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Astrophysics > Cosmology and Nongalactic Astrophysics

arXiv:1403.5898v2 (astro-ph)
[Submitted on 24 Mar 2014 (v1) , last revised 12 May 2014 (this version, v2)]

Title: Background power subtraction in Lyman-alpha forest

Title: 背景功率减去在莱曼-α森林中

Authors:Vid Iršič, Anže Slosar
Abstract: When measuring the one-dimensional power spectrum of the Ly$\alpha$ forest, it is common to measure the power spectrum in flux fluctuations red-ward of the Ly$\alpha$ emission of quasars and subtract this power from the measurements of the Ly$\alpha$ flux power spectrum. This removes excess power present in the Ly$\alpha$ forest which is believed to be dominated by metal absorption by the low-redshift metals uncorrelated with the neutral hydrogen aborbing in Ly$\alpha$. In this brief report we note that, assuming the contaminants are additive in optical depth, the correction contains a second order term. We estimate the magnitude of this term for two currently published measurements of the 1D Ly$\alpha$ flux power spectrum and show that it is negligible for the current generation of measurements. However, future measurements will have to take this into account when errorbars improve by a factor of two or more.
Abstract: 在测量类星体Ly$\alpha$森林的一维功率谱时,通常会在Ly$\alpha$发射线红移方向测量流量波动的功率谱,并从Ly$\alpha$流量功率谱的测量结果中减去这一功率。 这消除了Ly$\alpha$森林中存在的额外功率,据信这些功率主要由低红移金属吸收引起,与Ly$\alpha$中中性氢的吸收无关。 在本简短报告中我们注意到,假设污染物在光学深度上是相加的,修正中包含一个二阶项。 我们估计了这一项对于两个目前发表的1D Ly$\alpha$流量功率谱测量的大小,并表明对于当前一代的测量来说它是可以忽略的。 然而,未来测量在误差条改善两倍或更多时必须考虑这一点。
Comments: 5 pages, 2 figures; published in Physical Review D (5th of May 2014)
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
Cite as: arXiv:1403.5898 [astro-ph.CO]
  (or arXiv:1403.5898v2 [astro-ph.CO] for this version)
  https://doi.org/10.48550/arXiv.1403.5898
arXiv-issued DOI via DataCite
Journal reference: Phys. Rev. D 89, 107301 (2014)
Related DOI: https://doi.org/10.1103/PhysRevD.89.107301
DOI(s) linking to related resources

Submission history

From: Vid Iršič [view email]
[v1] Mon, 24 Mar 2014 10:17:58 UTC (320 KB)
[v2] Mon, 12 May 2014 09:35:09 UTC (321 KB)
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