Computation of the off-axis effective area of the New Hard X-ray Mission modules by means of an analytical approach
D. Spiga, V. Cotroneo

TL;DR
This paper introduces an analytical method to efficiently compute the off-axis effective area of X-ray telescope mirrors with multilayer coatings, improving over traditional ray-tracing techniques.
Contribution
The authors develop a novel analytical formalism for calculating the off-axis effective area of multilayer-coated X-ray mirrors, simplifying and speeding up the process.
Findings
Validated the analytical approach against ray-tracing results.
Applied the method to NHXM optical modules.
Demonstrated improved computational efficiency.
Abstract
One of the most important parameters determining the sensitivity of X-ray telescopes is their effective area as a function of the X-ray energy. The computation of the effective area of a Wolter-I mirror, with either a single layer or multilayer coating, is a very simple task for a source on-axis at astronomical distance. Indeed, when the source moves off-axis the calculation is more complicated, in particular for new hard X-ray imaging telescopes (NuSTAR, ASTRO-H, NHXM, IXO) beyond 10 keV, that will make use of multilayer coatings to extend the reflectivity band in grazing incidence. Unlike traditional single-layer coatings (in Ir or Au), graded multilayer coatings exhibit an oscillating reflectivity as a function of the incidence angle, which makes the effective area not immediately predictable for a source placed off-axis within the field of view. For this reason, the computation of…
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