PyGDSM is a Python interface for global diffuse sky models: all-sky maps in Healpix format of diffuse Galactic radio emission.
This package includes interfaces to:
- GSM2008: A model of diffuse Galactic radio emission from 10 MHz to 100 GHz, Oliveira-Costa et. al., (2008).
- GSM2016: An improved model of diffuse galactic radio emission from 10 MHz to 5 THz, Zheng et. al., (2016).
- LFSS: The LWA1 Low Frequency Sky Survey (10-408 MHz) Dowell et. al. (2017).
- Haslam: A frequency-scaled model using a spectral index, based on the Haslam 408 MHz all-sky map.
In general, these are not wrappers of the original code (GSM2008 was written in Fortan and GSM2016 in C); instead they provides a uniform API with some additional features and advantages, such as healpy integration for imaging, and sky rotation for observed skies.
Tip
We thank datacentral.org.au for hosting the component map data.
The first thing to do will be to make sure you've got the dependencies:
Then you should be able to install with:
pip install git+https://github.com/telegraphic/pygdsm
Alternatively, clone the directory:
git clone https://github.com/telegraphic/pygdsm
An run pip install .. On first run, the sky model data will be downloaded from Zenodo / LAMBDA. These are about 500 MB total, and will be downloaded into your astropy cache (~/.astropy/). The data are hosted by datacentral.org.au/, and are also available on Zenodo.
To get a quick feel of what PyGDSM does, have a look at the
GSM2008 quickstart guide, and the new
GSM2016 quickstart guide.
Q. What's the difference between this and the gsm.f from the main GSM2008 website?
The gsm.f is a very basic Fortran code, which reads and writes values to and from
ASCII files, and uses a command line interface for input. If you want to run this code
on an ancient computer with nothing but Fortran installed, then gsm.f is the way to go.
In contrast, PyGDSM is a Python code that leverages a lot of other Packages so that you
can do more stuff more efficiently. For example: you can view a sky model in a healpy
image; you can write a sky model to a Healpix FITS file; and believe it or not, the
Python implementation is much faster. Have a look at the
quickstart guide
to get a feel for what PyGDSM does.
Q. Are the outputs of gsm.f and pygdsm identical?.
NO. The cubic spline interpolation implementation differs, so values will differ by as
much as a few percent. The interpolation code used in gsm.f does not have an open-source
license (it's from Numerical Recipes ), so we haven't
implemented it (one could probably come up with an equivalent that didn't infringe).
Nevertheless, the underlying PCA data are identical, and I've run tests to check that
the two outputs are indeed comparable.
Q. What's the difference between this and the Zheng et. al. github repo?
pygdsm provides two classes: GlobalSkyModel16() and GSMObserver16(), which once instantiated
provide methods for programatically generating sky models. The Zheng et. al. github repo is a
simple, low-dependency, command line tool. As of PyGDSM 1.4.0, we have implemented improved interpolation
via cubic spline or PCHIP, which avoids discontinuities identified using the 2016 method. Have a look at the
GSM2016 quickstart guide
to get a feel for what PyGDSM does.
Q. Why does this package download so much data when first run?
The package size is dominated by the PCA healpix maps, which have about 3 million points each.
They're compressed using HDF5 LZF, so are actually about 3x smaller than the *.dat
files that come in the original gsm.tar.gz file. The next biggest thing is test data,
so that the output can be compared against precomputed output from gsm.f. The package now also includes
the Zheng et. al. data, which is another ~300 MB.
The sky model data contained here is from:
- GSM2008 http://space.mit.edu/~angelica/gsm/index.html (link no longer active)
- GSM2016 https://github.com/jeffzhen/gsm2016
- LFSS https://lda10g.alliance.unm.edu/LWA1LowFrequencySkySurvey/
- Haslam https://lambda.gsfc.nasa.gov/product/foreground/fg_2014_haslam_408_info.cfm
A model of diffuse Galactic radio emission from 10 MHz to 100 GHz
A. de Oliveira-Costa, M. Tegmark, B.M. Gaensler, J. Jonas, T.L. Landecker and P. Reich
MNRAS 388, 247-260 (2008)
https://ui.adsabs.harvard.edu/abs/2008MNRAS.388..247D/abstract
An Improved Model of Diffuse Galactic Radio Emission from 10 MHz to 5 THz
H. Zheng, M. Tegmark, J. Dillon, A. Liu, A. Neben, J. Jonas, P. Reich, W.Reich
MNRAS, 464, 3, 3486-3497 (2017)
https://ui.adsabs.harvard.edu/abs/2017MNRAS.464.3486Z/abstract
The LWA1 Low Frequency Sky Survey
J. Dowell, G. B. Taylor, F. Schinzel, N. E. Kassim, K. Stovall
MNRAS, 469, 4, 4537-4550 (2017)
https://ui.adsabs.harvard.edu/abs/2017MNRAS.469.4537D/abstract
An improved source-subtracted and destriped 408-MHz all-sky map
M. Remazeilles, C. Dickinson,A.J. Banday, M. Bigot-Sazy, T. Ghosh
MNRAS 451, 4, 4311-4327 (2014)
https://ui.adsabs.harvard.edu/abs/2015MNRAS.451.4311R/abstract
PyGSDM has an ascl.net entry:
D. C. Price, 2016, 2.0.0, Astrophysics Source Code Library, 1603.013
All code in PyGDSM is licensed under the MIT license (not the underlying data). The PCA data, by Zheng et. al. is licensed under MIT also (see https://github.com/jeffzhen/gsm2016).