| Stark broadening of neutral helium lines MS Dimitrijevic, S Sahal-Bréchot Journal of Quantitative Spectroscopy and Radiative Transfer 31 (4), 301-313, 1984 | 591* | 1984 |
| Stark widths of doubly-and triply-ionized atom lines. MS Dimitrijevic, N Konjevic Journal of Quantitative Spectroscopy and Radiative Transfer 24, 451-459, 1980 | 340 | 1980 |
| Experimental Stark widths and shifts for spectral lines of neutral atoms (a critical review of selected data for the period 1976 to 1982) N Konjević, MS Dimitrijević, WL Wiese Journal of physical and chemical reference data 13 (3), 619-647, 1984 | 309* | 1984 |
| Stark widths of doubly-and triply-ionized atom lines MS Dimitrijević, N Konjević Journal of Quantitative Spectroscopy and Radiative Transfer 24 (6), 451-459, 1980 | 280 | 1980 |
| Virtual atomic and molecular data centre ML Dubernet, V Boudon, JL Culhane, MS Dimitrijevic, AZ Fazliev, ... Journal of Quantitative Spectroscopy and Radiative Transfer 111 (15), 2151-2159, 2010 | 250 | 2010 |
| Simple estimates for Stark broadening of ion lines in stellar plasmas MS Dimitrijevic, N Konjevic Astronomy and Astrophysics (ISSN 0004-6361), vol. 172, no. 1-2, Jan. 1987, p …, 1987 | 232 | 1987 |
| Analysis of optical Fe II emission in a sample of active galactic nucleus spectra J Kovačević, LČ Popović, MS Dimitrijević The Astrophysical Journal Supplement Series 189 (1), 15, 2010 | 230 | 2010 |
| Stark broadening of Be II spectral lines MS Dimitrijević, S Sahal-Bréchot Journal of Quantitative Spectroscopy and Radiative Transfer 48 (4), 397-403, 1992 | 210* | 1992 |
| The virtual atomic and molecular data centre (VAMDC) consortium ML Dubernet, BK Antony, YA Ba, YL Babikov, K Bartschat, V Boudon, ... Journal of Physics B: Atomic, Molecular and Optical Physics 49 (7), 074003, 2016 | 186 | 2016 |
| The influence of Stark broadening on Cr II spectral line shapes in stellar atmospheres MS Dimitrijević, T Ryabchikova, Z Simić, LČ Popović, M Dačić Astronomy & Astrophysics 469 (2), 681-686, 2007 | 163* | 2007 |
| Electron-impact shifts of ion lines-Modified semiempirical approach MS Dimitrijevic, V Krsljanin Astronomy and Astrophysics (ISSN 0004-6361), vol. 165, no. 1-2, Sept. 1986 …, 1986 | 148 | 1986 |
| The flux ratio of the [O iii] λλ5007, 4959 lines in AGN: comparison with theoretical calculations MS Dimitrijević, LČ Popović, J Kovačević, M Dačić, D Ilić Monthly Notices of the Royal Astronomical Society 374 (3), 1181-1184, 2007 | 124 | 2007 |
| Stark broadening of visible Si II lines in stellar atmospheres T Lanz, MS Dimitrijevic, MC Artru Astronomy and Astrophysics (ISSN 0004-6361), vol. 192, no. 1-2, March 1988 …, 1988 | 115 | 1988 |
| A program to provide Stark-broadening data for stellar and laboratory plasma investigations MS Dimitrijević Journal of applied spectroscopy 63 (5), 684-689, 1996 | 106 | 1996 |
| Simple formulae for estimating Stark widths and shifts of neutral atom lines MS Dimitrijevic, N Konjevic Astronomy and Astrophysics (ISSN 0004-6361), vol. 163, no. 1-2, July 1986, p …, 1986 | 105 | 1986 |
| Stark broadening of Li II spectral lines MS Dimitrijevic, S Sahal-Bréchot Physica Scripta 54 (1), 50, 1996 | 103 | 1996 |
| Using the van der Waals broadening of the spectral atomic lines to measure the gas temperature of an argon microwave plasma at atmospheric pressure C Yubero, MS Dimitrijević, MC García, MD Calzada Spectrochimica Acta Part B: Atomic Spectroscopy 62 (2), 169-176, 2007 | 96 | 2007 |
| A decade with VAMDC: Results and ambitions D Albert, BK Antony, YA Ba, YL Babikov, P Bollard, V Boudon, F Delahaye, ... Atoms 8 (4), 76, 2020 | 93 | 2020 |
| Widths and shifts of isolated lines of neutral and ionized atoms perturbed by collisions with electrons and ions: An outline of the semiclassical perturbation (SCP) method and … S Sahal-Bréchot, MS Dimitrijević, N Ben Nessib Atoms 2 (2), 225-252, 2014 | 86 | 2014 |
| Stark broadening parameter tables for Mg I lines of interest for solar and stellar spectra research. I. MS Dimitrijevic, S Sahal-Bréchot Bulletin Astronomique de Belgrade, No. 149, p. 31-84 149, 31-84, 1994 | 86* | 1994 |
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