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Expected performance and simulated observations of the instrument HARMONI at the European Extremely Large Telescope (E-ELT)

机译:欧洲超大型望远镜(E-ELT)对HARMONI仪器的预期性能和模拟观察

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HARMONI has been conceived as a workhorse visible and near-infrared (0.47-2.45 microns) integral field spectrograph for the European Extremely Large Telescope (E-ELT). It provides both seeing and diffraction limited observations at several spectral resolutions (R= 4000, 10000, 20000). HARMONI can operate with almost any flavor of AO (e.g. GLAO, LTAO, SCAO), and it is equipped with four spaxel scales (4, 10, 20 and 40 mas) thanks to which it can be optimally configured for a wide variety of science programs, from ultra-sensitive observations of point sources to high-angular resolution spatially resolved studies of extended objects. In this paper we describe the expected performance of the instrument as well as its scientific potential. We show some simulated observations for a selected science program, and compare HARMONI with other ground and space based facilities, like VLT, ALMA, and JWST, commenting on their synergies and complementarities.
机译:HARMONI被认为是欧洲超大型望远镜(E-ELT)的主力可见和近红外(0.47-2.45微米)积分场光谱仪。它在几个光谱分辨率(R = 4000、10000、20000)下提供了有限的观察和衍射观察。 HARMONI几乎可以使用任何口味的AO(例如GLAO,LTAO,SCAO)进行操作,并且配备了四个Spaxel秤(4、10、20和40 mas),因此可以针对各种科学进行最佳配置程序,从对点源的超灵敏观测到对扩展对象的高角度分辨率的空间分辨研究。在本文中,我们描述了该仪器的预期性能及其科学潜力。我们显示了对选定科学计划的一些模拟观察结果,并将HARMONI与其他地面和空间基础设施(例如VLT,ALMA和JWST)进行了比较,并评论了它们的协同作用和互补性。

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