The first quarter of the postdoctoral project has been completed
June 30, 2025
March 1, 2025 – June 30, 2025
The first operational quarter and the month of June, in accordance with the project "Revealing the physical mechanism of mass ejection around young massive stars via CH3OH masers" plan, were marked by the first mobility period, in which postdoc researcher Artis Aberfelds visited the project partner – the Cagliari Astronomical Observatory (OAC), which is part of the Italian National Institute for Astrophysics (INAF).
During this period, I acquired the necessary knowledge to process data obtained using the Very Large Array (VLA) network of radio telescopes (see Figure 1). A standardized approach was developed to be applied to all 40 sources included in the survey of early evolutionary stage massive stars.
One of the most significant early results was the detection of 6.7 GHz methanol maser emission in the G240.32+0.07 star-forming region (Figure 2). The brightness of this source is four times lower than the theoretical sensitivity limit of the Irbene RT-32 radio telescope.
Figure 1. The VLA is a Y-shaped radio telescope array located in the United States, consisting of 28 antennas, each with a diameter of 25 meters. (Image from Wikipedia)
Figure 2. Map of the newly detected 6.7 GHz methanol masers (blue dots) toward the G240.32+0.07 source. The contours show the intensity of thermal emission. The brightest source in the center has already begun ionizing atoms. In contrast, the source to the right is more than ten times fainter and is at an earlier evolutionary stage. The observed methanol masers are associated with this source.
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On September 1 of this year, Ventspils University of Applied Sciences launched a new European Union (EU) co-funded project “Modernization of the Study Environment of Ventspils University of Applied Sciences”, No. 4.2.1.8/2/25/I/007. The project implementation period is 24 months, until August 31, 2027. The project aims to ensure the modernization of the study environment of Ventspils University of Applied Sciences, which includes the improvement and development of the infrastructure of the bachelor's study program "Computer Science" and the professional bachelor's study program "Electronics Engineering". To ensure high-quality and competitive education, targeted measures will be implemented within the project framework, focusing on the technological modernization of study spaces, enhancing the material and technical base, and introducing information and communication technologies (ICT). These engineering and IT programs are strategically important for the sustainable economic growth of the Ventspils region and the entire country of Latvia, preparing highly qualified specialists to promote digital transformation and technological development. During the project, the infrastructure of laboratories and classrooms will be enhanced to ensure that study rooms are equipped with the latest technologies and meet the standards of modern higher education. The latest technologies and equipment will be purchased and introduced, significantly expanding students' opportunities to work with current industry tools and software, thereby preparing them to work with technologies widely used in the industry. In addition, it is planned to continue adapting the digital infrastructure to modern requirements, allowing for the implementation of the hybrid and distance learning process in accordance with current educational trends. The modernization carried out will significantly improve the quality of studies and compliance with labour market requirements, providing students with the opportunity to acquire practical skills and adapt to the growing requirements of the industry. This project will not only improve the study environment and promote the integration of innovations into the learning process, but will also contribute to the development of Ventspils University of Applied Sciences as a higher education and research center in Latvia and beyond, attracting students from the region and the country, as well as from abroad. The total cost of the project “Modernization of the study environment of Ventspils University of Applied Sciences”, No. 4.2.1.8/2/25/I/007, is 215,083.00 EUR, of which the planned amount of the European Regional Development Fund is 85% of the eligible expenses – 182,820.55 EUR, and the amount of state funding is 15% of the eligible costs – 32,262.45 EUR.
We are pleased to invite you to participate in the VIRAC Summer School on Pulsar Observations at Centimetre and Metre Wavelengths: Ventspils, Latvia |September 8–19, 2025 This intensive and inspiring summer school is designed for Master’s students, PhD candidates, and early-career researchers in astronomy and astrophysics. The event is hosted by Ventspils University of Applied Sciences. Key Topics: Pulsar observations with the LOFAR telescope Pulsar astronomy fundamentals Observation planning Pulsar data processing and analysis Venue: Engineering Research Institute – Ventspils International Radio Astronomy Centre, Ventspils University of Applied Sciences, Room 407
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Today, the field of radio astronomy has experienced a resurgence in ‘transient’ science, with more and more astronomical phenomena found to be active on timescales of months, weeks, and even within a single day. For example, high-mass stars form in short, intense bursts of mass accretion that display active variations on day-long timescales. The use of single-baseline interferometers (two telescopes connected together) has been known in astronomy since the 1940s. However, demand for this observing technique was soon overtaken by the development of interferometers comprising large numbers of radio telescope dishes. As demand for aperture synthesis arrays increased, the time available for each observing programme became more limited. The recent emphasis on transient science has renewed the demand for facilities capable of high-cadence monitoring of brightness variations in radio emission—an area in which the now uncommon single-baseline radio interferometer is particularly well suited. The aim of this project is the development of the Irbene Single-Baseline Interferometer (ISBI), designed to detect variations in the radio emission associated with high-mass star-forming regions. The ISBI will be used to monitor both radio continuum and maser emission from high-mass protostars. This will enable clearer distinctions to be drawn between currently untested and competing theoretical models proposed to explain the enigmatic variability recently linked to the formation of high-mass stars. With recent discoveries confirming rapid accretion bursts in high-mass protostars, time-domain radio astronomy has become a key frontier in understanding the formation of massive stars. These short-lived accretion episodes give rise to measurable variations in both radio continuum and maser emission. However, existing large-scale arrays are often oversubscribed and are not optimised for long-term, targeted monitoring of such sources. “The method will enable clearer distinctions to be drawn between currently untested and competing theoretical models proposed to explain the enigmatic variability recently linked to the formation of high-mass stars.” High-cadence, long-term monitoring, such as that possible by ISBI, greatly benefits from automation, which makes it much easier to carry out long-term, frequent monitoring of space signals, from planning observations to processing the data. Latvian scientists have created a unique set of tools and automated systems for the ISBI, turning it into a one-of-a-kind instrument with capabilities not found anywhere else. ISBI stands out because, unlike single-dish telescopes or large VLBI arrays, it can both detect weak signals and track them regularly over time. This makes it ideal for studying the changing radio emissions of massive star-forming regions, helping researchers understand processes like matter falling onto stars and the jets they eject. Thanks to automation, almost the whole workflow runs smoothly, allowing continuous and efficient monitoring of these fascinating cosmic events.
