@inproceedings{71be64f327674817999a2d73dff7a710,
title = "Off-plane x-ray grating spectrometer camera for IXO",
abstract = "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/ΔE > 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.",
author = "Murray, {Neil J.} and Holland, {Andrew D.} and Harriss, {Richard D.} and Tutt, {James H.} and Barber, {Simeon J.} and Peter Pool and James Endicott and David Burt and Dave Walton and Mat Page and McEntaffer, {Randall L.} and Ted Schultz and Cash, {Webster C.} and Chuck Lillie and Suzanne Casement",
year = "2010",
doi = "10.1117/12.864051",
language = "English (US)",
isbn = "9780819482327",
series = "Proceedings of SPIE - The International Society for Optical Engineering",
booktitle = "High Energy, Optical, and Infrared Detectors for Astronomy IV",
note = "High Energy, Optical, and Infrared Detectors for Astronomy IV ; Conference date: 27-06-2010 Through 30-06-2010",
}