Volume 372, Number 3, June IV 2001
|Page(s)||1088 - 1094|
|Section||Numerical methods and codes|
|Published online||15 June 2001|
Optimization of grazing incidence mirrors and its application to surveying X-ray telescopes
Osservatorio Astronomico di Brera, Via Bianchi 46, 23807 Merate (Lc), Italy
Corresponding author: S. Campana, email@example.com
Accepted: 30 March 2001
Grazing incidence mirrors for X-ray astronomy are usually designed in the parabola-hyperbola (Wolter I) configuration. This design allows for optimal images on-axis, which however degrade rapidly with the off-axis angle. Mirror surfaces described by polynomia (with terms higher than order two), have been put forward to improve the performances over the field of view. Here we present a refined procedure aimed at optimizing wide-field grazing incidence telescopes for X-ray astronomy. We improve the angular resolution over existing (wide-field) designs by ~20% . We further consider the corrections for the different plate scale and focal plane curvature of the mirror shells, which sharpen by another ~20% the image quality. This results in a factor of ~2 reduction in the observing time needed to achieve the same sensitivity over existing wide-field designs and of ~5 over Wolter I telescopes. We demonstrate that such wide-field X-ray telescopes are highly advantageous for deep surveys of the X-ray sky.
Key words: telescopes / surveys / X / rays: general
© ESO, 2001
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