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VLBI NETWORK SIMULATOR: AN INTEGRATED SIMULATION TOOL FOR RADIO ASTRONOMERS KCI 등재 SCOPUS

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  • URLhttps://db.koreascholar.com/Article/Detail/383968
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천문학회지 (Journal of The Korean Astronomical Society)
한국천문학회 (Korean Astronomical Society)
초록

In this paper we introduce a software package, the Very long baseline interferometry Network SIMulator (VNSIM), which provides an integrated platform assisting radio astronomers to design Very Long Baseline Interferometry (VLBI) experiments and evaluate the network performance, with a userfriendly interface. Though VNSIM is primarily motivated by the East Asia VLBI Network, it can also be used for other VLBI networks and generic interferometers. The software package not only integrates the functionality of plotting (u; v) coverage, scheduling the observation, and displaying the dirty and CLEAN images, but also adds new features including sensitivity calculations for a given VLBI network. VNSIM provides exible interactions on both command line and graphical user interface and o ers friendly support for log reports and database management. Multi-processing acceleration is also supported, enabling users to handle large survey data. To facilitate future developments and updates, all simulation functions are encapsulated in separate Python modules, allowing independent invoking and testing. In order to verify the performance of VNSIM, we performed simulations and compared the results with other simulation tools, showing good agreement.

목차
Abstract
1. INTRODUCTION
2. THE VNSIM
    2.1. Overall Design
    2.2. Software Framework
3. MAJOR FUNCTIONS
    3.1. Simulation Functions
    3.2. Additional Functions
4. EXAMPLE EXPERIMENTS
    4.1. (u,v) Plotting of a Single Source
    4.2. (u,v) Plotting of Multiple Sources
    4.3. Dirty and CLEAN Images
5. SUMMARY
REFERENCES
저자
  • Zhen Zhao(Shanghai Astronomical Observatory, Key Laboratory of Radio Astronomy, Chinese Academy of Sciences)
  • Tao An(Shanghai Astronomical Observatory, Key Laboratory of Radio Astronomy, Chinese Academy of Sciences) Corresponding author
  • Baoqiang Lao(Shanghai Astronomical Observatory, Key Laboratory of Radio Astronomy, Chinese Academy of Sciences)