Published May 11, 2009 | Version v1
Journal article

Simbol-X Core Science in a Context

  • 1. INAF-OARoma, Via Frascati 33, I-00040 Monteporzio (Italy)
  • 2. CEA/DSM/Irfu/SAp and Laboratoire AIM, CEA/Saclay 91191 Gif-sur-Yvette Cedex (France)
  • 3. Max Planck Instituet fuer Extraterrestrische Physik, 85748 Garching (Germany)
  • 4. ASI ASDC c/o ESRIN, 00044 Frascati (Italy)
  • 5. CNES, 18 avenue Edouard Belin, 31041 Toulouse Cedex (France)
  • 6. INAF-OABo, via Ranzani 1, Bologna (Italy)
  • 7. CEA/DSM/Irfu/SAp, CEA/Saclay 91191 Gif-sur-Yvette Cedex, and Laboratoire APC, Paris (France)
  • 8. INAF-IASF-Bo, via Gobetti 101, 40129 Bologna (Italy)
  • 9. INAF-IASF-Mi, Via Bassini 15, 20133 Milano (Italy)
  • 10. INAF-OAPa, Palazzo dei Normanni, 90134 Palermo (Italy)

Description

Taking advantage of emerging technology in mirror manufacturing and spacecraft formation flying, Simbol-X will push grazing incidence imaging up to ∼80 keV, providing an improvement of roughly three orders of magnitude in sensitivity and angular resolution compared to all instruments that have operated so far above 10 keV. This will open a new window in X-ray astronomy, allowing breakthrough studies on black hole physics and census and particle acceleration mechanisms. We discuss here synergies between Simbol-X and the main multiwavelength facilities that will operate in the next decade, and present a quantitative comparison between Simbol-X and its main competitors, NuStar and Astro-H.

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
1126
Journal Issue
1
Journal Page Range
p. 9-14
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
2. international Simbol-X symposium
Dates
2-5 Dec 2008
Place
Paris (France)

Optional Information

Notes
(c) 2009 American Institute of Physics