New Measurements of the Ionizing Ultraviolet Background over 2 < z < 5 and Implications for Hydrogen Reionization

New Measurements of the Ionizing Ultraviolet Background over 2 < z < 5 and Implications for Hydrogen Reionization
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DOI:
10.1093/mnras/stt1610
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发表时间:
2013-07
影响因子:
4.8
通讯作者:
G. Becker;J. Bolton
G. Becker;J. Bolton
中科院分区:
物理与天体物理2区
文献类型:
--
作者:
G. Becker;J. Bolton

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我们提出了新的测量电离紫外背景的强度和电离光子的全球发射率超过2 - 4,并可能在所有红移z > 2.4。我们的研究结果表明,恒星形成星系的全球平均电离“效率”大幅增加,红移超过3.2 5。
We present new measurements of the intensity of the ionizing ultraviolet background and the global emissivity of ionizing photons over 2 4, and possibly at all redshifts z > 2.4. Our results suggest that the globally-averaged ionizing "efficiency" of star-forming galaxies increases substantially with redshift over 3.2 5.