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Science with UT's Dichroic-mirror Camera (DMC),15-band Simultaneous Imager

机译:科学与UT的二向色镜相机(DMC),15频段同声成像仪

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We introduce the Dichroic-Mirror Camera (DMC), an instrument devel oped at the University of Tokyo which is capable of performing simultaneous imaging in fifteen bands. The main feature of the DMC is the dichroic mirrors, which split incoming light into red and blue components. Combination of dichroic mirrors split light from the telescope focus into fifteen intermediate-width bands across 390 - 950 nm. The fifteen bands of DMC provide measurements of the object's spectral energy distribution (SED) at fifteen wavelength points. During May - June 2007 and March 2008, observing run of the DMC was carried out at Higashi-Hiroshima Observatory, Japan. We observed several objects i.e. planets, asteroids, standard stars & star clus ters, planetary nebulae, galaxies, and supernovae. We describe several early scientific results from the DMC.
机译:我们介绍了Dicroic-Mirror Camera(DMC),该仪器在东京大学开放,能够在十五条频段中进行同时成像。 DMC的主要特征是二向色镜,将输入光分成红色和蓝色组件。二向色反射镜的组合从望远镜分开光,焦点390-950nm的十五个中间宽度带。 DMC的十五条带提供了十五个波长点的物体光谱能量分布(SED)的测量。在2007年5月和2008年3月期间,DMC的观察竞选是在日本的Higashi-Higaroshima天文台进行。我们观察了几个物体,即行星,小行星,标准星星和星系,行星星云,星系和超新星。我们描述了DMC的几种早期科学结果。

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