Schwartz, Daniel A., Aldcroft, Thomas L., Bookbinder, Jay A., Cotroneo, Vincenzo, Davis, William N., Forman, William R., Freeman, Mark D., McMuldroch, Stuart, Reid, Paul, Tananbaum, Harvey, Vikhlinin, Alexey A., Trolier-McKinstry, Susan, Wilke, Derek, and Johnson-Wilke, Raegan. 2012. "The square meter arcsecond resolution x-ray telescope: SMART-X." Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series, 8503 08. https://doi.org/10.1117/12.930868.
We describe an X-ray Observatory mission with 0.5" angular resolution, comparable to the Chandra X-ray Observatory, but with 30 times more effective collecting area. The concept is based on developing the new technology of adjustable X-ray optics for ultra thin (0.4 mm), highly nested grazing incidence X-ray mirrors. Simulations to date indicate that the corrections for manufacturing and mounting can be determined on the ground and the effects of gravity release can be calculated to sufficient accuracy, so that all adjustments are applied only once on-orbit, without the need of any on-orbit determination of the required corrections. The mission concept is based on the Chandra Observatory, and takes advantage of the technology studies which have taken place over the past fifteen years developing large area, light weight mirrors.