101. Star formation in AGN hosts in GOODS-N
- Author
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Bruno Altieri, Emmanouel Rovilos, Marcella Brusa, V. Mainieri, Franz E. Bauer, Reinhard Genzel, Giulia Rodighiero, Andrea Grazian, N. M. Förster Schreiber, Albrecht Poglitsch, Francesca Pozzi, Paola Santini, Amélie Saintonge, David M. Alexander, Carlotta Gruppioni, Dieter Lutz, M. Wetzstein, L. Riguccini, E. Sturm, W. N. Brandt, Emanuele Daddi, Lijing Shao, Benjamin Magnelli, Roberto Maiolino, Ángel Bongiovanni, H. Dominguez-Sanchez, Linda J. Tacconi, Georgios E. Magdis, Mara Salvato, Ivan Valtchanov, S. Berta, Raanan Nordon, A. M. Pérez García, J. Cepa, Norbert Geis, Andrea Cimatti, Paola Popesso, Antonio Cava, E. Wieprecht, Herve Aussel, M. Sanchez Portal, David Elbaz, Paola Andreani, Shao L., Lutz D., Nordon R., Maiolino R., Alexander D. M., Altieri B., Andreani P., Aussel H., Bauer F. E., Berta S., Bongiovanni A., Brandt W. N., Brusa M., Cava A., Cepa J., Cimatti A., Daddi E., Dominguez-Sanchez H., Elbaz D., Förster Schreiber N. M., Geis N., Genzel R., Grazian A., Gruppioni C., Magdis G., Magnelli B., Mainieri V., Pérez García A. M., Poglitsch A., Popesso P., Pozzi F., Riguccini L., Rodighiero G., Rovilos E., Saintonge A., Salvato M., Sanchez Portal M., Santini P., Sturm E., Tacconi L. J., Valtchanov I., Wetzstein M., and Wieprecht E.
- Subjects
Physics ,Cosmology and Nongalactic Astrophysics (astro-ph.CO) ,Star formation ,Astrophysics::High Energy Astrophysical Phenomena ,Conjunction (astronomy) ,FOS: Physical sciences ,Astronomy and Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Astrophysics ,Galaxy ,Redshift ,Luminosity ,Space and Planetary Science ,Astrophysics::Solar and Stellar Astrophysics ,Astrophysics::Earth and Planetary Astrophysics ,Astrophysics::Galaxy Astrophysics ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
Sensitive Herschel far-infrared observations can break degeneracies that were inherent to previous studies of star formation in high-z AGN hosts. Combining PACS 100 and 160um observations of the GOODS-N field with 2Msec Chandra data, we detect ~20% of X-ray AGN individually at >3sig. The host far-infrared luminosity of AGN with L2-10~10^43erg/s increases with redshift by an order of magnitude from z=0 to z~1. In contrast, there is little dependence of far-infrared luminosity on AGN luminosity, for L2-10~1. We do not find a dependence of far-infrared luminosity on X-ray obscuring column, for our sample which is dominated by L2-10, Comment: Accepted for publication in A&A Herschel issue. 4 pages, 6 figures
- Published
- 2010