BlackGEM (BG) is an array of telescopes, currently under development at the Radboud University Nijmegen and at NOVA. It targets the detection of the optical counterparts of gravitational waves. The first 3 BG telescopes are planned to be installed in 2018 at the La Silla observatory. A single prototype telescope, named MeerLICHT, will already be commissioned early 2017 in Sutherland to provide an optical complement for the MeerKAT radio array. The BG array consists of, initially, a set of 3 robotic 65-cm wide-field telescopes. Each telescope is equipped with a single STA1600 CCD detector with 10.5k x 10.5k 9-mum pixels that covers a 2.7 square degrees field of view. The cryostats for housing these detectors are developed and built at the KU Leuven University. The operational model of BG requires long periods of reliable ands-off operation. Therefore, we designed the cryostats for long vacuum hold time and we make use of a closed-cycle cooling system, based on Polycold PCC Joule-Thomson coolers. A single programmable logic controller (PLC) controls the cryogenic systems of several BG telescopes simultaneously, resulting in a highly reliable, cost-efficient and maintenance-friendly system. PLC-based cryostat control offers some distinct advantages, especially for a robotic facility. Apart of temperature monitoring and control, the PLC also monitors the vacuum quality, the power supply and the status of the PCC coolers (compressor power consumption and temperature, pressure in the gas lines, etc.). Furthermore, it provides an alarming system and safe and reproducible procedures for automatic cool down and warm up. The communication between PLC and higher-level software takes place via the OPC-UA protocol, offering a simple to implement, yet very powerful interface. Finally, a touch-panel display on the PLC provides the operator with a user-friendly and robust technical interface.
翻译:BlackGEM (BG) 是一系列望远镜,目前正在Radboud大学尼杰梅根和NOVA开发中。 它的目标是探测重力波的光学对等器。 计划于2018年在La Silla观测台安装头3 BG望远镜。 一个名为MeerLICHT的单一原型望远镜将在2017年初委托萨瑟兰为MeerKAT的无线电阵列提供一个光学补充。 BG阵列最初由一套3个机械式温度为65厘米的宽空望远镜组成。 每台望远镜都配有一台STA1600C 的电压对等器。 每台望远镜配有一台STA1600 C 电压对等器, 一台10.5k 10.5k 9毫米像素的光学检测器, 覆盖2.7平方度的观测场。 安装这些探测器的加密望远镜的加密望远镜。 BG的操作模型需要很长一段时间的可靠操作时间。 因此, 我们设计了长真空的冷冻器, 我们用了一个闭式的冷控系统, 以PO-LC 并且提供了一个在PC 级的系统中, 提供了一个更高级的高级的 。