List of Participants
No | Name | Surname | Country | Contribution | Institution |
1 | Bojan | Arbutina | Serbia | Radial dependence of extinction in parent galaxies of supernovae (P) |
Astronomical Observatory Belgrade |
2 | Paul | Barklem | Sweden | The broadening of spectral lines by collisions with neutral hydrogen atoms in cool stars (IL) |
Uppsala University |
3 | Nebil | Ben Nessib | Tunisa | Experimental and theoretical determination of temperature in plasmas (IL) |
Faculté des Sciences de Bizerte, Tunisia |
4 | Edi | Bon | Serbia | The Broad Ha and Hb emission line shapes in an AGN sample (ST) |
Astronomical Observatory Belgrade |
5 | Viacheslav F. | Boretskij | Ukraine | Shapes of spectral lines of nonuniform plasma of electric arc discharge between copper electrodes (ST) | Radiophysics Dept. Taras Schevchenko Kyiv National University |
6 | George | Chartas | USA | Absorption Line Diagnostics of Quasar Outflows (IL) | Penn State University |
7 | Eleni | Chatzichristou | Greece | Studding the complex absorption and emission lines in AGNs spectra (ST) |
Institute of Astronomy and Astrophysics, National Observatory of Athens |
8 | Magdalena | Christova | Bulgaria | On the broadening of spectral lines in surface waves sustained discharges (IL) |
Technical University-Sofia |
9 | Miodrag | Dacic | Serbia | Stark broadening of Cr II spectral lines in stellar atmospheres |
Astronomical Observatory Belgrade |
10 | Emmanouel | Danezis | Greece | The DACs and SACs effects from stars to Quasars. Some first general notices (IL) |
University of Athens, Faculty of Physics, Department of Astrophysics, Astronomy and Mechanics |
11 | John | Danziger | Italy | Profiles in Novae Spectra (IL) | Astronomical Observatory Trieste |
12 | Milan | Dimitrijevic | Serbia | Stark broadening of Cr II spectral lines in stellar atmospheres (ST) |
Astronomical Observatory Belgrade |
13 | Natasa | Gavrilovic | Serbia | Connection between central black hole and circum-nuclear gas kinematics: The case of AGN with double-peaked lines (P) |
Astronomical Observatory Belgrade |
14 | Derek | Homeier | Germany | Collisional Broadening of Na I in Metal-rich White Dwarfs - Beyond the Single Perturber Approximation (ST) | Institut für Astrophysik Göttingen, Georg-August-Universität Göttingen |
15 | Dragana | Ilic | Serbia | Physical properties of the BLR: Boltzmann-Plot vs. CLOUDY calculations (ST) |
Department of Astronomy, Faculty of Mathematics, University of Belgrade |
16 | Zeljko | Ivezic | USA | SDSS Spectroscopic Survey(s) (IL) | University of Washington |
17 | Darko | Jevremovic | Serbia | The influence of Chemi-Ionization and Chemi-Recombination Processes on H lines in M Dwarf Atmospheres(P) | Astronomical Observatory Belgrade |
18 | Predrag | Jovanovic | Serbia | The shape of the Fe Ka spectral line in the case of partly obscured accretion disk (ST) |
Astronomical Observatory Belgrade |
19 | Andrei N. | Klyucharev | Russia | Chemi-ionization processes. Alkali-metal geocosmical plasmas (IL) |
St Petersburg State University / Research Institute of Physics |
20 | Wolfram | Kollatschny | Germany | Line Profile Variability in AGNs (IL) | Institut für Astrophysik Göttingen, Georg-August-Universität Göttingen |
21 | Jelena | Kovacevic | Serbia | Asymmetry of the CIV 1549 line in a sample of RQ and RL AGN (P) |
Astronomical Observatory Belgrade |
22 | Andjelka | Kovacevic | Serbia | Lag Between the Optical Continuum and Line Variabilities of NGC 4151 (P) |
Department of Astronomy, Faculty of Mathematics, University of Belgrade |
23 | Giovanni | La Mura | Italy | Detailed analysis of Balmer Lines in a selected sample of 90 broad line AGN (ST) |
Dipartimento di Astronomia, Universita di Padova |
24 | Evaggelia | Lyratzi | Greece | The evolution of some physical parameters in the DACs/SACs regions in Be stellar atmospheres (ST) | University of Athens, Faculty of Physics, Department of Astrophysics, Astronomy and Mechanics |
