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The MUSE Ultra Deep Field (MUDF). I. Discovery of a group of Lyα nebulae associated with a bright z ≈ 3.23 quasar pair

Lusso, E; Fumagalli, M; Fossati, M; Mackenzie, R; Bielby, RM; Battaia, F Arrigoni; Cantalupo, S; Cooke, R; Cristiani, S; Dayal, P; D’Odorico, V; Haardt, F; Lofthouse, E; Morris, S; Peroux, C; Prichard, L; Rafelski, M; Simcoe, R; Swinbank, M; Theuns, T

The MUSE Ultra Deep Field (MUDF). I. Discovery of a group of Lyα nebulae associated with a bright z ≈ 3.23 quasar pair Thumbnail


Authors

E Lusso

M Fossati

R Mackenzie

RM Bielby

F Arrigoni Battaia

S Cantalupo

R Cooke

S Cristiani

P Dayal

V D’Odorico

F Haardt

E Lofthouse

S Morris

C Peroux

L Prichard

M Rafelski

R Simcoe

M Swinbank



Abstract

We present first results from Multi Unit Spectroscopic Explorer (MUSE) observations at the Very Large Telescope in the MUSE Ultra Deep Field (MUDF), a ≈1.2 × 1.4 arcmin2 region for which we are collecting ≈200 hours of integral field spectroscopy. The ≈40-h observation completed to date reveals the presence of a group of three Lyα nebulae associated with a bright quasar pair at z ≃ 3.23 with projected separation of ≈500 kpc⁠. Two of the nebulae are physically associated with the quasars which are likely powering the Lyα emission, and extend for ≳100 kpc at a surface brightness level of ≈6 × 10−19 ergs−1cm−2arcsec−2⁠. A third smaller (≈35 kpc) nebula lies at a velocity offset of ≈1550 km s−1. Despite their clustered nature, the two large nebulae have properties similar to those observed in isolated quasars and exhibit no sharp decline in flux at the current depth, suggesting an even more extended distribution of gas around the quasars. We interpret the shape and the alignment of the two brighter nebulae as suggestive of the presence of an extended structure connecting the two quasar host galaxies, as seen for massive galaxies forming within gas-rich filaments in cosmological simulations.

Citation

Lusso, E., Fumagalli, M., Fossati, M., Mackenzie, R., Bielby, R., Battaia, F. A., …Theuns, T. (2019). The MUSE Ultra Deep Field (MUDF). I. Discovery of a group of Lyα nebulae associated with a bright z ≈ 3.23 quasar pair. Monthly Notices of the Royal Astronomical Society: Letters, 485(1), L62-L67. https://doi.org/10.1093/mnrasl/slz032

Journal Article Type Article
Acceptance Date Mar 1, 2019
Online Publication Date Mar 7, 2019
Publication Date May 31, 2019
Deposit Date Mar 27, 2019
Publicly Available Date Mar 28, 2024
Journal Monthly Notices of the Royal Astronomical Society: Letters
Electronic ISSN 1745-3933
Publisher Oxford University Press
Peer Reviewed Peer Reviewed
Volume 485
Issue 1
Pages L62-L67
DOI https://doi.org/10.1093/mnrasl/slz032

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Copyright Statement
© 2019 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society.





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