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Preparing the optics technology to observe the hot universe

Authors :
Brian Shortt
Peter Müller
Anders Clemen Jakobsen
Mauro Ghigo
Coen van Baren
Finn Erland Christensen
Marcos Bavdaz
Giuseppe Vacanti
Eric Wille
Michael Krumrey
Mark Olde Riekerink
Desiree Della Monica Ferreira
Dirk Kampf
Jeroen Haneveld
Maximilien J. Collon
Vadim Burwitz
Markus Ackermann
Karl-Heinz Zuknik
Sebastiaan Fransen
Ramses Guenther
Giovanni Pareschi
Kotska Wallace
Source :
SPIE Proceedings.
Publication Year :
2014
Publisher :
SPIE, 2014.

Abstract

With the selection of “The hot and energetic Universe” as science theme for ESA's second large class mission (L2) in the Cosmic Vision programme, work is focusing on the technology preparation for an advanced X-ray observatory. The core enabling technology for the high performance mirror is the Silicon Pore Optics (SPO) [1 to 23], a modular X-ray optics technology, which utilises processes and equipment developed for the semiconductor industry. The paper provides an overview of the programmatic background, the status of SPO technology and gives an outline of the development roadmap and activities undertaken and planned by ESA on optics, coatings [24 to 30] and test facilities [31, 33].

Details

ISSN :
0277786X
Database :
OpenAIRE
Journal :
SPIE Proceedings
Accession number :
edsair.doi...........d26379c00a71a90eee8b91fa51c02247