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____________________________________________________________ ɋɜ. 15 No. 15 PROCEEDINGS OF THE IX BULGARIAN-SERBIAN ASTRONOMICAL CONFERENCE: ASTROINFORMATICS Sofia, Bulgaria, July 2-4, 2014 Eds. Milcho K. Tsvetkov, Milan S. Dimitrijeviü, Ognyan Kounchev, Darko Jevremoviü and Katya Tsvetkova Ȼ ȿ Ɉ Ƚ Ɋ Ⱥ Ⱦ 2015 _________________________________________________________________________ _________________________________________________________________________ SCIENTIFIC COMMITTEE LOCAL ORGANIZING COMMITTEE Ognyan Kounchev (Co-chairman) Ognyan Kounchev (Co-chairman) Darko Jevremoviü (Co-chairman) Milcho K. Tsvetkov (Co-chairman) Milan S. Dimitrijevi Scientific secretary: Viktoria Naumova ü Milcho K. Tsvetkov Luka ý. Popoviü Members: Zoran Simiü Žarko Mijajloviü Anna Sameva Katya Tsvetkova Katya Tsvetkova Vasil Popov Svetlana Boeva Nikola Petrov Momchil Dechev Petko Nedialkov Damyan Kalaglarsky Under the auspices of Bulgarian Academy of Sciences Ministry of Education, Science and Technological Development of Serbia ORGANIZERS: Institute of Mathematics and Informatics of Bulgarian Academy of Sciences Astronomical Observatory Belgrade, Serbia Co-organizers: Institute of Astronomy with National Astronomical Observatory, BAS Department of Astronomy, Faculty of Physics, Sofia University “St. Kliment Ohridski” Faculty of Mathematics and Department of Astronomy, University of Belgrade Society of Astronomers of Serbia Cover design: Tatjana Milovanov Text arrangement by computer: Tatjana Milovanov Published and copyright © by Astronomical Society “Rudjer Boškoviü”, Kalemegdan, Gornji Grad 16, 11000 Belgrade, Serbia President of the Astronomical Society “Rudjer Boškoviü”: Miodrag Daþiü Financially supported by the Ministry of Education, Science and Technological Development of Serbia ISBN 978-86-89035-06-3 __________________________________________________________________ Production: Solution+, Bulevar umetnosti 27, 11070 Beograd, in 100 copies CONTENTS Darko Jevremović ASTROINFORMATICS IN SERBIA 7 Alexander A. Kolev ASTROWEB ASTROINFORMATICS PROJECT AND COMPARISON OF THE WEB-GIS PROTOCOL STANDARDS 13 Milan S. Dimitrijević, Sylvie Sahal-Bréchot, Nicolas Moreau and Nabil Ben Nessib STARK-B DATABASE FOR STARK BROADENING FOR ASTROPHYSICAL PLASMA ANALYSIS AND MODELLING 23 Katya Tsvetkova UV CETI TYPE VARIABLE STARS PRESENTED IN THE GENERAL CATALOGUE OF VARIABLE STARS 29 Jovan Aleksić, Veljko Vujčić and Darko Jevremović ALERT SIMULATOR - SYSTEM FOR SIMULATING DETECTION OF TRANSIENT EVENTS ON LSST 37 Nikolay Kirov, Milcho Tsvetkov and Katya Tsvetkova WFPDB: SOFTWARE FOR TIME AND COORDINATES CONVERSIONS 43 Zoran Simić, Milan S. Dimitrijević and Luka Č. Popović ATOMIC DATA AND STARK BROADENING OF Nb III 49 Damyan Kalaglarsky, Katya Tsvetkova and Milcho Tsvetkov WFPDB: UPGRADING THE CATALOGUE OF WIDE-FIELD PLATE ARCHIVES AND RECENT DEVELOPMENT 55 Cristina Yubero, Maria Carmen García, Milan S. Dimitrijević, Antonio Sola and Antonio Gamero ON THE DETERMINATION OF ELECTRON DENSITY IN NON- THERMAL PLASMAS USING BALMER SERIES HYDROGEN LINE 63 Alexandra M. Zubareva, Daria M. Kolesnikova, Kirill V. Sokolovsky, Sergei V. Antipin and Nikolai N. Samus VARIABLE STARS NEAR β CAS DISCOVERED ON SCANNED PHOTOGRAPHIC PLATES AT