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The Institute of Astronomy University of Zielona Góra was estabilished in 2000 at the Faculty of Mathematics, Physics and Technology of  School of education (WSP). At this time following professors joined the team: Piotr Amsterdamski, Roman Juszkiewicz, Włodek Kluźniak from Warsaw and Andrzej Maciejewski from Toruń. After the University of Zielona Góra was establised Institute of Astronomy was part of the Faculty of Science. In 2004 a new Department of Physics and Astronomy was formed which includes Institutes of Physics and Astronomy. Currently Institute of Astronomy employs four professors, three assistant professors and six doctors. Institute of Astronomy has a entitlement to conduct the direction ASTRONOMY with specialization in Computational Astrophysics. Since 2005, Faculty of Physics and Astronomy has a right to confer the degree of doctor of physical sciences in the field of Astronomy. In autumn 2005 the Braniborska Tower was completely restored and transformed into a modern astronomical observatory.

 

News



MAESTRO Grant

Two researches from the Department of Physics and Astronomy: prof. dr hab. Andrzej J. Maciejewski from Instutute of Astronomy and dr hab. Maria Przybylska from Instutute of Physics participate in the project entitled „Solvability, chaos and control in quantum systems". This project is headed by Prof. dr hab. Marek Kuś from Center for Theoretical Physics of the Polish Academy of Sciences in Warsaw.

Light pollution study of Zielona Góra

Light pollution study of Zielona Góra. A quick recording of various street lamps was done in an effort to map the light pollution around the observatory .

Equipment used The equipment was very simple .A diffraction grating with 300 lines per millimeter mounted in front of an 135mm telelens . The camera used was a CANON EOS 10D DSLR . The ISO setting was set to 800.

SN 2011dh in M51

Monitored from Braniborg Tower Observatory (BTO), Zielona Gora, Poland and Skinakas Observatory (SKO), Crete, Greece
We monitor supernova SN 2011dh that exploded in M51 in late May 2011. We are using both a 14-inch Meade LX200 telescope equipped with an SBIG ST-8XE CCD camera from BTO and the 1.3 m telescope in Skinakas Observatory. In BTO, we use either a clear filter and calibrate the images to SDSS g-band (with an alignment of 0.02 mag rms) or the V Bessel filter (not in the table yet). In SK, we use B, V, R, I, and H alpha filters.