Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003spie.4851..801k&link_type=abstract
X-Ray and Gamma-Ray Telescopes and Instruments for Astronomy. Edited by Joachim E. Truemper, Harvey D. Tananbaum. Proceedings
Astronomy and Astrophysics
Astronomy
Scientific paper
The pn-CCD camera on board of XMM-Newton as well as the Wide Field Imager (WFI) currently being designed for the XEUS mission can be read out in special fast timing modes, providing spectroscopy at very high time resolution. The two fast modes, Timing and Burst mode, of the pn-CCD camera on board XMM-Newton provide a time resolution of 30 μs, respectively. However, this fast timing is only possible at the expense of spatial resolution in readout direction. In contrast, the current baseline design of the WFI for XEUS will provide 25 μs timing at full spatial resolution. We describe the basic principles of the fast readout schemes of the pn-CCD and the SFI, discuss the potential of XEUS for high time resolution spectroscopy and present first results of pulse phase resolved spectroscopy of the Crab pulsar with the pn-CCD in Timing mode.
Becker Werner
Holl Peter
Kendziorra Eckhard
Kirsch Marcus
Kuster Markus
No associations
LandOfFree
High-time resolution spectroscopy with XMM-Newton and XEUS does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with High-time resolution spectroscopy with XMM-Newton and XEUS, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High-time resolution spectroscopy with XMM-Newton and XEUS will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1171069