A. Georgakakis, F. Carrera, G. Lanzuisi, M. Brightman, J. Buchner, J. Aird, M. Page, M. Cappi, J. Afonso, A. Alonso-Herrero, L. Ballo, X. Barcons, M. T. Ceballos, A. Comastri, I. Georgantopoulos, S. Mateos, K. Nandra, D. Rosario, M. Salvato, K. Schawinski, P. Severgnini, C. Vignali
Observations in the last decade have provided strong evidence that the growth of supermassive black holes at the centres of galaxies is among the most influential processes in galaxy evolution. Open questions that relate to our current understanding of black hole growth and its relation to the build-up of galaxies at redshifts z=1-4, when most black holes and stars we see in present-day galaxies were put in place, include: what is the nature of AGN feedback and whether it plays a significant role in the evolution of galaxies? what is the dominant population of accreting AGN at that critical epoch? is it dominated by obscured objects as required by many current observations and models? The Athena+ mission concept will provide the technological leap required for a breakthrough in our understanding of AGN and galaxy evolution at the heyday of the Universe. The high throughput of Athena+ will allow the systematic study of the incidence, nature and energetics of AGN feedback processes to z~4 via the identification and measurement of blue-shifted X-ray absorption lines. The excellent survey and spectral capabilities of the Athena+ Wide Field Imager will complete the census of black hole growth by yielding samples of up to 100 times larger than is currently possible of the most heavily obscured, including Compton thick, AGN to redshifts z~4. The demographics of this population relative to their hosts is fundamental for understanding how major black hole growth events relate to the build-up of galaxies.
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http://arxiv.org/abs/1306.2328
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