25 | Anatolij A. | Mihailov | Serbia | The influence of ion-atom and atom-Rydberg atom processes to the continuous and line spectra of star's atmospheres (P) |
Institute of physics |
26 | Zarko | Mijajlovic | Serbia | Stellar Spectroscopy on the New Astronomical Station at the Mountain Vidojevica (P) |
Faculty of Mathematics, University of Belgrade |
27 | Nenad | Milovanovic | Serbia | Cowan Code and Stark Broadening of Spectral Lines of S II, S III and S IV (ST) | Astronomical Observatory Belgrade |
28 | Alexei | Moiseev | Russia | The jet-clouds interaction in AGN: a panoramic spectroscopy view (IL) | Special Astrophysical Observatory of RAS |
29 | Slobodan | Ninkovic | Serbia | Studies of Local Milky-Way Kinematics via Line-of-Sight Velocities (IL) |
Astronomical Observatory Belgrade |
30 | Gillian | Peach | UK | Recent work on line shapes for the spectra of cool stars (IL) |
Department of Physics and Astronomy, University College London |
31 | Nada | Pejovic | Serbia | Stellar Spectroscopy on the New Astronomical Station at the Mountain Vidojevica (P) |
Department of Astronomy, Faculty of Mathematics, University of Belgrade |
32 | Zoran | Petrovic | Serbia | Electron, ion and atom collisions leading to anomalous Doppler broadening in hydrogen and hydrogen rare gas mixtures (IL) |
Institute of physics |
33 | Luka | Popovic | Serbia | Astronomical Observatory Belgrade | |
34 | Philippe | Prugniel | France | Modeling the spectrum of the stellar population in star forming and active galaxies (IL) |
CRAL-Observatoire de Lyon |
35 | Jagos | Puric | Serbia | Stark parameters regularities of multiply charged ions spectral lines originating from the same transition array (IL) |
Faculty of Physics, University of Belgrade |
36 | Piero | Rafanelli | Italy | 3D spectroscopy of nuclear and extranuclear regions of nearby AGN (IL) |
Dipartimento di Astronomia, Universita di Padova |
37 | Mikhail | Sachkov | Russia | Pulsation tomography of roAp stars (IL) | Institute of astronomy RAS |
38 | Nenad | Sakan | Serbia | The modeling of the continuous emission spectrum of a dense non-ideal plasma in optical region (ST) | Institute of physics |
39 | Zoran | Simic | Serbia | Experimental and theoretical stark widths for Au II (P) | Astronomical Observatory Belgrade |
40 | Sasa | Simic | Serbia | Spectral lines in the afterglow of Gamma Ray Bursts (ST) | University of Kragujevac, Faculty of Science, Department of Physics |
41 | Aleksandrina | Smirnova | Russia | Mrk334: connection between nuclei activity and merging of a companion (ST) |
Special Astrophysical Observatory of RAS |
42 | Vladimir | Sreckovic | Serbia | The modeling of the continuous emission spectrum of a dense non-ideal plasma in optical region (ST) | Institute of physics |
43 | Ilija | Stefanovic | Germany | Plasma analogue for astrophysical dust (IL) | Institute for Experimental Physics II, Ruhr University Bochum |
44 | Paolo | Tozzi | Italy | Emission lines in X--ray spectra of Clusters of Galaxies (IL) |
INAF Osservatorio Astronomico di Trieste |
45 | Dejan | Urosevic | Serbia | Optical search for supernova remnants in M81, M82 and NGC 3077 (P) |
Department of Astronomy, Faculty of Mathematics, University of Belgrade |
46 | Sonja | Vidojevic | Serbia | Correlation Line-of-Sight Velocity-Metallicity in a Sample of Stars with Possible Planetary Systems (ST) |
Department of Astronomy, Faculty of Mathematics, University of Belgrade |
47 | Branislav | Vukotic | Serbia | Optical search for supernova remnants in M81, M82 and NGC 3077 (P) |
Astronomical Observatory Belgrade |
48 | Alexander | Zakharov | Russia | The Fe K-alpha line simulations for BHs: the simplest model (IL) |
State Scientific Center - Institute of Theoretical and Experimental Physics |