THE STERNBERG ASTRONOMICAL INSTITUTE 67 3 Saša Simić and Luka Č. Popović BROAD SPECTRAL LINE AND CONTINUUM VARIABILITIES IN QSO SPECTRA INDUCED BY MICROLENSING: METHODS OF COMPUTATION 75 Andjelka Kovačević, Luka Č. Popović, Alla I. Shapovalova, and Dragana Ilić TIME SERIES ANALYSIS OF AGNs 83 Daniela Boneva FLUCTUATIONS IN THE FLOW AND DEVELOPMENT OF FLARE-UPS IN COMPACT BINARY STARS 93 Zorica Cvetković, Slobodan Ninković, Rade Pavlović, Svetlana Boeva and Georgi Latev DETERMINATION OF NATURE FOR ELEVEN DOUBLE STARS 99 Krasimira Yankova BEHAVIOUR OF THE FLOW ON THE BOUNDARY IN THE SYSTEM DISK-CORONA 107 Momchil Dechev, Kostadinka Koleva, Peter Duchlev and Nikola Petrov MULTI-WAVELENGTH OBSERVATIONS OF AN ERUPTIVE PROMINENCE ON 7 AUGUST 2010 117 Cyril Ron, Jan Vondrák and Yavor Chapanov ATMOSPHERIC, OCEANIC AND GEOMAGNETIC EXCITATION OF NUTATION 127 Aleksandra Nina, Vladimir M. Čadež, Luka Č. Popović, Vladimir A. Srećković and Saša Simić DIFFERENCES IN DETECTION OF D-REGION PERTURBATIONS INDUCED BY THE UV, X AND γ RADIATION FROM OUTER SPACE USING VLF SIGNALS 137 Boris Komitov, Momchil Dechev and Peter Duchlev THE RELATION BETWEEN SOLAR PROTON FLARES AND THE BACKGROUND CONCENTRATIONS OF NITROGEN OXIDES IN THE TROPOSPHERE 149 Zlatko Majlinger, Zoran Simić and Milan S. Dimitrijević ON THE STARK BROADENING OF Zr IV IN THE SPECTRA OF DB WHITE DWARFS 159 4 Goran Damljanović, Francois Taris, Georgi Latev and Milan Stojanović OBSERVATIONS AT THE 60 cm ASV TELESCOPE AND THE LINK GAIA CRF - ICRF 165 Katya Tsvetkova, Milan S. Dimitrijević and Milcho Tsvetkov THE MATHEMATICIAN AND THE ASTRONOMER SIMON MARIUS (1573 – 1624) 171 Nada Pejović, Saša Malkov, Nenad Mitić and Žarko Mijajlović MILUTIN MILANKOVIĆ DIGITAL LEGACY 179 Milan S. Dimitrijević SOCIETY OF ASTRONOMERS OF SERBIA 2012-2014 189 AUTHORS’ INDEX 207 5 Proceedings of the IX Bulgarian-Serbian Astronomical Conference: Astroinformatics (IX BSACA) Sofia, Bulgaria, July 2-4, 2014, Editors:M.K.Tsvetkov,M.S.Dimitrijevi´c, O. Kounchev, D. Jevremovi´candK.Tsvetkova Publ. Astron. Soc. ”Rudjer Boˇskovi´c” No 15, 2015, 7-12 ASTROINFORMATICS IN SERBIA DARKO JEVREMOVIC´ Astronomical Observatory, Volgina 7, 11060 Belgrade, Serbia E-mail: [email protected] Abstract. I review some aspects of development of the astroinformatics in Serbia. Special attention is paid to the funding and educational challenges. As we recently joined the LSST project, we expect huge impact on Serbian science especially in the Big Data areas. Among others, our contribution will be in building simulator of alerts for the astronomical community and prototype of the CEP engine for analyzing data generated by the survey. 1. OVERVIEW OF ASTRONOMY IN SERBIA There are two main institutions with significant number of astronomers in Serbia: Astronomical Observatory in Belgrade (AOB) and Department of Astronomy, Fac- ulty of Mathematics, Belgrade University (DAFM). AOB employs about twenty re- searchers with PhD at different stages of their career and about fifteen PhD students. DAFM has about ten tenured/tenure track professors and about 15 Phd students. There are few astronomers at other institutions such as Institute of Physics Belgrade, Institute of Nuclear Sciences Vinˇca, Department of Physics University of Kragujevac, Department of