The development of the THESEUS SXI optics
Charlotte H. Feldman, Paul O'Brien, Richard Willingale, Emile Schyns,, Romain Roudot, Ray Fairbend, Julien Seguy, Hannah Natasha Lerman, Ian, Hutchinson, Melissa McHugh, Alexander Lodge, Roisin Speight

TL;DR
This paper details the design and development of the THESEUS SXI optics, a lobster eye X-ray module with Micro Pore Optics, aiming for high-resolution transient X-ray monitoring in a future space mission.
Contribution
It presents the design of the THESEUS SXI lobster eye optics and discusses methods to improve MPO performance during Phase A development.
Findings
Optics design for the SXI modules is finalized.
Methods to enhance MPO performance are under investigation.
Performance goals include 4.5 arcmin resolution and 1 arcmin localization accuracy.
Abstract
The Transient High Energy Sources and Early Universe Surveyor is an ESA M5 candidate mission currently in Phase A, with Launch in 2032. The aim of the mission is to complete a Gamma Ray Burst survey and monitor transient X-ray events. The University of Leicester is the PI institute for the Soft X-ray Instrument (SXI), and is responsible for both the optic and detector development. The SXI consists of two wide field, lobster eye X-ray modules. Each module consists of 64 Micro Pore Optics (MPO) in an 8 by 8 array and 8 CMOS detectors in each focal plane. The geometry of the MPOs comprises a square packed array of microscopic pores with a square cross-section, arranged over a spherical surface with a radius of curvature twice the focal length of the optic. Working in the photon energy range 0.3-5 keV, the optimum ratio (length of pore and pore width ) is upwards of 50…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Gamma-ray bursts and supernovae · Particle Detector Development and Performance
