Highlights from XMM-Newton
| dc.creator | Barcons, X. | |
| dc.creator | Negueruela, I. | |
| dc.date | 2003-06-20 | |
| dc.date.accessioned | 2026-07-07T02:08:49Z | |
| dc.date.available | 2026-07-07T02:08:49Z | |
| dc.description | The launch of the Chandra (NASA) and XMM-Newton (ESA) X-ray observatories in 1999 has revolutionized our view of the Universe, by providing astrophysical information about many classes of sources with unprecedent detail. The high throughput of XMM-Newton makes it the ideal instrument to provide low to moderate resolution spectroscopy of faint and extended sources. After 3 years of operations, XMM-Newton has observed many types of astronomical sources and delivered very interesting results in many areas. In this review, we highlight a few points where the contribution of XMM-Newton has significantly furthered our knowledge of the energetic Universe. | |
| dc.description | 21 pages, inivited paper to appear in the "Boletin de la SEA", July 2003 issue (electronic release at http://sea.am.ub.es) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0306411 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0306411 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/6208 | |
| dc.subject | Astrophysics | |
| dc.title | Highlights from XMM-Newton | |
| dc.type | text |