EXPLORING DUST EXTINCTION AT THE EDGE OF REIONIZATION

被引:25
作者
Zafar, Tayyaba [1 ]
Watson, Darach J. [1 ]
Tanvir, Nial R. [2 ]
Fynbo, Johan P. U. [1 ]
Starling, Rhaana L. C. [2 ]
Levan, Andrew J. [3 ]
机构
[1] Univ Copenhagen, Niels Bohr Inst, Dark Cosmol Ctr, DK-2100 Copenhagen O, Denmark
[2] Univ Leicester, Dept Phys & Astron, Leicester LE1 7RH, Leics, England
[3] Univ Warwick, Dept Phys, Coventry CV4 7AL, W Midlands, England
基金
美国国家科学基金会; 新加坡国家研究基金会;
关键词
dark ages; reionization; first stars; dust; extinction; galaxies: high-redshift; gamma-ray burst: individual: (GRB 090423; 080913; and; 050904); GAMMA-RAY BURST; HIGH-REDSHIFT UNIVERSE; LYMAN-BREAK GALAXIES; DIGITAL SKY SURVEY; SIMILAR-TO; 5; HOST GALAXIES; OPTICAL AFTERGLOWS; DISTANT QUASARS; LIGHT CURVES; GRB; 080913;
D O I
10.1088/0004-637X/735/1/2
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The brightness of gamma-ray burst (GRB) afterglows and their occurrence in young, blue galaxies make them excellent probes to study star-forming regions in the distant universe. We here elucidate dust extinction properties in the early universe through the analysis of the afterglows of all known z > 6 GRBs: GRB 090423, 080913, and 050904, at z = 8.2, 6.69, and 6.295, respectively. We gather all available optical and near-infrared photometry, spectroscopy, and X-ray data to construct spectral energy distributions (SEDs) at multiple epochs. We then fit the SEDs at all epochs with a dust-attenuated power law or broken power law. We find no evidence for dust extinction in GRB 050904 and GRB 090423, with possible evidence for a low level of extinction in GRB 080913. We compare the high redshift GRBs to a sample of lower redshift GRB extinctions and find a lack of even moderately extinguished events (A(V) similar to 0.3) above z greater than or similar to 4. In spite of the biased selection and small number statistics, this result hints at a decrease in dust content in star-forming environments at high redshifts.
引用
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页数:6
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