Toward a 2-eV microcalorimeter x-ray spectrometer for Constellation-X

被引:20
作者
Stahle, CK [1 ]
Bandler, SR [1 ]
Barbee, T [1 ]
Beeman, J [1 ]
Brekosky, RP [1 ]
Cabrera, B [1 ]
Cunningham, M [1 ]
Deiker, S [1 ]
Figueroa-Feliciano, E [1 ]
Finkbeiner, FM [1 ]
Frank, M [1 ]
Gendreau, KC [1 ]
Haller, E [1 ]
Hilton, GC [1 ]
Irwin, KD [1 ]
Kelley, RL [1 ]
Labov, SE [1 ]
Li, MJ [1 ]
Madden, N [1 ]
Martinis, JM [1 ]
McCammon, D [1 ]
Nam, S [1 ]
Porter, FS [1 ]
Schnopper, H [1 ]
Silver, EH [1 ]
Szymkowiak, AE [1 ]
Tucker, GS [1 ]
Walker, A [1 ]
Wollman, DA [1 ]
机构
[1] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
来源
EUV, X-RAY, AND GAMMA-RAY INSTRUMENTATION FOR ASTRONOMY X | 1999年 / 3765卷
关键词
Constellation-X; low temperature detector; microcalorimeter; spectroscopy; x-ray;
D O I
10.1117/12.366490
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Constellation-X is a cluster of identical observatories that together constitute a promising concept for a next-generation, high-throughput, high-resolution, astrophysical x-ray spectroscopy mission. The heart of the Constellation-X mission concept is a high-quantum-efficiency imaging spectrometer with 2 eV resolution at 6 keV. Collectively across the cluster, this imaging spectrometer will have twenty times the collecting efficiency of XRS on Astro-E and better than 0.25 are minute imaging resolution. The spectrometer on each satellite will be able to handle count rates of up to 1000 counts per second per imaging pixel for a point source and 30 counts per second per pixel for an extended source filling the array. Focal plane coverage of at least 2.5 are minutes x 2.5 are minutes, comparable to XRS but with a factor of thirty more pixels, is required. This paper will present the technologies that have the potential to meet all these requirements. It will identify the ones chosen for development for Constellation-X and explain why those were considered closer to realization, and it will summarize the results, of the development work thus far.
引用
收藏
页码:82 / 93
页数:12
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