The effect of the Lyman-alpha forest on the ultraviolet continua of very high redshift quasars

Mathematics – Logic

Scientific paper

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Continuous Spectra, Lyman Alpha Radiation, Quasars, Red Shift, Spectral Energy Distribution, Ultraviolet Spectra, Astronomical Models, Astronomical Spectroscopy, Radiant Flux Density, Spectrum Analysis

Scientific paper

Absolute spectral energy distributions have been obtained for eight very high redshift quasars (zem ≥ 2.7) with the Hale double spectrograph in the observed wavelength range 3200 - 10000 Å (typically 800 - 2500 Å in the rest frame of the quasar). It is found that the true continuum in the region of the "Lyα forest" can be represented by the extrapolation of the continuum defined longward of Lyα emission by fν ≡ ν-α, where 0.28 ≤ α ≤ 0.99. Low-resolution quasar spectra in the ultraviolet (i.e., IUE spectra) can yield apparent continuum levels which are significantly below the true continuum level. Clearly high-resolution spectra of a quasar are needed to determine whether the apparent change in the slope of the continuum shortward of Lyα emission is inherent to the quasar itself or whether it is due to a cosmological distribution of intervening material.

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