Volume 430, Number 1, January IV 2005
|Page(s)||39 - 45|
|Section||Cosmology (including clusters of galaxies)|
|Published online||12 January 2005|
X-ray source overdensities in Chandra distant cluster fields: A new probe to map the cosmic tapestry?
IASF - CNR, Sezione di Bologna, Via Gobetti 101, 40129 Bologna, Italy e-mail: firstname.lastname@example.org
2 Dipartimento di Astronomia Università di Bologna, via Ranzani 1, 40127 Bologna, Italy
3 IRA - CNR, via Gobetti 101, 40129 Bologna, Italy
4 INAF - Osservatorio astronomico di Roma, via di Frascati, 33 00040 Monteporzio Catone, Rome, Italy
Accepted: 8 September 2004
The first systematic study of the serendipitous X-ray source density around 10 high z (0.24 < z < 1.2) clusters has been performed with Chandra. A factor ~2 overdensity has been found in 4 cluster fields, increasing to 11 the number of known source overdensities around high z clusters. The result is statistically highly significant (at >2σ per field, and >5σ overall) only on scales 8′ 8′ and peculiar to cluster fields. The blank field fluctuations, i.e. the most sensitive measurements to date of the X-ray cosmic variance on this scale, indicate 1σ variations within ~15–25% around the average value. The first marginal evidence that these overdensities increase with cluster redshift is also presented. We speculate that the most likely explanation for what has been observed is that the X-ray sources are AGNs which trace filaments connected to the clusters. Nevertheless other possible explanations such as an “X-ray Butcher-Oemler” effect are not ruled out by the present results. If the association of the overdensities with large-scale structures and their positive relation with cluster redshift is confirmed, these studies could represent a new, direct, way of mapping the cosmic web and its parameters at high z.
Key words: galaxies: clusters: general / galaxies: active / X-rays: galaxies: clusters / large-scale structure of Universe
© ESO, 2005
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