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BTFI2: a simple, light and compact Fabry-Perot instrument for the SOAR telescope

机译:BTFI2:SOAR望远镜的简单,轻巧,紧凑的法布里 - 珀罗仪器

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We present the concept of a new Fabry-Perot instrument called BTFI-2, which is based on the design of another Brazilian instrument for the SOAR Telescope, the Brazilian Tunable Filter Imager (BTFI). BTFI-2 is designed to be mounted on the visitor port of the SOAR Adaptive Module (SAM) facility, on the SOAR telescope, at Cerro Pachón, Chile. This optical Fabry-Perot instrument will have a field of view of 3 x 3 arcmin, with 0.12 arcsec per pixel and spectral resolutions of 4500 and 12000, at H-alpha, dictated by the two ICOS Fabry-Perot devices available. The instrument will be unique for the study of centers of normal, interacting and active galaxies and the intergalactic medium, whenever spatial resolution over a large area is required. BTFI-2 will combine the best features of two previous instruments, SAM-FP and BTFI: it will use an Electron Multiplication detector for low and fast scanning, it will be built with the possibility of using a new Fabry-Perot etalon which provides a range of resolutions and it will be light enough to work attached to SAM, and hence the output data cubes will be GLAO-corrected.
机译:我们提出所谓BTFI-2新的法布里 - 珀罗仪器,它是基于对SOAR望远镜,巴西可调滤波器成像仪(BTFI)另一个巴西仪器的设计理念。 BTFI-2被设计成安装在SOAR自适应模块(SAM)设施的访问者端口上,在SOAR望远镜,在山帕琼,智利。该光学法布里 - 珀罗器械将具有图3×3弧分的场,每个像素和的4500和12000光谱分辨率,在H-阿尔法0.12弧秒,通过可用的两个ICOS法布里 - 珀罗设备所决定的。该仪器将用于正常中心的研究独特,互动和活动星系和星系际介质,无论何时需要在大面积的空间分辨率。 BTFI-2将结合前面两个仪器,SAM-FP和BTFI的最佳特性:它会使用慢速和快速扫描的电子倍增探测器,它将使用新的法布里 - 珀罗标准具,其提供的可能性,建分辨率的范围,这将是足够轻,以附连到SAM的工作,因此输出数据立方体将GLAO校正。

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