Journal Article

Interpreting the transmission windows of distant quasars

A. Maselli, A. Ferrara and S. Gallerani

in Monthly Notices of the Royal Astronomical Society

Published on behalf of The Royal Astronomical Society

Volume 395, issue 4, pages 1925-1933
Published in print June 2009 | ISSN: 0035-8711
Published online May 2009 | e-ISSN: 1365-2966 | DOI:
Interpreting the transmission windows of distant quasars

Show Summary Details


We propose the apparent shrinking criterion (ASC) to interpret the spatial extent, Rw, of transmitted flux windows in the absorption spectra of high-z quasars. The ASC can discriminate between the two regimes in which Rw corresponds either to the physical size, RH ii, of the quasar H ii region or to the distance, Rmaxw, at which the transmitted flux drops to =0.1 and a Gunn–Peterson (GP) trough appears. In the first case [H ii region (HR) regime], one can determine the intergalactic medium mean H i fraction, xH I; in the second [proximity region (PR) regime], the value of Rw allows one to measure the local photoionization rate and the local enhancement of the photoionization rate, ΓG, due to nearby/intervening galaxies. The ASC has been tested against radiative transfer+smoothed particle hydrodynamics numerical simulations, and applied to a sample of 15 high-z (z > 5.8) quasar spectra. All sample quasars are found to be in the PR regime; hence, their observed spectral properties (inner flux profile, extent of transmission window) cannot reliably constrain the value of xH i. Four sample quasars show evidence for a local enhancement (up to 50 per cent) in the local photoionization rate possibly produced by a galaxy overdensity. We discuss the possible interpretations and uncertainties of this result.

Keywords: radiative transfer; methods: numerical; intergalactic medium; quasars: general; cosmology: theory; large scale structure of Universe

Journal Article.  7525 words.  Illustrated.

Subjects: Astronomy and Astrophysics

Full text: subscription required

How to subscribe Recommend to my Librarian

Users without a subscription are not able to see the full content. Please, subscribe or login to access all content.