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- W4230080759 abstract "The Constellation-X mission's Spectroscopic X-Ray Telescopes (SXT) require an angular resolution of 15 half-power diameter (HPD) with extremely lightweight grazing incidence mirrors. The areal density of the mirror must be about 1 kg/m<sup>2</sup> or less. In comparison with the state of the art X-ray mirrors represented by the XMM/Newton telescopes, this is approximately an order of magnitude less in mass areal density while maintaining the same angular resolution. We use a precision glass forming technique to fabricate mirrors that are 0.4mm thick and optical metrology to demonstrate that these mirrors can meet the stringent figure and micro-roughness requirements of the Constellation-X mission. We expect in the next few years to significantly improve the production yield and mirror quality to meet the goal of the mission, which is 5 HPD for two reflections at the same mass." @default.
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- W4230080759 date "2005-08-18" @default.
- W4230080759 modified "2023-09-29" @default.
- W4230080759 title "Development of lightweight x-ray mirrors for the Constellation-X mission" @default.
- W4230080759 doi "https://doi.org/10.1117/12.614462" @default.
- W4230080759 hasPublicationYear "2005" @default.
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