Possibilities for a Convenient Desktop Access to the GRID and to Virtual Observatories

Author(s):  
Hans Weghorn
2018 ◽  
Vol 477 (2) ◽  
pp. 1495-1507 ◽  
Author(s):  
T Dykes ◽  
A Hassan ◽  
C Gheller ◽  
D Croton ◽  
M Krokos

2010 ◽  
Vol 9 ◽  
pp. IGY85-IGY93 ◽  
Author(s):  
J. R. Thieman ◽  
D. A. Roberts ◽  
T. A. King ◽  
C. C. Harvey ◽  
C. H. Perry ◽  
...  

2012 ◽  
Vol 10 (H16) ◽  
pp. 565-565
Author(s):  
A. Mickaelian

AbstractThe Byurakan Astrophysical Observatory (BAO, Armenia, http://www.bao.am) are among the candidate IAU Regional Nodes for Astronomy for Development activities. It is one of the main astronomical centers of the former Soviet Union and the Middle East region. At present there are 48 qualified researchers at BAO, including six Doctors of Science and 30 PhDs. Five important observational instruments are installed at BAO, the larger ones being 2.6m Cassegrain (ZTA-2.6) and 1m Schmidt (the one that provided the famous Markarian survey). BAO is regarded as a national scientific-educational center, where a number of activities are being organized, such as: international conferences (4 IAU symposia and 1 IAU colloquium, JENAM-2007, etc.), small workshops and discussions, international summer schools (1987, 2006, 2008 and 2010), and Olympiads. BAO collaborates with scientists from many countries. The Armenian Astronomical Society (ArAS, http://www.aras.am/) is an NGO founded in 2001; it has 93 members and it is rather active in the organization of educational, amateur, popular, promotional and other matters. The Armenian Virtual Observatory (ArVO, http://www.aras.am/Arvo/arvo.htm) is one of the 17 national VO projects forming the International Virtual Observatories Alliance (IVOA) and is the only VO project in the region serving also for educational purposes. A number of activities are planned, such as management, coordination and evaluation of the IAU programs in the area of development and education, establishment of the new IAU endowed lectureship program and organization of seminars and public lectures, coordination and initiation of fundraising activities for astronomy development, organization of regional scientific symposia, conferences and workshops, support to Galileo Teacher Training Program (GTTP), production/publication of educational and promotional materials, etc.


2003 ◽  
Vol 208 ◽  
pp. 331-342 ◽  
Author(s):  
Piet Hut

Traditionally, a simulation of a dense stellar system required choosing an initial model, running an integrator, and analyzing the output. Almost all of the effort went into writing a clever integrator that could handle binaries, triples and encounters between various multiple systems efficiently. Recently, the scope and complexity of these simulations has increased dramatically, for three reasons: 1) the sheer size of the data sets, measured in Terabytes, make traditional ‘awking and grepping’ of a single output file impractical; 2) the addition of stellar evolution data brings qualitatively new challenges to the data reduction; 3) increased realism of the simulations invites realistic forms of ‘SOS’: Simulations of Observations of Simulations, to be compared directly with observations. We are now witnessing a shift toward the construction of archives as well as tailored forms of visualization including the use of virtual reality simulators and planetarium domes, and a coupling of both with budding efforts in constructing virtual observatories. This review describes these new trends, presenting Starlab as the first example of a full software environment for realistic large-scale simulations of dense stellar systems.


Author(s):  
Pierre Léna ◽  
Daniel Rouan ◽  
François Lebrun ◽  
François Mignard ◽  
Didier Pelat

Author(s):  
A.M.S. Richards ◽  
S.T. Garrington ◽  
P.A. Harrison ◽  
T.W.B. Muxlow ◽  
A.M. Stirling ◽  
...  

2016 ◽  
Vol 18 ◽  
pp. 40-48 ◽  
Author(s):  
Timothy Karpouzoglou ◽  
Zed Zulkafli ◽  
Sam Grainger ◽  
Art Dewulf ◽  
Wouter Buytaert ◽  
...  

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