Evidence of primordial clustering around the QSO SDSS J1030+0524 at z=6.281

被引:83
作者
Stiavelli, M
Djorgovski, SG
Pavlovsky, C
Scarlata, C
Stern, D
Mahabal, A
Thompson, D
Dickinson, M
Panagia, N
Meylan, G
机构
[1] Space Telescope Sci Inst, Baltimore, MD 21218 USA
[2] CALTECH, Dept Astron, Pasadena, CA 91125 USA
[3] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[4] Natl Opt Astron Observ, Tucson, AZ 85726 USA
[5] ESA, Space Telescope Div, Baltimore, MD 21218 USA
[6] Observ, Ecole Polytech Fed Lausanne, Astrophys Lab, CH-1290 Chavannes Des Bois, Switzerland
基金
美国国家航空航天局;
关键词
early universe; galaxies : formation; galaxies : high-redshift;
D O I
10.1086/429406
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present tentative evidence of primordial clustering, manifested as an excess of color-selected objects in the field of the QSO SDSS J1030 + 0524 at redshift z = 6.28. We have selected objects red in i(775) - z(850) on the basis of Hubble Space Telescope Advanced Camera for Surveys imaging of a field centered on the QSO. Compared to data at comparable depth obtained by the Great Observatories Origins Deep Survey, we find an excess of objects with i (775) - z(850) >= 1.5 in the QSO field. The significance of the detection is estimated to be similar to 97% on the basis of the counts alone and increases to 99.4% if one takes into account the color distribution. If confirmed, this would represent the highest redshift example of galaxy clustering and would have implications on models for the growth of structure. Bias-driven clustering of first luminous objects forming in the highest peaks of the primordial density field is expected in most models of early structure formation. The redshift of one of the candidates has been found to be z = 5.970 by our spectroscopy with the Keck I Low Resolution Imaging Spectrometer, confirming the validity of our color selection.
引用
收藏
页码:L1 / L4
页数:4
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