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--- download_install [2013/09/05 04:28]
mjc
+++ download_install [2015/04/28 05:43] (current)
mjc
@@ Line 1: / Line 1: @@
 ==== Download ====
-The latest version of **pywifes** is v0.5.0, which can be downloaded here:
+From version 0.7.0 of PyWiFeS, we have migrated the code to a github repository:
+[[https://github.com/pywifes]]
-  * [[http://www.mso.anu.edu.au/~mjc/wifes_redux/wifes_pypeline_v0.5.0.tar.gz|wifes_pypeline_v0.5.0.tar.gz]]
+To download the code, you need to first [[http://git-scm.com/downloads | install git]].  To install the PyWiFeS pipeline itself, create the directory you want to store it in then clone the PyWiFeS git repository with this command:
+<code>
+  git clone https://github.com/PyWiFeS/pipeline.git
+</code>
-Previous versions are also being stored [[http://www.mso.anu.edu.au/~mjc/wifes_redux/old_versions/|here]].  See Version Notes below for details.
+==== "Installation" ====
+To be able to run the pipeline, you need to do the following:
-==== Installation Instructions ====
+  - Add the 'src/' subdirectory to your PYTHONPATH
-Use of the pipeline does not require any installation script to be run. Instead just unpack the tar file into some directory and it will create the following upacked subdirectories:
+  - Tell the code where the reference data is stored by defining the environment variable 'PYWIFES_DIR' to point to the location of the 'reference_data/' directory.  Alternatively if you cannot define environment variables (Windows??) then you can update the reference directory location in the file 'src/wifes_metadata.py'.
-  * **src/** - Data reduction Python modules.
-  * **doc/** - Documentation on how to "install" the package (including README file) and how to use the metadata preparation script and data reduction script.
-  * **reference_data/** - Contains the metadata file with baseline wavelength solutions, and is where you should store standard star spectra.  We include the SSO extinction curve and standard star spectra from [[http://www.mso.anu.edu.au/~bessell/FTP/Spectrophotometry/| Mike Bessell's ftp site]] for which you should cite [[http://adsabs.harvard.edu/abs/1999PASP..111.1426B| Bessell et al. (1999)]], and the [[http://www.eso.org/sci/observing/tools/standards/spectra/stanlis.html| ESO spectrophotometric standards]] spectra for which you should site [[http://adsabs.harvard.edu/abs/1990AJ.....99.1621O| Oke et al. (1990)]].
-  * **reduction_scripts/** - Some high-level scripts which go through a full reduction procedure similar to what I myself use, you should feel free to write you own scripts which use the 'pywifes' package to perform your preferred reduction routine.
-  * **extractor_gui/** - A PyGTK-based GUI used for extracting spectra from hand-selected spaxels, mostly intended for me to be able to extract supernova spectra.
-=== "Installation" ===
-To be able to run the pipeline, you need to do the following:
-  - Add the 'src/' subdirectory to your PYTHONPATH
-  - Tell the code where the reference data is stored by defining the environment variable 'PYWIFES_DIR' to point to the location of the 'reference_data/' directory.  Alternatively if you cannot define environment variables (Windows??) then you can update the reference directory location in the file 'src/wifes_metadata.py'.
-=== Software Requirements ===
-The only software dependencies are standard Python modules:
-  - [[http://numpy.scipy.org/|NumPy]]
-  - [[http://www.scipy.org/|SciPy]] (note: versions before 0.9 will not work with the interpolation routine used here)
-  - [[http://www.stsci.edu/institute/software_hardware/pyfits|PyFITS]]
-It is //strongly// recommended to also install [[http://matplotlib.org/|matplotlib/pylab]] in order to view diagnostic plots.
-To be able to run the GUI, you will need to have [[http://pygtk.org/|PyGTK]] installed.
-==== Version Notes ====
-See the [[http://www.mso.anu.edu.au/~mjc/wifes_redux/PYWIFES_README|PYWIFES_README]] file for details.

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