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============================================== | ||
BORG SDSS data products | ||
============================================== | ||
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:Authors: Florent Leclercq, Jens Jasche, Guilhem Lavaux, Benjamin Wandelt | ||
:Last update: 16-06-2016 | ||
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---------------------- | ||
File Contents | ||
---------------------- | ||
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Including this file you should have received a copy of in total three files: | ||
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README.rst | ||
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borg_sdss_diva.npz | ||
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example.py | ||
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README.rst :This file contains the information you are currently reading. | ||
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borg_sdss_diva.npz :This file contains the maps obtained by Leclercq et al. (2016a), who performed | ||
a Bayesian analysis of the cosmic web in the SDSS volume. The results are four | ||
probabilistic maps of the voids, sheets, filaments, and clusters. | ||
Structures are defined using the DIVA algorithm (Lavaux & Wandelt 2010) | ||
Data is provided in terms of a standard 3D numpy array and can easily be accessed and | ||
processed with the open source Python programming language. For further details on | ||
the data and employed methods please consult the manuscript Leclercq et al. (2016a), | ||
of which the reference is provided below. | ||
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example.py :This file is an example script to be executed with the Python programming language. | ||
The script exemplifies loading and plotting the data contained in borg_sdss_diva.npz. | ||
This script can be used to reproduce figure 3 (top row) in Leclercq et al. (2016a). | ||
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---------------------- | ||
Usage | ||
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The file borg_sdss_diva.npz contains the probabilistic structure types maps in a standard uncompressed .npz format. | ||
To load and process the data with the Python programming language execute the following commands: | ||
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import numpy as np | ||
diva=np.load('borg_sdss_diva.npz') | ||
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To access the 3D structure maps use: | ||
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voids=diva['voids'] | ||
sheets=diva['sheets'] | ||
filaments=diva['filaments'] | ||
clusters=diva['clusters'] | ||
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Individual voxels in this 3D volumetric data cube can be accessed as follows: | ||
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voids_ijk=voids[k,j,i], | ||
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where i,j and k index voxel positions along the x,y and z axes respectively. | ||
All indices run from 0 to 255. | ||
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The ranges describing the extent of the cubic cartesian volume along | ||
the x,y and z axes can be accessed as follows: | ||
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xmin=diva['ranges'][0] | ||
xmax=diva['ranges'][1] | ||
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ymin=diva['ranges'][2] | ||
ymax=diva['ranges'][3] | ||
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zmin=diva['ranges'][4] | ||
zmax=diva['ranges'][5] | ||
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Units are Mpc/h. | ||
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(Note that all the maps that are part of the BORG SDSS data products have consistent consistent | ||
coordinate systems. The coordinate transform to change from Cartesian to spherical coordinates | ||
and vice versa is given in appendix B of Jasche et al. 2015) | ||
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A showcase of loading and plotting this data is provided by the file example.py, | ||
a copy of which you should have received along with this file. | ||
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---------------------- | ||
Credits | ||
---------------------- | ||
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If you are using this data in your publications please cite the | ||
following publication: | ||
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Leclercq, F. and Jasche, J. and Lavaux, G. and Wandelt, B. (2016a) | ||
Inference and classifications of the Lagrangian dark matter sheet in the SDSS | ||
arXiv:1601.00093 [astro-ph.CO] | ||
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As cosmic web analysis is a derived product of the BORG SDSS analysis, we also kindly | ||
ask you to cite the following publications: | ||
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Jasche, J. and Wandelt, B. D. (2013) | ||
Bayesian physical reconstruction of initial conditions from large-scale structure surveys | ||
Monthly Notices of the Royal Astronomical Society 432, 894-913 (2013) | ||
arXiv:1203.3639 [astro-ph.CO] | ||
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and: | ||
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Jasche, J. and Leclercq, F. and Wandelt, B. D. (2015) | ||
Past and present cosmic structure in the SDSS DR7 main sample | ||
Journal of Cosmology and Astroparticle Physics 01, 036 (2015) | ||
arXiv:1409.6308 [astro-ph.CO] | ||
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as well as the 'DIVA' paper: | ||
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Lavaux, G. and Wandelt, B. D. (2010) | ||
Precision cosmology with voids: definition, methods, dynamics | ||
Monthly Notices of the Royal Astronomical Society 403, 1392-1408 (2010) | ||
arXiv:0906.4101 [astro-ph.CO] | ||
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We suggest, for example, the following sentence: | ||
'This work uses the cosmic web maps obtained by Leclercq et al. (2016a), based on the DIVA definition (Lavaux & Wandelt 2010) | ||
and on the analysis of the SDSS (Jasche et al. 2015) by the BORG algorithm (Jasche & Wandelt 2013).' |
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