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First interferometric observations in Irbene - Torun baseline conducted by VIRAC

  • V. Bezrukovs*
  • , J. Shteinbergs
  • , I. Shmeld
  • , A. Aberfelds
  • , M. Bleiders
  • , A. Orbidans
  • , K. Skirmante
  • , M. Gawronski
  • , R. Feiler
  • *Corresponding author for this work

Research output: Contribution to journalConference articlepeer-review

Abstract

Ventspils International Radio Astronomy Centre (VIRAC, Latvia) operates two radio telescopes, RT-16 and RT-32 accordingly, with fully steerable 16- and 32-m Cassegrain type antennas. The main receiving systems of the both telescopes are cryogenic receivers with 4.5–8.8 GHz frequency range. Additionally, in 2019 radio telescope RT-32 will be equipped with a new L band receiver. Data registration units of the both antennas are suitable for interferometric observations. The Nicolaus Copernicus University Department of Radio Astronomy in Torun, Poland, operates a 32-m radio telescope RT-4, which also works in similar bands – L, C and M – and regularly participates in the VLBI observations. Moreover, VIRAC possesses a high-performance computer cluster with SFXC software correlator developed at JIVE. In the spring 2018, VIRAC team with support from Torun group conducted several VLBI experiments in the baseline Irbene–Torun using the Irbene RT-16 radio telescope and Torun RT-4 radio telescope. Successful fringes and FITS files with obtained uv data implies that data correlation and post processing facilities established in VIRAC allow to run small-scale interferometric tasks.

Original languageEnglish
JournalProceedings of Science
Volume344
Publication statusPublished - 2018
Externally publishedYes
Event14th European VLBI Network Symposium and Users Meeting, EVN 2018 - Granada, Spain
Duration: 8 Oct 201811 Oct 2018

Keywords

  • Correlation
  • Galactic masers
  • Radio astronomy
  • SFXC
  • VIRAC
  • VLBI observations

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