The Chandra Deep Field South (CDF-S) was observed by XMM-Newton for a total of about 3 Ms in many periods over the past decade (2001-2002 and 2008-2009). The main goal of the survey was to obtain good quality X-ray spectroscopy of the AGN responsible for the bulk of the X-ray background. We will present the scientific highlights of the XMM-Newton survey and briefly discuss the perspectives of future observations to pursue XMM deep survey science with current and forthcoming X-ray facilities.The Chandra Deep Field South (CDF-S) was observed by XMM-Newton for about 3 Ms in many periods over the past decade (2001\u20132002 and 2008\u20132009). The main goal of the survey was to obtain good quality X-ray spectroscopy of the active galactic nucl...
Context. X-ray spectroscopy of active galactic nuclei (AGN) offers the opportunity to directly probe...
We present the first results of the spectroscopy of distant, obscured AGN as obtained with the ultra...
Nuclear obscuration plays a key role in the initial phases of AGN growth, yet not many highly obscur...
The Chandra Deep Field South (CDF-S) was observed by XMM-Newton for a total of about 3 Ms in many p...
none13siThe XMM-Newton survey in the Chandra Deep Field South (XMM-CDFS) aims at detecting and study...
We present the X-ray spectra of 185 bright sources detected in the XMM-Newton deep survey of the Cha...
Nuclear obscuration plays a key role in the initial phases of AGN growth, yet not many highly obscur...
The ultradeep (about 3 Ms) XMM exposure in the Chandra Deep Field South (CDFS) will provide the most...
We extend our earlier work on X-ray source stacking in the deep XMM—Newton observation of the Lockma...
Context. X-ray spectroscopy of active galactic nuclei (AGN) offers the opportunity to directly probe...
We present the first results of the spectroscopy of distant, obscured AGN as obtained with the ultra...
We present the X-ray spectra of 185 bright sources detected in the XMM-Newton deep survey of the Cha...
We present the first results of the spectroscopy of distant, obscured AGN as obtained with the ultra...
none10siWe present results from the deep XMM-Newton observations of the two brightest X-ray sources ...
Context. X-ray spectroscopy of active galactic nuclei (AGN) offers the opportunity to directly probe...
We present the first results of the spectroscopy of distant, obscured AGN as obtained with the ultra...
Nuclear obscuration plays a key role in the initial phases of AGN growth, yet not many highly obscur...
The Chandra Deep Field South (CDF-S) was observed by XMM-Newton for a total of about 3 Ms in many p...
none13siThe XMM-Newton survey in the Chandra Deep Field South (XMM-CDFS) aims at detecting and study...
We present the X-ray spectra of 185 bright sources detected in the XMM-Newton deep survey of the Cha...
Nuclear obscuration plays a key role in the initial phases of AGN growth, yet not many highly obscur...
The ultradeep (about 3 Ms) XMM exposure in the Chandra Deep Field South (CDFS) will provide the most...
We extend our earlier work on X-ray source stacking in the deep XMM—Newton observation of the Lockma...
Context. X-ray spectroscopy of active galactic nuclei (AGN) offers the opportunity to directly probe...
We present the first results of the spectroscopy of distant, obscured AGN as obtained with the ultra...
We present the X-ray spectra of 185 bright sources detected in the XMM-Newton deep survey of the Cha...
We present the first results of the spectroscopy of distant, obscured AGN as obtained with the ultra...
none10siWe present results from the deep XMM-Newton observations of the two brightest X-ray sources ...
Context. X-ray spectroscopy of active galactic nuclei (AGN) offers the opportunity to directly probe...
We present the first results of the spectroscopy of distant, obscured AGN as obtained with the ultra...
Nuclear obscuration plays a key role in the initial phases of AGN growth, yet not many highly obscur...