4.6 Article

The extended ROSAT-ESO Flux-Limited X-ray Galaxy Cluster Survey (REFLEX II) V. Exploring a local underdensity in the southern sky

期刊

ASTRONOMY & ASTROPHYSICS
卷 574, 期 -, 页码 -

出版社

EDP SCIENCES S A
DOI: 10.1051/0004-6361/201424817

关键词

galaxies: clusters: general; X-rays: galaxies: clusters; cosmology: observations; large-scale structure of Universe

资金

  1. DFG Transregio Program [TR33]
  2. Munich Excellence Cluster Structure and Evolution of the Universe
  3. DLR [50 OR 1305]
  4. STFC
  5. ARI [ST/J001465/1]
  6. STFC [ST/J001465/1] Funding Source: UKRI
  7. Science and Technology Facilities Council [ST/J001465/1] Funding Source: researchfish

向作者/读者索取更多资源

Several claims have been made that we are located in a locally underdense region of the Universe based on observations of supernovae and galaxy density distributions. Two recent studies of K-band galaxy surveys have, in particular, provided new support for a local underdensity in the galaxy distribution out to distances of 200-300 Mpc. If confirmed, such local underdensities would have important implications interpreting local measurements of cosmological parameters. Galaxy clusters have been shown to be ideal probes for tracing the large-scale structure of the Universe. In this paper we study the local density distribution in the southern sky with the X-ray detected galaxy clusters from the REFLEX II cluster survey. From the normalised comoving number density of clusters, we find an average underdensity of similar to 30-40% in the redshift range out to z similar to 0.04 (similar to 170 Mpc) in the southern extragalactic sky with a significance greater than 3.4 sigma. On larger scales from 300 Mpc to over 1 Gpc, the density distribution appears remarkably homogeneous. The local underdensity seems to be dominated by the south Galactic cap region. A comparison of the cluster distribution with that of galaxies in the K-band from a recent study shows that galaxies and clusters trace each other very closely in density. In the south Galactic cap region both surveys find a local underdensity in the redshift range z = 0 to 0.05 and no significant underdensity in the north Galactic cap at southern latitudes. Cosmological models that attempt to interpret the cosmic acceleration, deduced from observations of type Ia supernovae, by a large local void without the need for reacceleration, require that we are located close to the centre of a roughly spherical void with a minimum size of similar to 300 Mpc. In contrast our results show that the local underdensity is not isotropic and limited to a size significantly smaller than 300 Mpc radius.

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