Optical models of MXT using Zemax
暂无分享,去创建一个
The Microchannel X-ray Telescope (MXT) is a soft X-rays instrument on board SVOM, a Sino French mission. The launch is planned in 2021 by a LM-2C rocket. The main SVOM general objective is the survey of Gamma Ray Bursts, in coordination with ground telescopes. The other main on board instruments are ECLAIR (gamma, french), GRM (gamma, Chinese) and VT (visible, chinese).
[1] Juan M. Fontenla,et al. High‐resolution solar spectral irradiance from extreme ultraviolet to far infrared , 2011 .
[2] Forbes R. Powell,et al. Transmittance measurements for a variety of x-ray/EUV filter materials and pinhole leak measurements utilizing a new visible light photometer system , 1994, Optics & Photonics.
[3] Hot Stars: Old-Fashioned or Trendy? , 2002, astro-ph/0212226.
[4] George W. Fraser,et al. Hard X-ray imaging with microchannel plate optics , 1998 .