29 August 2017 Optical integration of SPO mirror modules in the ATHENA telescope
Author Affiliations +
Abstract
ATHENA (Advanced Telescope for High-ENergy Astrophysics) is the next high-energy astrophysical mission selected by the European Space Agency for launch in 2028. The X-ray telescope consists of 1062 silicon pore optics mirror modules with a target angular resolution of 5 arcsec. Each module must be integrated on a 3 m structure with an accuracy of 1.5 arcsec for alignment and assembly. This industrial and scientific team is developing the alignment and integration process of the SPO mirror modules based on ultra-violet imaging at the 12 m focal plane. This technique promises to meet the accuracy requirement while, at the same time, allowing arbitrary integration sequence and mirror module exchangeability. Moreover, it enables monitoring the telescope point spread function during the planned 3-year integration phase.
Conference Presentation
© (2017) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
G. Valsecchi, F. Marioni, G. Bianucci, F. E. Zocchi, D. Gallieni, G. Parodi, M. Ottolini, M. Collon, M. Civitani, G. Pareschi, D. Spiga, M. Bavdaz, E. Wille, "Optical integration of SPO mirror modules in the ATHENA telescope", Proc. SPIE 10399, Optics for EUV, X-Ray, and Gamma-Ray Astronomy VIII, 103990E (29 August 2017); doi: 10.1117/12.2272997; https://doi.org/10.1117/12.2272997
PROCEEDINGS
10 PAGES + PRESENTATION

SHARE
RELATED CONTENT

Hartmann testing of x-ray telescopes
Proceedings of SPIE (September 26 2013)
Recent advance in segmented thin-foil x-ray optics
Proceedings of SPIE (January 30 2002)
Use of silicon pore optics for an SF class deployed...
Proceedings of SPIE (June 13 2006)
A comparison study of mass area ratio for large size...
Proceedings of SPIE (June 15 2006)

Back to Top