Paper
18 July 2000 The Maxim Pathfinder Mission: x-ray imaging at 100 micro-arcseconds
Author Affiliations +
Abstract
Ultra-high resolution imaging in the x-ray has the potential to revolutionize the way astronomers view the heavens. Through the use of interferometry at grazing incidence we can image the x-ray sky at the milli-arcsecond (or better) level. In this paper we describe the baseline design of the Maxim Pathfinder Mission, which will be the first interferometric x-ray observatory whose goal is to image the sky at 100 micro-arcsecond resolution in the 0.5 - 1.5 keV band with about 100 cm2 of collecting area. This resolution is adequate to image the coronae of nearby stars and the accretion disks of quasars.
© (2000) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Webster C. Cash, Nicholas White, and Marshall K. Joy "The Maxim Pathfinder Mission: x-ray imaging at 100 micro-arcseconds", Proc. SPIE 4012, X-Ray Optics, Instruments, and Missions III, (18 July 2000); https://doi.org/10.1117/12.391561
Lens.org Logo
CITATIONS
Cited by 6 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Mirrors

Interferometers

Sensors

Space operations

X-rays

Charge-coupled devices

Target acquisition

RELATED CONTENT

GOES solar x-ray imager: overview and operational goals
Proceedings of SPIE (October 18 1996)
JET X instrument for the USSR Spectrum RG mission ...
Proceedings of SPIE (January 01 1992)
MAXIM x-ray interferometry mission
Proceedings of SPIE (January 29 2004)
MAXIM science and technology
Proceedings of SPIE (October 20 2004)
MAXIM Pathfinder x-ray interferometry mission
Proceedings of SPIE (March 11 2003)
Laboratory testbeds for broadband x-ray interferometry
Proceedings of SPIE (October 11 2004)

Back to Top