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Ubiquitous giant Lyα nebulae around the brightest quasars at z ∼ 3.5 revealed with MUSE

Journal Article · · Astrophysical Journal
; ; ; ; ;  [1]; ; ; ;  [2]; ;  [3]; ; ;  [4];  [5]; ; ;  [6]
  1. Institute for Astronomy, ETH Zurich, Wolfgang-Pauli-Strasse 27, 8093 Zurich (Switzerland)
  2. Univ Lyon, Univ Lyon1, Ens de Lyon, CNRS, Centre de Recherche Astrophysique de Lyon UMR5574, F-69230, Saint-Genis-Laval (France)
  3. Institut de Recherche en Astrophysique et Planétologie (IRAP), CNRS, 9 Avenue Colonel Roche, F-31400 Toulouse (France)
  4. Leiden Observatory, Leiden University, P.O. Box 9513, 2300 RA Leiden (Netherlands)
  5. Department of Physics, University of Malta, Msida MSD 2080 (Malta)
  6. Leibniz-Institut für Astrophysik Potsdam (AIP), An der Sternwarte 16, D-14482 Potsdam (Germany)
Direct Lyα imaging of intergalactic gas at z∼2 has recently revealed giant cosmological structures around quasars, e.g., the Slug Nebula. Despite their high luminosity, the detection rate of such systems in narrow-band and spectroscopic surveys is less than 10%, possibly encoding crucial information on the distribution of gas around quasars and the quasar emission properties. In this study, we use the MUSE integral-field instrument to perform a blind survey for giant Lyα nebulae around 17 bright radio-quiet quasars at 3
OSTI ID:
22868534
Journal Information:
Astrophysical Journal, Journal Name: Astrophysical Journal Journal Issue: 1 Vol. 831; ISSN ASJOAB; ISSN 0004-637X
Country of Publication:
United States
Language:
English

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