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NeXT的使命

The NeXT Mission

T. Takahashi, R. Kelley, K. Mitsuda, H. Kunieda, R. Petre, N. White, T. Dotani, R. Fujimoto, Y. Fukazawa, K. Hayashida, M. Ishida, Y. Ishisaki, M. Kokubun, K. M… 展开作者

T. Takahashi, R. Kelley, K. Mitsuda, H. Kunieda, R. Petre, N. White, T. Dotani, R. Fujimoto, Y. Fukazawa, K. Hayashida, M. Ishida, Y. Ishisaki, M. Kokubun, K. Makishima, K. Koyama, G. M. Madejski, K. Mori, R. Mushotzky, K. Nakazawa, Y. Ogasaka, T. Ohashi, M. Ozaki, H. Tajima, M. Tashiro, Y. Terada, H. Tsunemi, T. G. Tsuru, Y. Ueda, N. Yamasaki, S. Watanabe, the NeXT team

摘要:

NeXT(新探索X射线望远镜)是继朱雀之后的新的日本X射线天文卫星,是一项国际X射线任务,目前计划于2013年发射。NeXT是由多层涂层、聚焦硬X射线镜和硬X射线成像探测器提供的宽带X射线光谱(3 - 80 keV)和由薄箔X射线光学器件和微量热计阵列提供的高能量分辨率软X射线光谱(0.3 - 10 keV)的组合。该飞行任务还将携带一台X射线CCD照相机作为软X射线望远镜的焦平面探测器和一台非聚焦软伽马射线探测器。有了这些仪器,NeXT涵盖了从0.3 keV到600 keV的非常宽的能量范围。微量热计系统将由ISAS/JAXA和NASA牵头的国际合作开发。同时的宽带通,再加上高光谱分辨率的Δ E ~ 7 eV的微量热计将使各种重要的科学主题被追求。

英文摘要:

The NeXT (New exploration X-ray Telescope), the new Japanese X-ray Astronomy Satellite following Suzaku, is an international X-ray mission which is currently planed for launch in 2013. NeXT is a combination of wide band X-ray spectroscopy (3 - 80 keV) provided by multi-layer coating, focusing hard X-ray mirrors and hard X-ray imaging detectors, and high energy-resolution soft X-ray spectroscopy (0.3 - 10 keV) provided by thin-foil X-ray optics and a micro-calorimeter array. The mission will also carry an X-ray CCD camera as a focal plane detector for a soft X-ray telescope and a non-focusing soft gamma-ray detector. With these instruments, NeXT covers very wide energy range from 0.3 keV to 600 keV. The micro-calorimeter system will be developed by international collaboration lead by ISAS/JAXA and NASA. The simultaneous broad bandpass, coupled with high spectral resolution of Delta E ~ 7 eV by the micro-calorimeter will enable a wide variety of important science themes to be pursued.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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