首页> 外文会议>International Astronautical Congress >43rd SYMPOSIUM ON THE SEARCH FOR EXTRATERRESTRIALINTELLIGENCE (SETI) - The Next Steps (A4) SETI 1: SETI Science and Technology (1):RADIO SEARCHES FOR EXTRATERRESTRIAL INTELLIGENCE AS FACILITY OBSERVING PROGRAMS
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43rd SYMPOSIUM ON THE SEARCH FOR EXTRATERRESTRIALINTELLIGENCE (SETI) - The Next Steps (A4) SETI 1: SETI Science and Technology (1):RADIO SEARCHES FOR EXTRATERRESTRIAL INTELLIGENCE AS FACILITY OBSERVING PROGRAMS

机译:43题目关于extrasterRestrialIntelligence的搜索研讨会(SETI) - 下一步(A4)Seti 1:Seti Science和Technology(1):无线电搜索外星智力作为设施观察程序

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The vast majority of radio searches for extraterrestrial intelligence (SETI) are conducted using specialized purpose-built hardware and software, largely due to their unique signal processing requirements. This differs markedly from radio astronomy in general, in which a small collection of digital instruments and software packages can be used to conduct a wide range of experiments with varied scientific goals. Because of the relatively high cost and steep learning curve associated with the use of dedicated hardware and software, it has historically been difficult for new SETI practitioners to conduct their own observational programs, and as a result most SETI experiments are conducted by only a few scientists. In the last several years, the radio astronomy digital instrumentation landscape has changed significantly and custom integrated circuits are being replaced by commercial compute elements like field programmable gate arrays (FPGAs) and commodity CPUs/GPUs. In addition to being much more capable, these new instruments are also much more configurable than their predecessors. It has now become possible to conduct high sensitivity searches for extraterrestrial intelligence using only the digital instrumentation provided by observatory facilities, offering the prospect of SETI observing becoming as routine as continuum mapping or pulsar searching. Here we will present the status of our group's facility-SETI observing efforts at several observatories,including the Green Bank Telescope, the Arecibo Observatory and the Low Frequency Array (LOFAR). We will describe targeted and survey SETI observations we are conducting at these facilities and also detailing an open-source SETI software pipeline, currently under development, that is capable of processing data in many formats and employing a range of search algorithms.
机译:大多数广播搜索外星智能(SETI)使用专业的专用硬件和软件进行,主要是由于它们独特的信号处理要求。这通常是从射频天文学的显着不同,其中可以使用小集合数字仪器和软件包来进行各种科学目标的实验。由于与使用专用硬件和软件相关的成本和急剧学习曲线相对较高,新的SETI从业者历史上难以进行自己的观测程序,因此,只有少数科学家们进行大多数SETI实验。在过去的几年中,无线电天文数字仪表景观发生了显着变化,并且自定义集成电路正在由现场可编程门阵列(FPGA)和商品CPU / GPU等商业计算元件所取代。除了更具能力之外,这些新仪器也比他们的前辈更具可配置。现在可以仅使用天文台设施提供的数字仪器来对外星智能进行高敏感性搜索,提供SETI观察的前景作为常规作为连续映射或脉冲脉搜索的常规。在这里,我们将在几个观察者,包括绿色银行望远镜,槟榔天文台和低频阵列(Loofar),介绍我们集团的设施 - Seti观察努力的地位。我们将描述我们在这些设施中进行的有针对性的和调查确定的观察,并且还详细说明目前正在开发的开源Seti软件管道,其能够以多种格式处理数据并采用一系列搜索算法。

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