Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Faculty of Physics, University of Belgrade, P.O. Box 368, Studentski Trg 14, 11001 Belgrade, Serbia and Montenegro.
Faculty of Physics, University of Belgrade, 11001 Belgrade, PO Box 368, Serbia; Isaac Newton Institute of Chile, Yugoslavia Branch, Belgrade, Serbia
Faculty of Physics, University of Belgrade, 11 001 Belgrade, PO Box 368, Serbia
Faculty of Physics, University of Belgrade PO Box 368, 11000 Belgrade, Serbia, Yugoslavia
Faculty of Physics, Studentski Trg 12-16, 11000 Belgrade, Serbia
Faculty of Physics, University of Belgrade, Studentski trg 12-16, P.O.Box 368, 11000 Belgrade, Serbia
Faculty of Physics, University of Belgrade, 11001 Belgrade, PO Box 368, Serbia, Yugoslavia; Isaac Newton Institute of Chile, Yugoslavia Branch, Belgrade, Yugoslavia
Faculty of Physics, University of Belgrade, 11001 Belgrade, PO 368, Serbia; Isaac Newton Institute of Chile, Yugoslavia Branch, Belgrade, Serbia
Faculty of Physics, University of Belgrade, PO Box 368, Belgrade, Serbia
Faculty of Physics, University of Belgrade, Studentski trg 12-16, P.O. Box 368, 11 000 Belgrade, Serbia of Physics, University of Belgrade, POB 368, Belgrade, Serbia; Isaac Newton Institute of Chile, Yugoslavia Branch, Belgrade, Serbia
Faculty of Physics, University of Belgrade, Studentski Trg 12-16, Belgrade, Serbia of Physics, University of Belgrade 11001 Belgrade, POB 368, Serbia; Isaac Newton Institute of Chile, Yugoslavia Branch, Belgrade, Serbia
Faculty of Physics, University of Belgrade, PO Box 368, 11000 Belgrade, Serbia, Yugoslavia
Faculty of Physics, University of Belgrade, Studentski trg 14, Belgrade, Serbia of Physics, University of Belgrade, Studentski trg 14, 11000 Belgrade, Serbia
Faculty of Physics, PO Box 368, 11000, Belgrade, Serbia
Faculty of Physics, University of Belgrade, 11001 Belgrade, POB 368, Serbia, Yugoslavia; Isaac Newton Institute of Chile, Yugoslavia Branch, Belgrade, Yugoslav
Advanced fit technique for astrophysical spectra (Bukvic+, 2008)
Advanced fit technique for astrophysical spectra. Approach insensitive to a large fraction of outliers
An alternative approach to data processing
An alternative approach to spectrum base line estimation
Bowen Fluorescence, Stark Broadening, and Transition Probabilities in the O III Spectrum
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