Testing the connection between the X-ray and submillimetre source populations using Chandra

Details Testing the connection between the X-ray and submillimetre source populations using Chandra Testing the connection between the X-ray and submillimetre source populations using Chandra

2000-02-16

arxiv.org/abs/astro-ph/0002322v2

Mon.Not.Roy.Astron.Soc.315:L8,2000

Astronomy and Astrophysics

Astrophysics

Revised version including one improved figure, accepted for publication in MNRAS, 5 pages, 2 figures

Scientific paper

10.1046/j.1365-8711.2000.03621.x

The powerful combination of the Chandra X-ray telescope, the SCUBA submillimetre-wave camera and the gravitational lensing effect of the massive galaxy clusters A2390 and A1835 has been used to place stringent X-ray flux limits on six faint submillimetre SCUBA sources and deep submillimetre limits on three Chandra sources which lie in fields common to both instruments. One further source is marginally detected in both the X-ray and submillimetre bands. For all the SCUBA sources our results are consistent with starburst-dominated emission. For two objects, including SMMJ14011+0252 at z=2.55, the constraints are strong enough that they can only host powerful active galactic nuclei if they are both Compton-thick and any scattered X-ray flux is weak or itself absorbed. The lensing amplification for the sources is in the range 1.5-7, assuming that they lie at z>1. The brightest detected X-ray source has a faint extended optical counterpart (I~22) with colours consistent with a galaxy at z~1. The X-ray spectrum of this galaxy is hard, implying strong intrinsic absorption with a column density of about 1e23 cm-2 and an intrinsic (unabsorbed) 2-10 keV luminosity of 3e44 erg/s. This source is therefore a Type-II quasar. The weakest detected X-ray sources are not detected in HST images down to I~26.

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