1. Astrophysical spectroscopy of extragalactic objects – Research at AOB Лука Ч. Поповић (Luka C. Popovic)

3. AGN Some of the investigation will be present at the Conference by Edi, Dragana, Natasha and Jelena

5. Gravitational lens Some of our work will be present at the Conference by Predrag and Tihomir

6. GRB (see presentation of Sasha)

7. Some of the papers: Popovic, L. C., Jovanovic, P., Mediavilla, E. G., Zakharov, A.F., Munoz, J. A., Chartas, G. 2006 ApJ, 637, pp. 620. - lens Popovic, L. C., Chartas, G. 2005, MNRAS, 357, 135 – lens Simic, S., Andersen, M.I., Popovi'c, L. C., Christensen, L. 2005., AIPCS, 801, 139. – GRB model Popovic, L. C., Mediavilla, E., Bon, E.,Ilic, D., 2004, A&A., 423, 909 – AGN, BLR kinematics Zakharov, F., Popovic, L. C., Jovanovic,P. 2004, A&A., 420, 881 - Lens Christensen, L., Snchez, S. F., Jahnke, K., Becker, T., Wisotzki, L., Kelz, A., Popovic, L. C., Roth, M. M. 2004,A&A, 417, 487 – AGN, extended regions Popovic, L. C., Mediavilla, E.G., Bon, E.,Ilic, D., Richter, G. 2004, Astron. Nachr., 325, 376 – AGN, HII regions Arbutina, B., Urosevic, M. Stankovic, and Lj. Tesic, 2004, MNRAS,350, 346 – supernova remnants Popovic L. C. 2003, ApJ, 599, 140 – AGN, BLR physics Popovic L. C., Mediavilla E., Bon E.,Stanic N. \& Kubicela A. 2003, ApJ, 599, 185 – AGN, BLR kinematics Popovic, L. C., Mediavilla, E. G., Jovanovic, P.; Munoz, J. A.: 2003, A&A, 398, 975 – X-ray, microlensing

8. Participants 1.Еди Бон, (рођ. 1970, АОБ) from 2002 to 2005.- 42 m. 2.Наташа Гавриловић, (рођ. 1979, АОБ) only 2005.- 3 m 3.Милан С. Димитријевић, (рођ. 1947, АОБ) from 2002 to 2005. - 8 m 4. Драгана Илић (рођ. 1978, МФБ) from 2002 to 2005. total 32 m 5.Катарина Ковач (рођ. 1976, АОБ) only in 2002. total 8 m 6.Предрага Јовановић, (рођ. 1968, АОБ) from 2002 to 2005. - 18 m 7.Л. Ч. Поповић, (рођ. 1964, АОБ) from 2002 to 2005. - 40 m 8.Срђан Самуровић (рођ. 1967, АОБ) from 2002 to 2004. - 36 m 9.Саша Симић (рођ. 1971, ФФК) from 2002 to 2005. - 32 m 10.Наташа Станић (рођ. 1969, АОБ) from 2002 to 2004 - 29 m 11.Деајан Урошевић (рођ. 1970, МФБ) from 2002 to 2004. - 6 m 12.Милан Ћирковић (рођ. 1971, АОБ) from 2002 to 2004. - 12 m ------------------------------------------------------------------------------------------------ Total 266 m (born in 1970. with work during 22.2 years.)

9. Results Published over 100 papers (23 in journals from SCI list as ApJ, MNRAS, A&A, Phys. Scr., A&A SS, etc.) Defended 2 PhD thesis (1 at Bel. Univ., and 1 at Univ. of Trieste) Defended 4 MSc thesis (1 Uni. of Padova, Diploma th.) Organized 3 conferences (Serb.-Bulg. 2004, SCSLSA – 2003 and 2005) Participation in the international projects (e.g. SANU and BAN with Bulgaria, program ‘Pavle Savic’ with Lyon, RAN and SANU, etc.) Observation at big telescopes (PI was participants of the Project) Etc. (in more details in the paper that will be published in the Proceedings)

10. Other activity: Development of international collaboration (Bulgaria, Russia, Germany, France, Greece, Italy, SAD, etc.) Popularization of the astronomy Participation in SOC, LOC, Editorial board of SAJ, PAOB, PASRB, etc. Missions at different institutes Etc. (in more details in the Proceedings)

11. Financed by Ministry of Science of Serbia Three categories which have been financed through project: 2005. 1. Salaries 1995940 2. Support financial sources (e.g. traveling, conference fee, page charges, etc.) - SFS 517000 3. Administrative expenses – AE 831204 Total 3 344 144 din 2004. 1. Salaries + AE3183174 2. SFS 88709 Total 3 271 883 din 2002-2003. 1. Salaries + AE 4218270 2. SFS 210914 Total 4 429 184 din --------------------------------------------------------------------------------------------------- Total 2002-2005 11 045 211 din (~130 000 Еur. ~ 35000 Eur/year)

12. Future? Our proposal for the project in the perod of 2006. – 2010 is accepted Now our group has 9 researchers (3 MSc students, 3 PhD students, 1 postdoc, and 2 senior researchers) – total 82 i.m./year Investigations: (i) AGNs from central part to the extended stellar structure; (ii) Gravitational lens – influence on the spectra of lensed QSOs; (iii) Gamma ray bursts; (iv) spectral line shape phenomena from starts to the QSOs

13. Ok, let us investigate!