sarabande: 3/4 point correlation functions with fast Fourier transforms

Author:

Sunseri James1ORCID,Slepian Zachary2ORCID,Portillo Stephen3ORCID,Hou Jiamin24ORCID,Kahraman Sule5ORCID,Finkbeiner Douglas P6ORCID

Affiliation:

1. Department of Astronomy, University of California , Berkeley, CA 94720-3411 , USA

2. Department of Astronomy, University of Florida , 211 Bryant Space Science Center, Gainesville, FL 32611 , USA

3. DIRAC Institute, Department of Astronomy, University of Washington , Seattle, WA 98195-1580 , USA

4. Max-Planck-Institut für Extraterrestrische Physik , Postfach 1312, Giessenbachstrasse 1, D-85748 Garching bei München , Germany

5. Massachusetts Institute of Technology, Department of Electrical Engineering and Computer Science , 77 Massachusetts Avenue, Cambridge, MA 02139 , USA

6. Center for Astrophysics, Harvard & Smithsonian , 60 Garden Street, Cambridge, MA 02138 , USA

Abstract

AbstractWe present a new python package sarabande for measuring 3- and 4-point correlation functions (3/4 PCFs) in $\mathcal {O} (N_{\mathrm{g}}\log N_{\mathrm{g}})$ time using fast Fourier transforms (FFTs), with Ng being the number of grid points used for the FFT. sarabande can measure both projected and full 3-point correlation function and 4-point correlation function on gridded two- and three-dimensional data sets. The general technique is to generate suitable angular basis functions on an underlying grid, radially bin these to create kernels, and convolve these kernels with the original gridded data to obtain expansion coefficients about every point simultaneously. These coefficients are then combined to give us the 3/4 PCF as expanded in our basis. We apply sarabande to simulations of the interstellar medium to show the results and scaling of calculating both the full and projected 3/4 PCFs.

Funder

Horizon 2020 Framework Programme

National Science Foundation

Publisher

Oxford University Press (OUP)

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