Physics University of Niˇs, Department of Physics University of Novi Sad. Funding of Astronomy (and generally science) in Serbia is grant based. Serbian Government currently funds the following eight projects with significant astronomical component: ◦ Astrophysical Spectroscopy of Extragalactic Objects (led by Luka Popovi´c) ◦ Gravitation and the large scale structure of the Universe (Predrag Jovanovi´c) ◦ Emission nebulae: structure and evolution (Dejan Uroevi´c) ◦ Influence of collisions on astrophysical plasma spectra (Milan Dimitrijevi´c, Zo- ran Simi´c) ◦ Stellar physics (Gojko Djuraˇsevi´c) ◦ Visible and Invisible Matter in Nearby Galaxies: Theory and Observations (Srdjan Samurovi´c) ◦ Dynamics and kinematics of celestial bodies and systems (Zoran Kneˇzevi´c, Rade Pavlovi´c) ◦ Astroinformatics: application of IT in astronomy and close fields (Darko Jevre- movi´c). 7 D. JEVREMOVIC´ 1. 1. INTERNATIONAL COLLABORATION Astronomers from Serbia were and are involved in many internationally funded projects. The first European project we were involved was Virtual Atomic and Molecular Data Center VAMDC (Dubernet et al. 2010, Jevremovi´c et al. 2009). More details in section 2.1.3. Project BELISSIMA (BELgrade Initiative for Space Science, Instrumentation and Modeling in Astrophysics) started in 2010. It is funded by European Comission under the FP7 REGPOT schema. The BELISSIMA will be concluded in June 2015. Main goals are: ◦ Reinforcement of the scientific potential of AOB (and, therefore, Serbian as- tronomical and space sciences) through increase of both width and depth of its overall research activities, observational and theoretical, as a consequence of ”brain gain”. This will be operational on several levels, in both theoretical and observational aspects of envisioned future research activity. ◦ Purchase, installation and testing of new observing equipement (telescope ”Mi- lankovi´c” with1.5 m-class mirror, to be installed on Astronomical Station Vi- dojevica ◦ Human potential, training and public outreach. Exchange of know-how and experience between EU research institutes and AOB. Training of AOB re- searchers in observational astronomy techniques and work towards establishing collaboration with other observatories in Europe and worldwide ◦ Popularization of Astronomy and Science Stardust, the Asteroid and Space Debris Network, is an Advanced research net- work we participate in. One PhD student from Greece started his PhD thesis work at AOB in the September of the last year. Astromundus is a master program in astrophysics. Five universities are involved - namelly Insbruck, Goettingen, Padova, Rome and Belgrade. Typically, 4-6 students attend classes in Belgrade during the fall semester of the second year of their course. Also, few students are doing their master thesis research in the final semester in Bel- grade (either under our supervision or under joint supervision between two partners). We actively participate in the following COST actions: ◦ MP0905 - Black Holes in a Violent Universe 24 March 2010 - 01 June 2014 ◦
