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# Getting Started

FabIO is a Python module for reading and handling data from two-dimensional X-ray detectors.

FabIO is a Python module written for easy and transparent reading of raw two-dimensional data from various X-ray detectors. The module provides a function for reading any image and returning a fabioimage object which contains both metadata (header information) and the raw data. All fabioimage object offer additional methods to extract information about the image and to open other detector images from the same data series.

## Introduction

One obstacle when writing software to analyse data collected from a two-dimensional detector is to read the raw data into the program, not least because the data can be stored in many different formats depending on the instrument used. To overcome this problem we decided to develop a general module, FabIO (FABle I/O), to handle reading and writing of two-dimensional data. The code-base was initiated by merging parts of our fabian imageviewer and ImageD11 peak-search programs and has been developed since 2007 as part of the TotalCryst program suite for analysis of 3DXRD microscopy data. During integration into a range of scientific programs like the FABLE graphical interface, EDNA and the fast azimuthal integration library, pyFAI; FabIO has gained several features like handling multi-frame image formats as well as writing many of the file formats.

## FabIO Python module

Python is a scripting language that is very popular among scientists and which also allows well structured applications and libraries to be developed.

### Philosophy

The intention behind this development was to create a Python module which would enable easy reading of 2D data images, from any detector without having to worry about the file format. Therefore FabIO just needs a file name to open a file and it determines the file format automatically and deals with gzip and bzip2 compression transparently. Opening a file returns an object which stores the image in memory as a 2D NumPy array and the metadata, called header, in a Python dictionary. Beside the data and header attributes, some methods are provided for reading the previous or next image in a series of images as well as jumping to a specific file number. For the user, these auxiliary methods are intended to be independent of the image format (as far as is reasonably possible).

FabIO is written in an object-oriented style (with classes) but aims at being used in a scripting environment: special care has been taken to ensure the library remains easy to use. Therefore no knowledge of object-oriented programming is required to get full benefits of the library. As the development is done in a collaborative and decentralized way; a comprehensive test suite has been added to reduce the number of regressions when new features are added or old problems are repaired. The software is very modular and allows new classes to be added for handling other data formats easily. FabIO and its source-code are freely available to everyone on-line, licensed under the GNU General Public License version 3 (GPLv3). FabIO is also available directly from popular Linux distributions like Debian and Ubuntu.

### Implementation

The main language used in the development of FabIO is Python; however, some image formats are compressed and require compression algorithms for reading and writing data. When such algorithms could not be implemented efficiently using Python or NumPy native modules were developed, in i.e. standard C code callable from Python (sometimes generated using Cython). This code has to be compiled for each computer architecture and offers excellent performance. FabIO is only dependent on the NumPy module and has extra features if two other optional Python modules are available. For reading XML files (that are used in EDNA) the Lxml module is required and the Python Image Library, PIL is needed for producing a PIL image for displaying the image in graphical user interfaces and several image-processing operations that are not re-implemented in FabIO. A variety of useful image processing is also available in the scipy.ndimage module and in scikits-image.

Images can also be displayed in a convenient interactive manner using matplotlib and an IPython shell , which is mainly used for developing data analysis algorithms. Reading and writing procedure of the various TIFF formats is based on the TiffIO code from PyMCA.

In the Python shell, the fabio module must be imported prior to reading an image in one of the supported file formats (see Table Supported formats, hereafter). The fabio.open function creates an instance of the Python class fabioimage, from the name of a file. This instance, named img hereafter, stores the image data in img.data as a 2D NumPy array. Often the image file contains more information than just the intensities of the pixels, e.g. information about how the image is stored and the instrument parameters at the time of the image acquisition, these metadata are usually stored in the file header. Header information, are available in img.header as a Python dictionary where keys are strings and values are usually strings or numeric values.

Information in the header about the binary part of the image (compression, endianness, shape) are interpreted however, other metadata are exposed as they are recorded in the file. FabIO allows the user to modify and, where possible, to save this information (the table Supported formats summarizes writable formats). Automatic translation between file-formats, even if desirable, is sometimes impossible because not all format have the capability to be extended with additional metadata. Nevertheless FabIO is capable of converting one image data-format into another by taking care of the numerical specifics: for example float arrays are converted to integer arrays if the output format only accepts integers.

### FabIO methods

One strength of the implementation in an object oriented language is the possibility to combine functions (or methods) together with data appropriate for specific formats. In addition to the header information and image data, every fabioimage instance (returned by fabio.open) has methods inherited from fabioimage which provide information about the image minimum, maximum and mean values. In addition there are methods which return the file number, name etc. Some of the most important methods are specific for certain formats because the methods are related to how frames in a sequence are handled; these methods are img.next(), img.previous(), and img.getframe(n). The behaviour of such methods varies depending on the image format: for single-frame format (like mar345), img.next() will return the image in next file; for multi-frame format (like GE), img.next() will return the next frame within the same file. For formats which are possibly multi-framed like EDF, the behaviour depends on the actual number of frames per file (accessible via the img.nframes attribute).

## Usage

### Examples

In this section we have collected some basic examples of how FabIO can be employed.

