Translator Disclaimer
11 October 2004 MAXIM: the black hole imager
Author Affiliations +
The Beyond Einstein Program in NASA's Office of Space Science Structure and Evolution of the Universe theme spells out the top level scientific requirements for a Black Hole Imager in its strategic plan. The MAXIM mission will provide better than one tenth of a microarcsecond imaging in the X-ray band in order to satisfy these requirements. We will overview the driving requirements to achieve these goals and ultimately resolve the event horizon of a supermassive black hole. We will present the current status of this effort that includes a study of a baseline design as well as two alternative approaches
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Keith C. Gendreau, Webster C. Cash, Paul Gorenstein, David L. Windt, Phil Kaaret, and Chris Reynolds "MAXIM: the black hole imager", Proc. SPIE 5488, UV and Gamma-Ray Space Telescope Systems, (11 October 2004);


X-ray interferometry: ultra-high-resolution astronomy
Proceedings of SPIE (December 20 2001)
A practical system for x-ray interferometry
Proceedings of SPIE (October 11 2004)
The milli arc second structure imager (MASSIM) a new...
Proceedings of SPIE (July 15 2008)
X-ray interferometric observatory
Proceedings of SPIE (October 01 1991)
INTEGRAL: the next major gamma-ray astronomy mission?
Proceedings of SPIE (November 01 1993)

Back to Top