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Vogt, S.S., Allen, S.L., Bigelow, B.C., Bresee, L., Brown, W.E., Cantrall, T., et al. (1994) HIRES: The High-Resolution Echelle Spectrometer on the Keck 10-m Telescope. SPIE Proceedings, 2198, 362.
https://doi.org/10.1117/12.176725

has been cited by the following article:

• TITLE: Study of Warm Dark Matter with the Lyman-α Forest

  AUTHORS: Bruce Hoeneisen

  KEYWORDS: Lyman-α Forest, Warm Dark Matter, Free Streaming, Dark Matter

  JOURNAL NAME: International Journal of Astronomy and Astrophysics, Vol.16 No.3, July 20, 2026

  ABSTRACT: Quasar light becomes absorbed by the Lyman-α line of neutral hydrogen in “clouds” along the line-of-sight in the highly ionized intergalactic medium after re-ionization. The received flux spectrum is known as the “Lyman-α forest”. Limits on the dark matter “standard thermal relic mass” have been obtained in the literature from the power spectrum of the Lyman-α forest, e.g. m th >5.7 keV. These limits are in tension with four independent estimates of the dark matter warmness: 0.6≲ m th ≲1.6 keV. To try to understand this tension we attempt to measure the dark matter warmness by two methods: the power spectrum of the Lyman-α forest, and the width of individual absorption lines, e.g. “Lyman-α trees”. We obtain a measurement of the dark matter warmness with the Lyman-α forest power spectrum, in agreement with the four independent estimates. In conclusion, the warm dark matter free-streaming is clearly observed as a cut-off of the Lyman-α forest power spectrum.