论文标题
纳斯科的新型多光束接收器和望远镜控制系统的开发
Development of the new multi-beam receiver and telescope control system for NASCO
论文作者
论文摘要
我们报告了NASCO(Nanten2 Super Co调查作为旧版项目)的当前状态,该项目旨在使用Nanten2 4-M亚毫米望远镜通过开发新的多梁接收机和一个新的望远镜控制系统,使用Nanten2 4-M亚毫米望远镜提供南半球的全sky Co数据立方体。接收器由5个梁组成。四个梁位于正方形的四个角,梁分离为720 $''$,安装了一个100 GHz频带SIS接收器,具有2偏振边界分离滤波器。另一个位于光轴上的光束安装了一个具有200 GHz带SIS接收器,具有2极化侧带分离滤波器。为每个梁模块化冷却的成分,并使用冷却的镜子。对于100和200 GHz频段的IF带宽分别为8和4 GHz。使用带宽为2 GHz的XFFTS光谱仪,$^{12} $ CO,$^{13} $ CO和C $^{18} $ o of $ j $ = 1 $ - $ - $ - $ = 2 $ = 2 $ = 2 $ - $ 1的行可同时观察到每个光束。控制系统是在ROS架构上重建的,ROS架构是机器人控制的开源框架,以实现灵活的观察模式并处理大量数据。该框架通常在机器人领域中使用和维护,因此与先前使用的系统相比,可靠性,灵活性,可扩展性和开发效率得到提高。接收器和控制系统于2019年12月安装在Nanten2望远镜上,其调试和科学验证正在进行中。我们计划在2021年初开始科学运营。
We report the current status of the NASCO (NAnten2 Super CO survey as legacy) project which aims to provide all-sky CO data cube of southern hemisphere using the NANTEN2 4-m submillimeter telescope installed at the Atacama Desert through developing a new multi-beam receiver and a new telescope control system. The receiver consists of 5 beams. The four beams, located at the four corners of a square with the beam separation of 720$''$, are installed with a 100 GHz band SIS receiver having 2-polarization sideband-separation filter. The other beam, located at the optical axis, is installed with a 200 GHz band SIS receiver having 2-polarization sideband-separation filter. The cooled component is modularized for each beam, and cooled mirrors are used. The IF bandwidths are 8 and 4 GHz for 100 and 200 GHz bands, respectively. Using XFFTS spectrometers with a bandwidth of 2 GHz, the lines of $^{12}$CO, $^{13}$CO, and C$^{18}$O of $J$=1$-$0 or $J$=2$-$1 can be observed simultaneously for each beam. The control system is reconstructed on the ROS architecture, which is an open source framework for robot control, to enable a flexible observation mode and to handle a large amount of data. The framework is commonly used and maintained in a robotic field, and thereby reliability, flexibility, expandability, and efficiency in development are improved as compared with the system previously used. The receiver and control system are installed on the NANTEN2 telescope in December 2019, and its commissioning and science verification are on-going. We are planning to start science operation in early 2021.