1. European Southern Observatory, Karl-Schwarzschild-Strae 2, D-85748 Garching bei München, Germany
2. Institute of Physics and Astronomy, University of Aarhus, Ny Munkegade, DK-8000 Århus C, Denmark
3. Astronomical Observatory, University of Copenhagen, Juliane Maries Vej 30, DK-2100 Copenhagen Ø, Denmark

Correspondence to: Michael Weidinger^1,2 Email: mweiding@eso.org

Abstract

Quasars are the visible signatures of gas falling into the deep potential well of super-massive black holes in the centres of distant galaxies. It has been suggested¹ that quasars are formed when two massive galaxies collide and merge, leading to the prediction that quasars should be found in the centres of regions of largest overdensity in the early Universe. In dark matter (DM)-dominated models of the early Universe, massive DM halos are predicted to attract the surrounding gas, which falls towards their centres. The neutral gas is not detectable in emission by itself, but gas falling into the ionizing cone of such a quasar will glow in the Lyman- line of hydrogen, effectively imaging the DM halo². Here we present a Ly image of a DM halo at redshift z = 3, along with a two-dimensional spectrum of the gaseous halo. Our observations are best understood in the context of the standard model for DM haloes³; we infer a mass of (2 - 7) 10¹² solar masses (M) for the halo.

1. European Southern Observatory, Karl-Schwarzschild-Strae 2, D-85748 Garching bei München, Germany
2. Institute of Physics and Astronomy, University of Aarhus, Ny Munkegade, DK-8000 Århus C, Denmark
3. Astronomical Observatory, University of Copenhagen, Juliane Maries Vej 30, DK-2100 Copenhagen Ø, Denmark

Correspondence to: Michael Weidinger^1,2 Email: mweiding@eso.org

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