The MUSE Ultra Deep Field (MUDF) - I. Discovery of a group of Ly alpha nebulae associated with a bright z approximate to 3.23 quasar pair


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Date

2019-05

Publication Type

Journal Article

ETH Bibliography

yes

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Data

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 erg s⁻¹ cm⁻² arcsec⁻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.

Publication status

published

Editor

Book title

Volume

485 (1)

Pages / Article No.

Publisher

Oxford University Press

Event

Edition / version

Methods

Software

Geographic location

Date collected

Date created

Subject

galaxies: formation; galaxies: haloes; galaxies: high-redshift; intergalactic medium; quasars: general; large-scale structure of Universe

Organisational unit

03613 - Lilly, Simon (emeritus) / Lilly, Simon (emeritus) check_circle
09592 - Cantalupo, Sebastiano (ehemalig) / Cantalupo, Sebastiano (former) check_circle

Notes

It was possible to publish this article open access thanks to a Swiss National Licence with the publisher.

Funding

163824 - From Cosmic Web to Galaxies: Illuminating the Gaseous Link between the Dark and the Bright Universe (SNF)

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