Architecture and Implementation of a 25000 FPS Radio Camera on the Long Wavelength Array

Karthik Reddy, Judd D. Bowman, Jayce Dowell, Greg B. Taylor, Adam P. Beardsley, Craig Taylor

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

A highly optimized E-field Parallel Imaging Correlator (EPIC), currently under commissioning on the Long Wavelength Array in Sevilleta, New Mexico, can image the sky at a rate of 25,000 FPS per polarization and frequency. The system consists of six processing nodes, each producing images of the visible sky with a 1-degree spatial resolution at an 80 ms temporal resolution, covering a 3.2 MHz spectral window below 100 MHz, yielding a total bandwidth of 19.2 MHz. Light curves for selected sources of interest will be extracted from each image into a distributed database, and 5-minute accumulations are archived on the disk for further analysis. In this paper, we describe the components of our real-time imaging system, designed as a plug-and-play solution to deploy EPIC on similar arrays with only minor modifications.

Original languageEnglish (US)
Title of host publicationSoftware and Cyberinfrastructure for Astronomy VIII
EditorsJorge Ibsen, Gianluca Chiozzi
PublisherSPIE
ISBN (Electronic)9781510675254
DOIs
StatePublished - 2024
EventSoftware and Cyberinfrastructure for Astronomy VIII 2024 - Yokohama, Japan
Duration: Jun 16 2024Jun 21 2024

Publication series

NameProceedings of SPIE - The International Society for Optical Engineering
Volume13101
ISSN (Print)0277-786X
ISSN (Electronic)1996-756X

Conference

ConferenceSoftware and Cyberinfrastructure for Astronomy VIII 2024
Country/TerritoryJapan
CityYokohama
Period6/16/246/21/24

Keywords

  • EPIC
  • Long Wavelength Array
  • Real-time radio imaging
  • System Architecture

ASJC Scopus subject areas

  • Electronic, Optical and Magnetic Materials
  • Condensed Matter Physics
  • Computer Science Applications
  • Applied Mathematics
  • Electrical and Electronic Engineering

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