Linear redshift distortions and power in the IRAS Point Source Catalog Redshift Survey

Linear redshift distortions and power in the IRAS Point Source Catalog Redshift Survey
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IRAS 点源目录红移巡天中的线性红移畸变和功率

DOI:
10.1046/j.1365-8711.2000.03888.x
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发表时间:
2000
影响因子:
4.8
通讯作者:
N. Padmanabhan
N. Padmanabhan
中科院分区:
物理与天体物理2区
文献类型:
--
作者:
A. Hamilton;M. Tegmark;N. Padmanabhan

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我们提出了一个国家的最先进的线性红移失真分析最近出版的IRAS点源目录红移巡天(PSCz)。该过程包括线性压缩成4096 Karhunen-Loeve(信噪比)模式,这些模式是从一个103 ×105的潜在模式库中挑选出来的,然后进行二次压缩成三个独立的功率谱,即星系-星系功率谱、星系-速度功率谱和速度-速度功率谱。最小二乘拟合的解相关功率谱产生一个线性红移失真参数
We present a state-of-the-art linear redshift distortion analysis of the recently published IRAS Point Source Catalog Redshift Survey (PSCz). The procedure involves linear compression into 4096 Karhunen–Loeve (signal-to-noise) modes culled from a potential pool of ∼3×105 modes, followed by quadratic compression into three separate power spectra, the galaxy–galaxy, galaxy–velocity and velocity–velocity power spectra. Least squares-fitting to the decorrelated power spectra yields a linear redshift distortion parameter