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首页> 外文期刊>The Astrophysical journal >Intrinsic Properties of the (z) = 2.7 Lyα Forest from Keck Spectra of Quasar HS 1946+7658
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Intrinsic Properties of the (z) = 2.7 Lyα Forest from Keck Spectra of Quasar HS 1946+7658

机译:类星体HS 1946 + 7658的Keck光谱中(z)= 2.7Lyα森林的内在特性

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摘要

We present the highest quality Lyα forest spectra published to date. We have complete 7.9 km s~-1 FWHM spectra between the Lyα and Lyβ emission lines of the bright, high-redshift (V = 15.9, z = 3.05) QSO HS 1946+7658. The mean redshift of observed Lyα forest clouds is (z) = 2.7. The spectrum has a signal-to-noise ratio per pixel of 2 km s~-1 that varies from 15 at 4190 A deg to 100 at 4925 A deg . The absorption lines in the spectrum have been fitted with Voigt profiles, and the distribution of Voigt parameters has been analyzed. We show that fitting Voigt profiles to high quality data does not give unique results. We have performed simulations to differentiate between true features of the line distributions and artifacts of line blending and the fitting process.
机译:我们展示了迄今为止发布的最高质量的Lyα森林光谱。我们在明亮的高红移(V = 15.9,z = 3.05)QSO HS 1946 + 7658的Lyα和Lyβ发射谱线之间具有完整的7.9 km s〜-1 FWHM光谱。观察到的Lyα森林云的平均红移为(z)= 2.7。该频谱的每个像素的信噪比为2 km s-1,从4190 A度的15到4925 A度的100变化。光谱中的吸收线已经拟合了Voigt轮廓,并且已经分析了Voigt参数的分布。我们表明,将Voigt轮廓与高质量数据拟合不会产生独特的结果。我们进行了仿真,以区分线分布的真实特征和线融合的伪影以及拟合过程。

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