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LIINUS/SERPIL: a design study for interferometric imagingspectroscopy at the LBT

机译:LIINUS / SERPIL:LBT干涉成像光谱学的设计研究

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We present two design concepts and the science drivers of a proposed near-infrared interferometric integral field spectrograph for the LBT. This instrument will expand the capabilities of the currently-under-construction interferometric camera LINC-N1RVANA with spectroscopy by means of an integral field unit (IFU) located inside the LINC cryostat. Two instrument concepts have been studied in detail: a microlens array IFU with a spectrograph built entirely inside LINC (the LIINUS approach), and a lenslet+fibers IFU feeding an external spectrograph (the SERPIL approach). In both cases, the instrument incorporates imaging interferometry with integral field spectroscopy, an ideal combination for detailed studies of astronomical objects down to below 10mas angular resolution in the near-infrared. The scientific applications range from solar system studies and spectroscopy of exoplanets to the dynamics of stars and gas in the central regions of the Milky Way and other nearby galaxies.
机译:我们介绍了LBT的拟议近红外干涉积分场光谱仪的两个设计概念和科学驱动力。该仪器将通过位于LINC低温恒温器内的积分现场单元(IFU)扩展具有光谱学的当前在建干涉仪LINC-N1RVANA的功能。已经详细研究了两个仪器概念:一个微透镜阵列IFU,其光谱仪完全内置在LINC内部(LIINUS方法),以及小透镜+光纤IFU供给外部光谱仪(SERPIL方法)。在这两种情况下,该仪器都将成像干涉仪与积分场光谱仪结合在一起,这是详细研究近红外角分辨率低于10mas的天文物体的理想组合。科学应用范围从太阳系研究和系外行星的光谱学到银河系中部和其他附近星系的恒星和气体动力学。

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