Vladislavs Bezrukovs (Ventspils International Radio Astronomy Centre): Ventspils International Radio Astronomy Centre (VIRAC): overview of facilities and recent results
Ventspils International Radio Astronomy Centre (VIRAC) of Ventspils University of Applied Sciences (VUAS) was established in 1994 with the aim to develop the research activities in radio astronomy, astrophysics and space sciences. The most important instrumental base for the centre comprised two fully steerable parabolic antennas, RT-16 and RT-32 (i.e. with the mirror diameter of 16 m and 32 m) and LOFAR-LATVIA station. The intensive reconstruction and instrumental refurbishment carried out in 2014 – 2019 made it possible to use radio telescopes for the international scale fundamental and applied research in the field of radio astronomy. The most important aspect of this work is participation in the VLBI (Very Long Baseline Interferometry) international experiments. During the renovation, radio telescopes were instrumented with two channel right circular polarization (RCP) and left circular polarization (LCP) cryogenic broad band receivers with frequency coverage of 4.5 – 8.8 GHz and instantaneous bandwidth of approx. 1200 MHz. Receivers are cryogenically cooled to 14 Kelvin which nominally achieves system noise temperatures of 30 to 50 Kelvin throughout the whole bandwidth. A secondary receiver is available at RT-32 for observations at 1.40 to 1.72 GHz. It is an uncooled receiver with dual (RCP and LCP) polarization channels and achieves system temperatures of 60 to 100 K. Each telescope has VLBI equipment available, which includes Active Hydrogen masers, DBBC/Mark5c/FlexBuff data registration back-ends and 10 Gbit optical fibre network. Maximum azimuth and elevation tracking velocities are up to 5 degrees/s with RMS tracking accuracies 4 arcsec allowing to track Near Earth satellites.
Additionally, radio telescope RT-32 performs routine spectral polarimetric observations of the Sun by the multi-channel (16 frequency channels) spectral polarimeter for the wavelength range 3.2 – 4.7 cm (6.3 - 9.3 GHz) and both circular polarizations. The new multi-channel spectral polarimeter, installed in 2022 is expected to observe right and left circular polarization of the solar emission in the wavelength range 2.1 – 7.5 cm (4.1 – 14.3 GHz) divided into 12 frequency bands. The dynamic range of the receiver is up to 36 db; the signal/noise ratio (referred to quiet Sun brightness temperatures) is 22-24 db.
The LOFAR-Latvia is an international LOFAR station (IS). It contains 96 low band (LBA) (10 - 90 MHz, total area 3200 sq.m) and 96 high band (HBA) (110 - 240 MHz, total area 2400 sq.m) antennas.
One of the main scientific objectives for the VIRAC centre is VLBI observations in centimetre and meter wavelengths in collaboration with the global VLBI networks, such as European VLBI network (EVN), LOFAR, IVS and others. The new receiving and recording systems provide a high stability of the time frame, which is a prerequisite for the VLBI observations. Since October 2015 VIRAC radio telescopes have regularly taken part in international VLBI sessions. VIRAC is a member of pan-European networks such as CERN (Member State since 2021), International Low Frequency Array (LOFAR) Telescope (ILT) since 2019, European VLBI (EVN) and JIV-ERIC networks since 2016.
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Open Funder Deadlines
Due to the implementation of a new UKRI funding system (TFS) there will be a fixed quarterly deadlines for some grants which would previously have been on open calls, this is to allow necessary system amendments and updates.
The first deadline after implementation will be 28th September 2023 and applies to those calls listed below: