Library for pseudo-Cl computation
Project description
NaMaster
NaMaster is a C library, Python module and standalone program to compute full-sky angular cross-power spectra of masked, spin-0 and spin-2 fields with an arbitrary number of known contaminants using a pseudo-Cl (aka MASTER) approach. The code also implements E/B-mode purification and is available in both full-sky and flat-sky modes.
Installation
Unless you care a lot about optimizing the code, you should probably use the conda recipe for NaMaster currently hosted on conda-forge (infinite kudos to Mat Becker for this). This means simply running:
conda install -c conda-forge namaster
If that works for you and you don't care about optimizing the code too much, skip the rest of this section. If you don't have admin permissions, you can give virtual environments a try (or else follow the instructions below).
0- Dependencies
NaMaster has the following dependencies, which should be present in your system before you can install the code:
- GSL. Version 2 required.
- FFTW. Version 3 required. Install with
--enable-openmp
and potentially also--enable-shared
. - libsharp. Libsharp is automatically installed with NaMaster (see section 3 below). However, if you want to use your own preinstalled version, you should simlink it into the directory
_deps
, such that_deps/lib/libsharp.a
can be seen (see instructions in NERSC_installation.md for more details on libsharp). - cfitsio. Any version >3 should work.
- HEALPix. Any version >2 should work. You only need to install the C libraries (including the shared ones).
1- Python
Installing the python module pymaster
should be as simple as running
python setup.py install [--user]
or, even better, if you can use pip
:
pip install . [--user]
where the optional --user
flag can be used if you don't have admin privileges.
You can check that the python installation works by running the unit tests:
python -m unittest discover -v
Note that the test
directory, containing all unit tests, also contains all the sample python scripts described in the documentation (see below).
If you installed pymaster
via pip
, you can uninstall everything by running
pip uninstall pymaster
Note that the C library is automatically compiled when installing the python module. If you care about the C library at all, or you have trouble compiling it, see the next section.
2- C library
The script scripts/install_libnmt.sh
contains the instructions run by setup.py
to compile the C library (libnmt.a
). You may have to edit this file or make sure to include any missing compilation flags if setup.py
encounters issues compiling the library.
If you need the C library for your own code, scripts/install_libnmt.sh
installs it in _deps/lib
and _deps/include
. Note that the script process will also generate an executable namaster
, residing in _deps/bin
that can be used to compute power spectra. The use of this program is discouraged over using the python module.
You can check that the C code works by running
make check
If all the checks pass, you're good to go.
3- Libsharp
setup.py
attempts to download and install libsharp automatically. This is done by running the script scripts/install_libsharp.sh
. If you encounter any trouble during this step, inspect the contents of that file. Libsharp gets installed in _deps/lib
and _deps/include
.
Documentation
The following sources of documentation are available for users:
- Scientific documentation: description of the methods implemented in NaMaster
- C API documentation: description of the C library functionality and the NaMaster executable. Installation instructions and a description of all dependencies can also be found here.
- Python wrapper documentation: also available in readthedocs
Licensing, credits and feedback
You are welcome to re-use the code, which is open source and freely available under terms consistent with BSD 3-Clause licensing (see LICENSE).
If you use NaMaster for any scientific publication, we kindly ask you to cite this github repository and the companion paper https://arxiv.org/abs/1809.09603. Special kudos should go to the following heroes for their contributions to the code:
- Mat Becker (@beckermr)
- Giulio Fabbian (@gfabbian)
- Daniel Lenz (@DanielLenz)
- Zack Li (@xzackli)
- Thibaut Louis (@thibautlouis)
For feedback, please contact the author via github issues or emaild (david.alonso@physics.ox.ac.uk).
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