Sign for Notice Everyday    Sign Up| Sign In| Link| English|

Our Sponsors


    ASTRO-HPC 2012 - Workshop on High-Performance Computing for Astronomy

    View: 727

    Website www.hpdc.org/2012 | Want to Edit it Edit Freely

    Category ASTRO-HPC 2012

    Deadline: February 18, 2012 | Date: June 18, 2012-June 22, 2012

    Venue/Country: Delft, Netherlands

    Updated: 2011-12-13 17:53:34 (GMT+9)

    Call For Papers - CFP

    In the past 5 years, astronomy has become one of the biggest consumers of computing resources. Therefore, new computational solutions (both hardware and software) are emerging, dedicated to the various fields of the science. For example, in radioastronomy, instruments are becoming extremely large. Comprising of thousands of antennas, these radio telescopes generate huge amounts of data that have to be analyzed in a timely manner. As a result, large scale systems (both distributed and centralized) are employed for data gathering, filtering, analysis, and imaging. Furthermore, the Square Kilometer Array (SKA), a very large scale international project, seems to push the limits of radioastronomy data processing to new limits, as proven by pathfinders such as LOFAR, ASKAP, MeerKAT or anzSKA.

    All in all, it is expected that astronomy experiments will become larger in all dimensions: larger data collections, more accurate data analysis and processing, and more detailed results (i.e., imaging). This significant increase of the large-size experiments to be performed by the instruments built around the world require not only huge processing power, but also clever system design, all the way from the hardware construction to the software development and deployment.

    In this context, this first edition of the Astro-HPC workshop focuses on system design for large-scale astronomy systems. We aim to give specialists from both astronomy and computer science and engineering the opportunity to discuss both the requirements of large-scale high-performance computing systems suitable and/or usable for various astronomy applications, and practical examples of such designs and implementations. Therefore, we encourage both contributions that analyze the size and needs of large-scale astronomy systems to be used in the near future, as well as contributions that show how existing algorithms and methods should be adapted or replaced to the larger scale of these near future experiments.

    The First Workshop on Social Media Processing (SocMP’12) solicits papers that address the data management and processing challenges raised by running and mining large-scale social media platforms from a systems and infrastructure-oriented perspective. The workshop will be co-located with ACM/IEEE HPDC (http://www.hpdc.org/2012/) and will take place in June 2012 in Delft, The Netherlands. SocMP’12 will bring together researchers and practitioners in discussing and creating new knowledge about the social media infrastructure and methods of the future.

    Topics of interest include, but are not limited to:

    Systems

    Specific design requirements and solutions

    Benchmarking and performance evaluation

    Performance analysis and limitations of new system configurations

    Energy efficiency: predictions, measurements, analysis.

    Accelerators

    Evaluation of accelerator-based systems in the field of astronomy

    The requirements for accelerators in astronomy applications

    The impact of various accelerator on the performance and/or energy of HPC systems for astronomy

    Applications

    Novel large-scale astronomy applications

    Evaluation and benchmarking of applications in large-scale environments

    Updates, tuning, and optimizations of existing astronomy applications

    Algorithms

    Performance evaluation and analysis of traditional algorithms

    Novel algorithms for astronomy kernels


    Keywords: Accepted papers list. Acceptance Rate. EI Compendex. Engineering Index. ISTP index. ISI index. Impact Factor.
    Disclaimer: ourGlocal is an open academical resource system, which anyone can edit or update. Usually, journal information updated by us, journal managers or others. So the information is old or wrong now. Specially, impact factor is changing every year. Even it was correct when updated, it may have been changed now. So please go to Thomson Reuters to confirm latest value about Journal impact factor.