The He II Lyman alpha Forest: Evaluation of Simulated Data

Astronomy and Astrophysics – Astrophysics

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Scientific paper

Using an artificial H I Lyα spectrum we simulate the corresponding He II forest with fixed values of η and a Doppler parameter consisting of a thermal and a turbulent part. In addition metal lines with line strengths and line density as expected in the case of HS 1700+6416 are superimposed. FUSE-like noise is added. The analysis of the simulated spectra in terms of Doppler profiles recovers the input η = N(He II)/N(H I) with a scatter by a factor of 10. About 10 % have significantly lower η-values for various reasons. The majority of the extremely high η-values (up to 1000) are evidently caused by metal lines. We conclude that part of the scatter in η of previous analyses of the He II forest in HE 2347-4342 can be regarded as an artifact. However, we confirm that the correlation between small column densities (in voids) and high η-values is not a methodical artifact and appears to be a true phenomenon.

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