, in agreement with the inference made from the large-scale clustering of DLAs. We finally show how larger surveys targeting ≈25 absorbers have the potential of constraining the characteristic masses of haloes hosting high-redshift DLAs with sufficient accuracy to discriminate between different models.
Original languageEnglish
Pages (from-to)5070-5096
Number of pages27
JournalMonthly Notices of the Royal Astronomical Society
Volume487
Issue number4
Early online date4 Jun 2019
DOIs
Publication statusPublished - 1 Aug 2019

Keywords

  • galaxies: evolution
  • galaxies: formation
  • galaxies: high-redshift
  • intergalactic medium
  • quasars: absorption lines
  • UKRI
  • STFC
  • ST/P000541/1

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