Asset Publisher

Off-plane x-ray grating spectrometer camera for IXO

Off-plane x-ray grating spectrometer camera for IXO

Publication date: 01 August 2010

Authors: Murray, N., et al.

Journal: Proc. SPIE
Volume: 7732
Year: 2010

Copyright: SPIE

The International X-ray Observatory (IXO) is a merger of the former ESA XEUS and NASA Constellation-X missions, with additional collaboration from JAXA, proposed for launch ~2020. IXO will address the leading astrophysical questions in the 'hot universe' through its breakthrough capabilities in X-ray spectroscopy. The mission covers the 0.1 to 40 keV energy range, complementing the capabilities of the next generation observatories, such as ALMA, LSST, JWST and 30 meter ground-based telescopes. An X-ray Grating Spectrometer is baselined to provide science in the energy range 0.3-1.0 keV at a spectral resolution of E/DeltaE > 3,000 with an effective area greater than 1,000 cm2. This will require an array of soft X-ray enhanced CCDs operating at a modest frame rate to measure the diffracted light in both position and energy. Here we describe the baseline camera for the Off-plane XGS instrument using mature CCD technology.

This paper was presented at the SPIE conference on Astronomical Instrumentation 2010 conference.

Link to publication
Last Update: Sep 1, 2019 8:57:48 AM
15-Nov-2019 08:09 UT

ShortUrl Portlet

Shortcut URL

https://sci.esa.int/s/wQdDz4A

Images And Videos

Related Publications

Related Links

See Also

Documentation