The XMM deep survey in the CDF-S
Overview & Synopsis
The Chandra Deep Field is the region of the sky with the highest concentration of X-ray data available: 4 Ms of Chandra and 3 Ms of XMM-Newton data, allowing excellent quality spectra to be extracted even for faint sources. We took advantage of this to compile a sample of heavily obscured active galactic nuclei (AGN) using X-ray spectroscopy. We selected our sample among the 176 brightest XMM-Newton sources, searching for either flat X-ray spectra (ฮ
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Document Information
| Document Title | The XMM deep survey in the CDF-S |
|---|---|
| Author / Organization | I. Georgantopoulos, A. Comastri, C. Vignali, P. Ranalli, E. Rovilos, K. Iwasawa, R. Gilli, N. Cappelluti, F. Carrera, J. Fritz, M. Brusa, D. Elbaz, R. J. Mullaney, N. Castello-Mor, X. Barcons, P. Tozzi, I. Balestra, S. Falocco |
| Subject & Discipline | Multidisciplinary Academic Open Research |
| Categories | Science & Mathematics |
| Publication Year | 2013 |
| License / Rights | Open Access / Creative Commons |
| Resource Verification | Listed PDF (Verification Pending) |
| Original Host Website |
HAL Open Science
(hal.science)
|
| File Format | application/pdf (Portable Document Format) |
| Language | EN |
| Catalog ID | DOC-242003 |
| Original Source Link | Visit Source Page on hal.science » |