The unresolved hard X-ray background: the missing source population implied by the Chandra and XMM-Newton deep fields
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W. Brandt | G. Hasinger | M. Worsley | A. Fabian | D. Alexander | F. Bauer | H. Brunner | S. Mateos | D. Schneider | A. C. Fabian | D. Alexander | D. P. Schneider | F. Bauer | G. Hasinger | S. Mateos | H. Brunner