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Data Access Library (DAL)

Contents:

  1. Introduction
  2. Getting the source code
  3. Organization of the source code
  4. External dependencies
  5. Configuration, build and installation
  6. Contributing changes
  7. Further reading

1. Introduction

The size and complexity of astronomical data are growing at relentless rates. This increase is especially apparent in the radio community as evidenced by the data challenges faced by many of the SKA pathfinders and other major radio telescopes such as LOFAR, EVLA, ALMA, ASKAP, MeerKAT, MWA, LWA and eMERLIN. Enormous data rates are also becoming a challenge for large optical projects that are currently ramping up including Pan-Starrs and LSST. As progress towards meeting these challenges, ASTRON and the LOFAR project are currently exploring the use of the Hierarchical Data Format, version 5 (HDF5) for LOFAR radio data encapsulation.

The Data Access Library (DAL) is a library that abstracts the underlying file format from the user when working with radio astronomy data. Underlying formats may include HDF5, AIPS++/CASA tables, FITS or specific raw formats. This library is available to both the C/C++ developer and the Python user via the "pydal" module.

2. Getting the source code

As of Feb 15, 2001 the DAL can be cloned directly from the master repository hosted on Github (http://github.com):

git clone https://github.com/nextgen-astrodata/DAL.git DAL

Once your checkout from the Git repository is complete, follow the instructions as described in the section "Configuration and build" below.

3. Organization of the source code

The components of the DAL is organized into the following directory structure:

DAL
|-- build
|-- cmake
|-- data                     ..   Reference data sets used for rest programs.
|-- doc                      ..   Documentation.
|    `-- figures
`-- src
      |-- apps               ..   Application programs build on top of the library.
      |    `-- bf2h5
      |-- lib
      |    |-- core          ..   Core library classes
      |    |    `-- test
      |    |-- coordinates   ..   Representation of world coordinates
      |    |    `-- test
      |    |-- data_common   ..   Common functionality for datasets
      |    |    `-- test
      |    `-- data_hl       ..   High-level interfaces to datasets
      |          `-- test
      |-- bindings
      |   `-- python         ..   Bindings to the Python scripting language
      |       `-- test
      `-- test
            |-- hdf5
            |-- python
            `-- swig

4. External dependencies

To build the DAL from the sources you need a number of installed software packages and utilities:

Package Version Status/Description
CMake >=2.8 required
Doxygen >=1.6 optional, for documentation
HDF5 library >=1.8.3 required, for LOFAR data
WCSLIB >=4.2 optional, for casacore
CFITSIO >=3.0 optional, for FITS support
casacore optional, for MS support
Boost libraries >=1.40.0 optional
Python >= 2.6 optional, Python bindings

5. Configuration, build and installation

The DAL uses the CMake (www.cmake.org) Cross-Platform Makefile Generator for configuration and control of the build.

Once your checkout from the Git repository is complete you will have a directory structure on disk as described in section "Organization of the source code" above.

cd DAL
mkdir build
cd build
cmake ..
make

The default installation location is "/opt/dal"; if you want to change this, you can tell CMake so by using

cmake -D DAL_INSTALL_PREFIX=<installation prefix> ..

The CMake scripts will check a number of standard locations for the required 3-party packages (such as Boost, HDF5, etc.), but if you are using a custom version installed at a non-standard location, you might need to aid CMake in finding all required components:

cmake -DHDF5_ROOT_DIR=<basedir of HDF5 install> ..

In to install the DAL you will have to run

make install

from within the build directory. Depending on whether you are installing into a local directory or into a system-directory, appropriate permissions might be required.

In order to maintain compatibility with the Filesystem Hierarchy Standard (FHS) the following default installation layout has been defined:

/opt
└── dal                            CMAKE_INSTALL_PREFIX   = DAL_INSTALL_PREFIX
    ├── bin                        DAL_INSTALL_BINDIR     = DAL_INSTALL_PREFIX/bin
    ├── include                    DAL_INSTALL_INCLUDEDIR = DAL_INSTALL_PREFIX/include
    │   ├── coordinates
    │   ├── core
    │   ├── data_common
    │   └── data_hl
    ├── lib                        DAL_INSTALL_LIBDIR     = DAL_INSTALL_PREFIX/lib
    └── share
        └── doc
            └── html

However the installation configuration can be tailored depending on your personal needs:

  1. Default settings.

    If no further command line parameter are provided, the installation will be done according to the above described structure.

  2. Custom installation prefix.

    In order to install into an existing standard directory structure -- such such as e.g. "/usr/local" -- use

    -D DAL_INSTALL_PREFIX=

  3. Installation as part of the LUS.

    In order to simplify installation of the DAL as part of the LOFAR User Software distribution, a preset has been defined which can be used through

    -D LUS_INSTALL_PREFIX=

    where =$LOFARSOFT/release

For further details and additional configuration options, consult the Doxygen-based documentation.

6. Contributing changes

Direct write access to the project's code respository is limited to a small core team, responsible for the guiding the development of the DAL. If you are in more than simply using the DAL, but actively contributing to it development, the advised work-flow is as follows:

  1. Create your own fork from the master repository of the project.

    CAUTION: If you are planning to to actually development work, make sure you fork from the 'master' branch, not from 'release'. Following common Git policy create a new branch on which to carry out the development - this will make separation from other development activities easier and will enable more granularity in the selection of new features into the main development branch or the preparation of a new release version.

  2. Work on push changes you are working on - be it bug fixes or feature enhancements - back to your fork.

  3. When ready to have your changes integrated into the project's development master branch, issue a pull request. This will give the core team a chance to have a look at your contribution, before merging it into the master branch. If everything is just fine, the pull request will be requested right away, otherwise a short conversation might be necessary of how to go about the integration of your code contribution.

Suggested reading:

7. Further reading

Further detailed information regarding

  • configuration options
  • installation options
  • organization of the code base
  • library modules

can be found in the HTML documentation generated using Doxygen:

cd build
cmake ..
make Documentation

If you are having trouble with unresolved package dependencies, you can configure for generation of documentation only:

cmake -DDOCUMENTATION_ONLY=YES ..
make

Point your web-browser to

build/doc/html/index.html

About

The Data Access Library (DAL) is a library that abstracts the underlying file format from the user when working with radio astronomy data.

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