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Single-baseline interferometer for mJy observations

  • J. Šteinbergs*
  • , A. Aberfelds
  • , V. Bezrukovs
  • , K. Šķirmante
  • , A. Orbidans
  • , I. Shmeld
  • , R. A. Burns
  • *Corresponding author for this work
  • Ventspils University College
  • National Astronomical Observatory of Japan
  • Korea Astronomy and Space Science Institute

Research output: Contribution to journalConference articlepeer-review

Abstract

The Ventspils International Radio Astronomy Centre (VIRAC) of Ventspils University of Applied Sciences (VeUAS) has developed an 800 m single-baseline interferometer consisting of 32 m (IR) and 16 m (IB) radio telescopes with 15 arcseconds of angular resolution. Irbene radio telescopes are operating at C/M/X-band (4.5-8.8 GHz). Raw telescope data are correlated with the Software FX Correlator (SFXC) [1] and output visibilities are calibrated with a ParselTongue pipeline. Data processing techniques provide a velocity resolution of 0.088 kms-1 and spectral resolution of 0.002 MHz and enabling observations to approach the theoretical sensitivity limit of the interferometer, at about 6 mJy for a 120 s integration. We propose to use the Irbene interferometer for discoveries in a new age of transient astrophysics. In this paper, we will show correlation and calibration schema and initial monitoring results.

Original languageEnglish
Article number033
JournalProceedings of Science
Volume399
Publication statusPublished - 2021
Externally publishedYes
Event2021 European VLBI Network Mini-Symposium and Users' Meeting, EVN 2021 - Virtual, Online
Duration: 12 Jul 202114 Jul 2021

Keywords

  • Galactic masers
  • high-mass protostars
  • ParselToung
  • SFXC
  • VLBI observations

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