Opening an image:

    import fabio
    im100 = fabio.open('Quartz_0100.tif') # Open image file
    print(im0.data[1024,1024])            # Check a pixel value
    im101 = im100.next()                  # Open next image
    im270 = im1.getframe(270)             # Jump to file number 270: Quartz_0270.tif

Normalising the intensity to a value in the header:

    img = fabio.open('exampleimage0001.edf')
    print(img.header)
    {'ByteOrder': 'LowByteFirst',
     'DATE (scan begin)': 'Mon Jun 28 21:22:16 2010',
     'ESRFCurrent': '198.099',
    ...
    }
    # Normalise to beam current and save data
    srcur = float(img.header['ESRFCurrent'])
    img.data *= 200.0/srcur
    img.write('normed_0001.edf')

Interactive viewing with matplotlib:

    from matplotlib import pyplot       # Load matplotlib
    pyplot.imshow(img.data)             # Display as an image
    pyplot.show()                       # Show GUI window

## Future and perspectives

The Hierarchical Data Format version 5 (hdf5) is a data format which is increasingly popular for storage of X-ray and neutron data. To name a few facilities the synchrotron Soleil and the neutron sources ISIS, SNS and SINQ already use HDF extensively through the NeXus format. For now, mainly processed or curated data are stored in this format but new detectors (Eiger from Dectris) are natively saving data in HDF5. FabIO will rely on H5Py, which already provides a good HDF5 binding for Python, as an external dependency, to be able to read and write such HDF5 files.

## Conclusion

FabIO gives an easy way to read and write 2D images when using the Python computer language. It was originally developed for X-ray diffraction data but now gives an easy way for scientists to access and manipulate their data from a wide range of 2D X-ray detectors. We welcome contributions to further improve the code and hope to add more file formats in the future.

### Acknoledgements

We acknowledge Andy Götz and Kenneth Evans for extensive testing when including the FabIO reader in the Fable image viewer (Götz et al., 2007).We also thank V. Armando Solé for assistance with his TiffIO reader and Carsten Gundlach for deployment of FabIO at the beamlines i711 and i811, MAX IV, and providing bug reports. We finally acknowledge our colleagues who have reported bugs and helped to improve FabIO. Financial support was granted by the EU 6th Framework NEST/ADVENTURE project TotalCryst (Poulsen et al., 2006).

### Citation

Knudsen, E. B., Sørensen, H. O., Wright, J. P., Goret, G. & Kieffer, J. (2013). J. Appl. Cryst. 46, 537-539.

http://dx.doi.org/10.1107/S0021889813000150

### List of file formats that FabIO can read and write

In alphabetical order. The listed filename extensions are typical examples. FabIO tries to deduce the actual format from the file itself and only uses extensions as a fallback if that fails.

Supported formats
Python Module | Detector / Format | Extension | Read | Multi-image | Write
--- | --- | --- | --- | --- | ---
ADSC | ADSC Quantum | .img | Yes | No | Yes
Bruker | Bruker formats | .sfrm | Yes | No | Yes
DM3 | Gatan Digital Micrograph | .dm3 | Yes | No | No
EDF | ESRF data format | .edf | Yes | Yes | Yes
EDNA-XML | Used by EDNA | .xml | Yes | No | No
CBF | CIF binary files | .cbf | Yes | No | Yes
kcd | Nonius KappaCCD | .kccd | Yes | No | No
fit2d mask | Used by Fit2D | .msk | Yes | No | Yes
fit2d spreadsheet | Used by Fit2D | .spr | Yes | No | Yes
GE | General Electric | No | Yes | Yes | No
HiPiC | Hamamatsu CCD | .tif | Yes | No | No
HDF5 | Hierachical data dormat | .h5 | Yes | No | No
marccd | MarCCD/Mar165 | .mccd | Yes | No | No
mar345 | Mar345 image plate | .mar3450 | Yes | No | Yes
OXD | Oxford Diffraction | .img | Yes | No | Yes
Pixi | pixi | . | Yes | No | No
pilatus | Dectris Pilatus Tiff | .tif | Yes | No | Yes
PNM | Portable aNy Map | .pnm | Yes | No | No
Raxis | Rigaku Saxs format | .img | Yes | No | No
TIFF | Tagged Image File Format | .tif | Yes | No | Yes

### Adding new file formats

We hope it will be relatively easy to add new file formats to fabio in the future. The basic idea is the following:
  1. inherit from fabioimage overriding the methods _readheader, read and optionally write. Name your new module XXXimage where XXX means something (eg tifimage).
  2. readheader fills in a dictionary of “name”:”value” pairs in self.header. No one expects to find anything much in there.
  3. read fills in self.data with a numpy array holding the image. Some redundant info which also appears are self.dim1 and self.dim2: the image dimensions, self.bpp is the bytes per pixel and self.bytecode is the numpy.dtype.type of the data.
  4. The member variables “_need_a_seek_to_read” and “_need_a_real_file” are there in case you have trouble with the transparent handling of bz2 and gz files.
  5. Register the file type (extension naming) in fabioutils.py:FILETYPES
  6. Add your new module as an import into fabio.openimage
  7. Fill out the magic numbers for your format in fabio.openimage if you know them (the characteristic first few bytes in the file)
  8. Upload a testimage to the file release system and create a unittest testcase which opens an example of your new format, confirming the image has actually been read in successfully (eg check the mean, max, min and esd are all correct, perhaps orientation too)
  9. Run pylint on your code and then please go clean it up. Have a go at mine while you are at it.
  10. Bask in the warm glow of appreciation when someone unexpectedly learns they don’t need to convert their data into another format

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