SWIFT/XRT follow-up observations of INTEGRAL AGNs
| dc.creator | Landi, R. | |
| dc.creator | Malizia, A. | |
| dc.creator | Bassani, L. | |
| dc.creator | Masetti, N. | |
| dc.creator | Stephen, J. B. | |
| dc.creator | Gianotti, F. | |
| dc.creator | Schiavone, F. | |
| dc.creator | Bazzano, A. | |
| dc.creator | Ubertini, P. | |
| dc.creator | Bird, A. J. | |
| dc.creator | Dean, A. J. | |
| dc.creator | Walter, R. | |
| dc.date | 2006-10-12 | |
| dc.date.accessioned | 2026-07-07T07:26:56Z | |
| dc.date.available | 2026-07-07T07:26:56Z | |
| dc.description | In five years of operation, data from INTEGRAL has been used to discover a large number of gamma-ray sources, a substantial fraction of which have turned out to be active galactic nuclei (AGN). Recently Bassani et al. (2006) have presented a sample of around 60 AGNs of which some still lack optical identification or information in the X-ray band. In this work we present X-ray data for 8 objects acquired with the XRT telescope on-board Swift satellite. The XRT positioning has allowed us to identify the optical counterparts and to classify their types through follow-up measurements. Analysis of these data has also provided information on their spectra below 10 keV. | |
| dc.description | 4 pages, submitted proceeding of the 6th INTEGRAL Workshop "The Obscured Universe" July 2-8, 2006 Space Research Institute Moscow, Russia | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0610358 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0610358 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/117205 | |
| dc.subject | Astrophysics | |
| dc.title | SWIFT/XRT follow-up observations of INTEGRAL AGNs | |
| dc.type | text |