R Jampani, F Xu, M Wu, L Perez… - ACM Transactions on …, 2011 - dl.acm.org In this article we describe MCDB, a database system that permits a wide spectrum of stochastic models to be used in conjunction with the data stored in a large database, without ever extracting the data. MCDB facilitates in-database execution of tasks such as risk assessment, ...
[PDF] from arxiv.orgS Vennes, JR Thorstensen, A Kawka… - The Astrophysical …, 2011 - iopscience.iop.org S. VENNES1,4, JR THORSTENSEN2, A. KAWkA1, P. NÉMETH1,4, JN SkINNER2, A. PIGULSkI3, M. STESLICkI3, Z. KOłLACzkOWSkI3, AND P. SRÓDkA3 1 Astronomický ústav, Akademie ved Ceské republiky, Fricova 298, CZ-251 65 Ondrejov, Czech Republic 2 Department of ...
PE Christopoulou, A Parageorgiou… - The Astronomical …, 2011 - iopscience.iop.org New CCD photometric BVRI observations of the puzzling W UMa type binary star, TZ Bootis, are presented from our observations in 2010. By using the updated version of the Wilson–Devinney code, the first modern photometric solution is deduced from new photometric ...
[PDF] from arxiv.org…, I Marti-Vidal, JBL Bouquin, LM Close… - Arxiv preprint arXiv: …, 2011 - arxiv.org ... ABDoradus is a quadruple stellar system, consisting of two close pairs, AB Dor A / AB Dor C and AB Dor Ba / AB Dor Bb, separated by about 9”. The brightest star of the system, ABDorA, is a well-known, pre-main sequence K1-star, with strong emission at all wavelengths, from ...
MA Pogodin, NG Beskrovnaya, IS Guseva… - Astrophysics, 2011 - Springer Photometric and high resolution spectroscopic data for the Herbig star HD 52721 obtained from October 2009 through October 2010 are presented. We confirm the cyclical character of the photometric variability of HD 52721 discovered previously by others. The variability shows up as ... Related articles - All 2 versions
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