Optical design of type-1 x-ray telescopes and their application to STAR-X.
Journal
Applied optics
ISSN: 1539-4522
Titre abrégé: Appl Opt
Pays: United States
ID NLM: 0247660
Informations de publication
Date de publication:
10 Jan 2022
10 Jan 2022
Historique:
entrez:
24
2
2022
pubmed:
25
2
2022
medline:
25
2
2022
Statut:
ppublish
Résumé
An astronomical x-ray telescope's capability rests on the quality of its optics, which in turn rests on its point spread function (PSF), field of view (FOV), and photon-collecting area. The design and implementation of telescope optics must optimize these three parameters in the context of mathematical prescription, optical fabrication, engineering, and resources such as mass and cost constraints. In this paper, after reviewing important features of grazing incidence optics and the many different mathematical prescriptions in the literature, we quantitatively compare the advantages and disadvantages of these prescriptions, using detailed ray trace, to optimize the PSF and FOV for a given set of requirements. Then, we apply this approach to optimizing the designs for a proposed future x-ray telescope, Survey and Time-Domain Astrophysical Research eXplorer (STAR-X), a NASA Medium-Class (MIDEX) mission by optimizing the combination of PSF and FOV.
Identifiants
pubmed: 35200890
pii: 466631
doi: 10.1364/AO.446958
doi:
Types de publication
Journal Article
Langues
eng
Sous-ensembles de citation
IM