paper

The far-infrared--submm spectral energy distribution of high-redshift quasars

arXiv:astro-ph/0102116 · doi:10.1046/j.1365-8711.2001.04548.x

Abstract

We combine submm photometric data of z>4 quasars, to obtain a mean far-infrared (FIR) (rest-frame) spectral energy distribution (SED) of thermal emission from dust, parameterised by a single temperature (T) and power-law emissivity index (beta). Best-fit values are T=41+/-5K, beta=1.95+/-0.3. The redshift spread of this set of quasars is exploited to allow us to sample the SED at a greater number of rest wavelengths than is possible for a single object. This parameterisation is of use to any study that extrapolates from a flux at a single submm wavelength, for example to infer dust masses and FIR luminosities. We then interpret the submm component as arising from dust heated by star-formation in the quasar's host galaxy, and investigate a simple scheme of AGN--host coevolution, in which the timescale for formation of the host galaxy is c.0.5-1.0Gyr, with star formation proceeding at a constant rate c.1000Msol/yr. The luminous quasar phase occurs towards the end of the star-forming period, just before the galaxy's reservoir of cold gas is depleted. Given the youth of the Universe at z=4 (1.6Gyr), the coexistence of a massive black hole and a luminous starburst can be a powerful constraint on models of quasar host-galaxy formation.

Accepted version to appear in MNRAS: minor revisions. 5 pages. PostScript version available, with information about related high-redshift quasar projects, at http://www.ast.cam.ac.uk/~quasars

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