Toruń Centre For Astronomy
Radio astronomy
Since 1981 the observatory has been a part of worldwide network of radio telescopes participating in VLBI (Very Long Baseline Interferometry). The 32 m telescope is a 620-ton construction designed by Zygmunt Bujakowski based on initial geometric parameters created by Dr Jerzy Usowicz. It is used in VLBI experiments, as well as spectroscopic, flux, polarisation measurements and pulsar observations. Currently receivers for frequencies 1.4–1.8 GHz, 5 GHz, 6.5 GHz, 10.8 GHz and 30 GHz are in use.
The 15 m telescope is used for training students of the Nicolaus Copernicus University.
The observatory's role as a VLBI station is unique in central/eastern Europe. International collaboration and involvement in various European research projects is the major activity of this department. The research concentrates on observations and theoretical interpretation of physical processes in compact active regions of radio galaxies and quasars, observational cosmology, the timing of pulsars, the search for new planetary systems and Solar System studies. In addition, the development of instrumentation for radio astronomy (ultra low noise receivers, spectrometers, frequency converters, digital electronics, control systems) is also a significant part of activities in the observatory. From 1997 to 2019, the Department of Radio Astronomy was a part of what was known in publications as the Toruń Centre for Astronomy, at the Faculty of Physics, Astronomy and Applied Informatics of the Nicolaus Copernicus University in Toruń. From 1998, the department undertook the additional function of a National Facility with a major aims of serving Polish astronomers and emphasizing international cooperation.
Reorganisation of the university in the context of the 2018–2019 Law on higher education and science (Poland) led to the closing of the administrative structures of the Department of Radio Astronomy and the Department of Astronomy and Astrophysics. The astronomy research centre, without substructures, was recreated as the Institute of Astronomy starting on 1 October 2019.
WASP-3c & TTV
Transit Timing Variation (TTV), a variation on the transit method, was used to discover an exoplanet WASP-3c by Rozhen Observatory, Jena Observatory, and Toruń Centre for Astronomy.
See also
References
- ^ "Struktura organizacyjna Uniwersytetu Mikołaja Kopernika w Toruniu" [Organisational structure of Nicolaus Copernicus University in Toruń] (PDF). Nicolaus Copernicus University (in Polish). 2019-11-04. Archived (PDF) from the original on 2019-11-06. Retrieved 2019-11-06.
- ^ Lancaster, Katy; Birkinshaw, Mark; Gawroński, Marcin (2011). "Sunyaev-Zel'dovich observations of a statistically complete sample of galaxy clusters with OCRA-p". Monthly Notices of the Royal Astronomical Society. 418 (3): 1441–1451. arXiv:1106.3766. Bibcode:2011MNRAS.418.1441L. doi:10.1111/j.1365-2966.2011.19241.x.
- ^ "Planet Hunting: Finding Earth-like Planets".