Real-Time Survey for Rapid Source Variability in Astronomical Objects using the Very Large Array

对显示时间迅速变化的来源的研究是天文学最后的前沿之一。这涵盖了很宽的波长范围。在无线电范围内，我们的太阳在20世纪40年代被发现了变化。在20世纪60年代，天文光源的缓慢时间变化被发现。后来，人们发现了发射规则脉冲的射电源。在过去的几年里，发现了不重复的爆发源。其中一组最具能量的射电源是快速射电暴，简称frb。快速射电暴是一种罕见现象。对快速射电暴的研究是一个新的领域，它们的距离和确切位置是一个悬而未决的问题。如果快速射电暴位于其他星系，这种爆发的能量将达到可能的发射机制的极限。短暂现象的吸引力应引起广泛的公众兴趣。学生将学习时变天体物理学、高性能计算和高效算法等主题。该项目将构建一个系统，用于在使用甚大阵列（VLA）进行的预定成像观测期间搜索瞬态现象。图像是由许多小时内的平均数据生成的。然而，快速变化的证据在平均过程中丢失了。该项目将建立一个系统，用于在50毫秒到分钟的时间尺度上搜索数据的变化，与预定的天文项目并行。这些搜索将实时进行。在实时系统中，只有那些显示出显著射电能量爆发的样本才会被存储。这个系统将在任何时候都在使用，当标准的科学项目进行时，即一个共生系统。在这种情况下，来自VLA的数据流将被一个强大的、特别设计的系统搜索，以寻找显著的、短期的无线电能量爆发。这不会影响利用VLA进行的正常科学观测。VLA可以很容易地提供误差小于1角秒的FRB位置，允许光学识别。该系统将利用VLA的大量观测时间，包括分配给已经计划好的VLA巡天的6000小时。该项目是未来大型设施计划的先驱，如平方公里阵列。学生们将有很多机会学习在大数据集中搜索瞬态事件的算法，国家射电天文台的网站也将提供拓展服务。

The study of sources showing rapidly time variability is one of last frontiers of astronomy. This covers a wide range of wavelengths. In the radio range, variations had been found for our Sun in the 1940s. In the 1960s, slow time variations of astronomical sources were discovered. Later, radio sources emitting regular pulses were found. In the last few years, non-repeating, bursting sources have been found. One group of the most energetic radio sources is Fast Radio Bursts, or FRBs. FRBs are a rare phenomenon. The study of FRBs is a new one, and their distance and exact location is an open question. If the FRBs are located in other galaxies, the energy of such outbursts would reach the limits of possible emission mechanisms. The appeal of transient phenomena should provide wide public interest. There will be student in topics such as time variable astrophysics, high performance computing and efficient algorithms. This project will construct a system to search for transient phenomena during scheduled imaging observations made with the Very Large Array (VLA). Images are produced from the average of data over many hours. However, the evidence for rapid variations is lost in the averaging process. This project will construct a system designed to search the data for variability on time scales from 50 milliseconds to minutes, in parallel with scheduled astronomical programs. These searches will be carried out in real time. With the real-time system, only those samples showing significant bursts of radio energy would be stored. This system will be in use at all times when standard scientific programs are carried out, that is, a commensal system. In this, the data stream from the VLA will be searched for significant, short term bursts of radio energy with a powerful, especially designed system. This will not affect the normal scientific observations made with the VLA. The VLA can easily provide FRB positions that have errors smaller than 1 arc second, allowing optical identifications. This system will take advantage of the large amount of observing time available at the VLA, including the 6000 hours to be allocated to the already-planned VLA Sky Survey. This project is a precursor for larger facilities planned for the future, such as the Square Kilometer Array. There will be many opportunities for student training in the algorithms used to search for transient events in large data sets, and there will be outreach at the website of the National Radio Astronomy Observatory.