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Pomenis: A small portable astrograph for SSA

机译:Pomenis:SSA的小型便携式天体

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The Steward Observatory SSA team developed the Pomenis Astrograph System as an alternative to more traditional narrow field of view small SSA systems. The astrograph is innovative with its fast optical design versus a traditional longer focal length found on commercial Cassegrain telescope that most "Raven class" systems are based on. Compared with other systems used for SSA, the Pomenis astrograph has an exceptionally wide 4.2°x4.2° field of view and a fast readout CCD camera. These features enable synoptic survey of the deep space satellite population several times per night. The aperture and focal length were carefully selected to achieve sensitivity relevant to synoptic GEO SSA with an integration time short enough to allow high precision astrometric reference using the streaked background stars. With its 7-color filter wheel, Pomenis also performs multi-color photometric screening of deep space satellites looking for anomalous behavior and can identify objects for higher fidelity measurements and study. Pomenis is housed in a unique trailer mounted enclosure, which enables the system to be deployed with minimal infrastructure, operated remotely and autonomously, and quickly relocated as required. In addition to the SSA measurements described above, the astrograph is taking full-hemisphere night sky brightness (NSB) measurements in multiple color bands. These measurements will be compared to previously conducted each decade on Mt. Hopkins and Kitt Peak to study the increase in light pollution in southern Arizona. Pomenis will allow these measurements to be made on a more routine basis, and over a tighter spatial grid. This will facilitate our monitoring of the light pollution environment at the University's observatory sites and assess the impact of future development on the quality of the night sky. Additionally, Pomenis will be used for serendipitous astronomical surveys and to develop new techniques for precise photometric reduction over a wide field of vie
机译:管家天文台SSA团队开发了POMENIS天体乐乐系统,作为更传统的狭窄视野小型SSA系统的替代方案。天体乐乐乐乐乐乐乐都是具有快速光学设计的创新性,而在商用Cassegrain望远镜上发现的传统较长的焦距,大多数“乌鸦级”系统是基于的。与用于SSA的其他系统相比,Pomenis天体乐乐乐乐乐乐乐乐乐乐乐乐谱具有出色的4.2°x4.2°视野和快速读数CCD摄像头。这些功能使得每晚几次深度空间卫星人口的概要调查。孔径和焦距被仔细选择,以实现与Synoptic Geo SSA相关的灵敏度,其具有足够短的整合时间,以允许使用条纹的背景恒星允许高精度的星形测量值。凭借其7滤色器轮,Pomenis还对寻找异常行为的深空卫星进行多色光度筛选,可以识别用于更高保真度测量和研究的对象。 Pomenis坐落在独特的拖车安装机箱中,使系统能够以最少的基础设施部署,远程和自主操作,并根据需要快速重新安置。除了上述SSA测量外,天体乐乐仪在多个色带中采用全半球夜空亮度(NSB)测量。将与先前对Mt.Hopkins和Kitt Peak进行比较,以研究南亚利桑那州南部光污染的增加。 Pomenis将允许这些测量更加常规,并且在更严格的空间网格上进行。这将促进我们对大学的天文台遗址的光污染环境监测,并评估未来发展对夜空质量的影响。此外,Pomenis将用于偶然的天文调查,并开发新技术,用于在宽阔的vie领域进行精确的光度降低

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