The Rest‐Frame Extreme‐Ultraviolet Spectral Properties of Quasi‐stellar Objects

TLDR

The sample is nearly twice as large as that used by Zheng et al. and offers superior extreme‑ultraviolet spectral coverage. The study uses 332 HST spectra of 184 QSOs (z > 0.33) to investigate their typical ultraviolet spectral properties, focusing on the ionizing continuum. The authors derive the EUV spectral index αEUV for individual QSOs, analyzing 39 radio‑quiet and 40 radio‑loud objects, and construct composite spectra.

Abstract

We use a sample of 332 Hubble Space Telescope spectra of 184 quasi-stellar objects (QSOs) with z > 0.33 to study the typical ultraviolet spectral properties of QSOs, with emphasis on the ionizing continuum. Our sample is nearly twice as large as that from previous work by W. Zheng and colleagues and provides much better spectral coverage in the extreme-ultraviolet (EUV). The overall composite continuum can be described by a power law with index αEUV = -1.76 ± 0.12 (fν ∝ να) between 500 and 1200 Å. The corresponding results for subsamples of radio-quiet and radio-loud QSOs are αEUV = -1.57 ± 0.17 and αEUV = -1.96 ± 0.12, respectively. We also derive αEUV for as many individual objects in our sample as possible, totaling 39 radio-quiet and 40 radio-loud QSOs. The typical individually measured values of αEUV are in good agreement with the composites. We find no evidence for evolution of αEUV with redshift for either radio-loud or radio-quiet QSOs. However, we do find marginal evidence for a trend toward harder EUV spectra with increasing luminosity for radio-loud objects. An extrapolation of our radio-quiet QSO spectrum is consistent with existing X-ray data, suggesting that the ionizing continuum may be represented by a single power law. The resulting spectrum is roughly in agreement with models of the intergalactic medium photoionized by the integrated radiation from QSOs.