18–22 Mar 2019
MPI for Nuclear Physics
Europe/Berlin timezone

Session

Tuesday

19 Mar 2019, 09:30
MPI for Nuclear Physics

MPI for Nuclear Physics

Saupfercheckweg 1, 69117 Heidelberg

Presentation materials

There are no materials yet.

  1. francois-xavier pineau (Université de Strasbourg)
    19/03/2019, 09:30
    Talk

    After a brief presentation of HEALPix, I will discuss the specificities of the CDS implementation.
    This implementation has been natively coded in both Java and Rust. Wrappers make the Rust library accessible in Javascript/WebAssembly and Python.
    Particular emphasis will be placed on the exact solution of cone/polygon coverage queries and on MOCs in which each cell contains a boolean flag.

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  2. Mr Matthieu Baumann (CDS (Centre de Données de Strasbourg))
    19/03/2019, 10:00
    Talk

    I will give a brief presentation about the new Rust system programming langage:
    - the compiler rules enabling memory safety
    - how one can interface Rust code with Python

    Then, regarding to what has been currently done in cdshealpix I will talk about the CI pipeline I used for generating and deploying binary wheels for different platforms.

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  3. Mr Thomas Boch (CDS - Observatoire de Strasbourg)
    19/03/2019, 10:30
    Talk

    I will present MOC (Multi Order Coverage maps), a Virtual Observatory standard allowing one to describe and compare spatial coverage of astronomical datasets.

    After presenting the MOC format (based on HEALPix tessellation), I will show some practical applications of MOC usage, using the MOCPy library developed at CDS.

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  4. Cosimo Nigro
    19/03/2019, 11:30
    Talk

    Analysis and combination of data from different gamma-ray instruments involves the use of collaboration proprietary software and case-by-case methods.
    By defining a common open format for high-level gamma-ray data (containing event lists and instrument response functions, using the FITS standard) we allow multi-instrument analysis within the context of open-source software.
    This project aims...

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  5. Dr Atreyee SINHA (APC, IN2P3/CNRS)
    19/03/2019, 12:00
    Talk

    In several branches of astrophysics, high-level data format consists of event lists - containing the reconstructed energy, direction and arrival time (and some other informations, eg: event type) of each event. For analysis and visualisation, maps are made by astronomers with a pixelisation and binning chosen to suit the use case. FITS maps, using either a WCS or a HEALPix format, are commonly...

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  6. 19/03/2019, 12:30
    Talk
    • Andrea Tramacere - ASTErIsM (poster)
    • Felix Kunzweiler - Rapid Fermi-GBM GRB localization with BALROG (poster)
    • Björn Biltzinger - Physically Motivated Background Model for GBM (poster)
    • Jeremy Perkins - BurstCube
    • Thomas Robitaille - Data visualization with glue
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  7. Dr Eric Charles (SLAC)
    19/03/2019, 14:30
    Talk

    I will summarize two software suites used for analysis of Fermi-LAT data: the fermitools (formerly ScienceTools), and the fermipy python-based software package.

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  8. Prof. Toby Burnett (University of Washington)
    19/03/2019, 15:00
    Talk

    The Fermi-LAT instrument differs in a fundamental way from its predecessors, particularly EGRET, in having a much larger field of view and energy range. With also having a much larger effective area, the data volume is also substantially larger. The design of pointlike took these factors into account in contrast to the more standard software tools based on the EGRET experience. I will explain...

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  9. Dr Daniel Kocevski (NASA MSFC)
    19/03/2019, 15:30
    Talk

    The Fermi Gamma-ray Burst Monitor (GBM), with its broad energy range and instantaneous coverage of 2/3 of the sky, observes a wide variety of flaring or transient phenomena. These capabilities make it ideally suited for the search of transient events and to contribute to the new era of multi-messenger astrophysics. The GBM team has recently released the GSPEC analysis package, a modern...

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