Creating the Astrophysicists of Tomorrow

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Creating the astrophysicists of tomorrow EU project designs university course in astrophysics and astronomy for high-achieving students The Erasmus Mundus European Master ‘Astromundus’ is a course on astrophysics and astronomy for master’s degree students, helping them ahead in their career. The two-year course was designed by professors from the universities of Innsbruck (Austria), Padua and Rome (Italy), Gottingen (Germany), Belgrade (Serbia), and EU-funded scholarships Photo: © University of Innsbruck have boosted numbers taking part. Students on the programme start their study in Innsbruck focusing on astronomy and basics and then they can choose which partner university they wish Key facts and figures to attend. Erasmus+ Participants: Countries: The main topics covered by the course are galactic astrophysics Field: Higher Education 116 4 (including the sun, solar system and the Milky Way); solar astro- Action: Erasmus Mundus physics and space weather; extra solar planets; extragalactic Joint Master Degrees EU grant: Project duration: astrophysics (including the evolution of the galaxy and star € 3,007,400 2010-2016 formation), cosmology, astroparticle physics, gravitational waves, observational astrophysics from the ground and space, Project title and computational astrophysics. Erasmus Mundus Joint Master’s Degree programme in Astronomy At the end of each two-year cycle the best master’s thesis and Astrophysics (Astromundus) is awarded a prize. Students come from all over the world, but they must have a degree in physics, astronomy, astrophysics or mathematics to be accepted for the course. Student Yana Khusanova said: I cannot describe in words how Astromundus changed my life and how many things " I learned! I hope that all talented students will be able to pursue their dreams like I did!” Following the course, the majority of graduates take their study to PhD level at universities or research insti- tutes all over the world including South Africa, Serbia, Turkey and the USA. Lead organisation Name: University of Innsbruck Location: Innsbruck, Austria Website: www.uibk.ac.at More information Project website: Partners Georg-August-Universität, Göttingen, Germany; Università degli Studi di Padova, Italy; www.astromundus.eu University of Rome, Italy; University of Belgrade, Serbia The Erasmus+ Project Results Platform: http://ec.europa.eu/programmes/erasmus-plus/ projects Erasmus+.

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The Intrinsic Baldwin Effect in Broad Balmer Lines of Six Long-Term
Astronomy & Astrophysics manuscript no. 30085_paper c ESO 2018 July 2, 2018 The intrinsic Baldwin effect in broad Balmer lines of six long-term monitored AGNs N. Rakic´1, 2, G. La Mura3, D. Ilic´2, 4, A.I. Shapovalova5, W. Kollatschny6, P. Rafanelli3, L. C.ˇ Popovic´1, 2, 7 1 Faculty of Science, University of Banjaluka, Mladena Stojanovica´ 2,78000 Banjaluka, Republic of Srpska, Bosnia and Herzegovina; e-mail: [email protected] 2 Department of Astronomy, Faculty of Mathematics, University of Belgrade, Studentski Trg 16, 11000 Belgrade, Serbia 3 Department of Physics and Astronomy, University of Padova, vicolo dell’Osservatorio 3, I-35122 Padova, Italy 4 Isaac Newton Institute of Chile, Yugoslavia Branch 5 Special Astrophysical Observatory of the Russian Academy of Science, Nizhnij Arkhyz, Karachaevo-Cherkesia 369167, Russia 6 Institut fur Astrophysik, Universitat Gottingen, Friedrich-Hund Platz 1, 37077, Göttingen, Germany 7 Astronomical Observatory, Volgina 7, 11060 Belgrade, Serbia ABSTRACT We investigate the intrinsic Baldwin effect (Beff) of the broad Hα and Hβ emission lines for six Type 1 active galactic nuclei (AGNs) with different broad line characteristics: two Seyfert 1 (NGC 4151 and NGC 5548), two AGNs with double-peaked broad line profiles (3C 390.3 and Arp 102B), one narrow line Seyfert 1 (Ark 564), and one high-luminosity quasar with highly red asymmetric broad line profiles (E1821+643). We find that a significant intrinsic Beff was present in all Type 1 AGNs in our sample. Moreover, we do not see strong differences in intrinsic Beff slopes in different types of AGNs, which probably have different physical properties such as inclination, broad line region (BLR) geometry, or accretion rate.
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Nhut Truong Eötvös Loránd University Email: [email protected] Positions held and education: - 09/2017- present: postdoctoral researcher at “Lendület Hot Universe” research group, Eötvös Loránd University (Budapest, Hungary) - 04-07/2017: short-visiting researcher at Theoretical Physics group, Institute For Disciplinary Research in Science and Education (IFIRSE, Vietnam) - 12/2016: Ph.D. in Astrophysics, University of Rome “Tor Vergata”, Italy. - 09/2013: Master Degree in Science within the Astromundus Master Program, Cum Laude, University of Padova, Italy. - 09/2010: Bachelor of Science in theoretical physics, very good, University of Science, Ho Chi Minh City, Vietnam. Research Interests - Cosmological simulations of large-scale structures. - Neutrinos in cosmology. - Future missions in X-ray observations. Awards and Fellowships - 2013: Fellowship in the Joint Ph.D. Programme in Astronomy, Astrophysics, and Space Science, organized by University of Rome “La Sapienza”, University of Rome “Tor Vergata”, and INAF. - 2011: Erasmus Mundus Fellowship in the Astromundus Master Programme in Astronomy and Astrophysics. - 2011: Vietnam Education Foundation Fellowship (VEF, declined). - 2011: ICTP pre-PhD Programme Scholarship (declined). - 2010: CERN Summer School Scholarship. Recent Contributed Talks and Posters - 06/2019: MPIA Galaxy Coffee Seminar, Max Planck Institute for Astronomy (MPIA), Heidelberg, Germany. Talk: “Correlations between supermassive black holes, hot atmospheres, and the total masses of early-type galaxies.” - 03/2019: Physics of The Intra-cluster Medium Conference, Budapest, Hungary. Talk: “X-ray Scaling Relations in Early-type Galaxies from IllustrisTNG Simulations and X-ray Observations”. - 10/2018: IllustrisTNG Scientiﬁc Workshop, Max Planck Institute for Astrophysics (MPA), Germany. Talk: “Preliminary results on the X-ray Scaling Relations in Early-type Galaxies from IllustrisTNG Simulations”.
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Astromundus Brochure
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