SIBELIUS-DARK: a galaxy catalogue of the local volume from a constrained realization simulation. Issue 4 (8th February 2022)

• Record Type: Journal Article
• Authors: McAlpine, Stuart; Helly, John C; Schaller, Matthieu; Sawala, Till; Lavaux, Guilhem; Jasche, Jens; Frenk, Carlos S; Jenkins, Adrian; Lucey, John R; Johansson, Peter H
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 512:Issue 4(2022)
• Page Start: 5823
• Page End: 5847
• Publication Date: 2022-02-08
• Subjects: methods: numerical -- galaxies: formation -- cosmology: theory -- dark matter -- large-scale structure of Universe; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/stac295
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: We present sibelius-dark, a constrained realization simulation of the local volume to a distance of 200 Mpc from the Milky Way. sibelius-dark is the first study of the ' Simulations Beyond The Local Universe ' (sibelius ) project, which has the goal of embedding a model Local Group-like system within the correct cosmic environment. The simulation is dark-matter-only, with the galaxy population calculated using the semi-analytic model of galaxy formation, galform . We demonstrate that the large-scale structure that emerges from the sibelius constrained initial conditions matches well the observational data. The inferred galaxy population of sibelius-dark also match well the observational data, both statistically for the whole volume and on an object-by-object basis for the most massive clusters. For example, the K -band number counts across the whole sky, and when divided between the northern and southern Galactic hemispheres, are well reproduced by sibelius-dark . We find that the local volume is somewhat unusual in the wider context of ΛCDM: it contains an abnormally high number of supermassive clusters, as well as an overall large-scale underdensity at the level of ≈5 per cent relative to the cosmic mean. However, whilst rare, the extent of these peculiarities does not significantly challenge the ΛCDM model. sibelius-dark is the most comprehensive constrained realization simulation of the local volume to date, and with this paper we publicly release the halo and galaxy catalogues at z = 0, which we hope will be useful to the wider astronomy community.