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    Iveigh Ivones Izearde Izzach Izzox Ivelan Ivoomb Izeart Izzack Izzoyd Iveland Ivoombe Izech Izzacke Izzsard Ivelane Ivor Izeck Izzaech Izzude Ivelant Ivors Izerd Izzaeck Izzume Ivelen Ivory Izert Izzaick Izzyck Ivelend Ivvaren Izett Izzaitch Izzyke Ivelent Ivy Iziac Izzake Ivelind Ivye Izick Izzaock Ivelint Ivymey Izitch Izzaox Ivelyn Ivys Izock Izzard Ivelynd Iwadby Izod Izzarde Ivemey Iwardbey Izode Izzarn Ivemmy Iwardby Izoed Izzarne Ivemy Iwardy Izoit Izzart Iveney Iwerdby Izold Izzarte Ivens Iwoodby Izombe Izzat Iver Ix Izon Izzatt Iverach Ixton Izood Izzayck Iverack Iyon Izoode Izzayke Iveragh Iyone Izoold Izzeard Iverake Iyonne Izoomb Izzearde Iverech Izaac Izoombe Izzeart Ivereck Izaach Izord Izzech Iverick Izaack Izould Izzeck Iveritch Izaacs Izoyd Izzerd Iverock Izaacson Izrael Izzert Iverox Izaake Izraeler Izzett Ivers Izach Izraely Izzick Iverson Izack Izreeli Izzitch Ivery Izacke Izsard Izzock Iveryck Izaech Izsarde Izzod Iveryke Izaeck Izsardt Izzode Ives Izaick Izsart Izzoed Iveson Izaitch Izsarte Izzoit Ivet Izake Izseard Izzold Ivett Izaock Izsearde Izzolm Ivetts Izaox Izseart Izzomb Ivey Izard Izserd Izzombe Ivie Izarde Izsert Izzome Ivimey Izarn Izsord Izzone Ivinges Izarne Izude Izzood Ivington Izart Izyck Izzoode Ivinney Izarte Izyke Izzoold Ivins Izat Izzaac Izzoom Ivinson Izatson Izzaach Izzoomb Iviormy Izatt Izzaack Izzoombe Ivison Izayck Izzaacs Izzord Ivombe Izayke Izzaacson Izzould Ivone Izeard Izzaake Izzown Hall of Names by Swyrich © 1999 Swyrich Corporation www.swyrich.com 1-888-468-7686 557 Jackline Jacok
  • Are the Orbital Poles of Binary Stars in the Solar Neighbourhood Anisotropically Distributed?

    Are the Orbital Poles of Binary Stars in the Solar Neighbourhood Anisotropically Distributed?

    A&A 574, A6 (2015) Astronomy DOI: 10.1051/0004-6361/201323056 & c ESO 2015 Astrophysics Are the orbital poles of binary stars in the solar neighbourhood anisotropically distributed? J.-L. Agati1,D.Bonneau2, A. Jorissen3,E.Soulié4,S.Udry5,P.Verhas6, and J. Dommanget†,7 1 13 rue Beyle Stendhal, 38000 Grenoble, France 2 Laboratoire Lagrange, UMR 7293, Univ. Nice Sophia-Antipolis, CNRS, Observatoire de la Côte d’Azur, 06300 Nice, France e-mail: [email protected] 3 Institut d’Astronomie et d’Astrophysique, Université Libre de Bruxelles, CP 226, Boulevard du Triomphe, 1050 Brussels, Belgium 4 CEA/Saclay, DSM, 91191 Gif-sur-Yvette Cedex, France 5 Observatoire de Genève, Chemin des Maillettes, 1290 Sauverny, Suisse 6 251 vieille rue du Moulin, 1180 Brussels, Belgium 7 Observatoire Royal de Belgique, Avenue Circulaire 3, 1180 Bruxelles, Belgique Received 15 November 2013 / Accepted 30 October 2014 ABSTRACT We test whether or not the orbital poles of the systems in the solar neighbourhood are isotropically distributed on the celestial sphere. The problem is plagued by the ambiguity on the position of the ascending node. Of the 95 systems closer than 18 pc from the Sun with an orbit in the 6th Catalogue of Orbits of Visual Binaries, the pole ambiguity could be resolved for 51 systems using radial velocity collected in the literature and CORAVEL database or acquired with the HERMES/Mercator spectrograph. For several systems, we can correct the erroneous nodes in the 6th Catalogue of Orbits and obtain new combined spectroscopic/astrometric orbits for seven systems [WDS 01083+5455Aa,Ab; 01418+4237AB; 02278+0426AB (SB2); 09006+4147AB (SB2); 16413+3136AB; 17121+4540AB; 18070+3034AB].