English

SARABANDE: 3/4 Point Correlation Functions with Fast Fourier Transforms

Instrumentation and Methods for Astrophysics 2022-10-26 v2 Cosmology and Nongalactic Astrophysics

Abstract

We present a new python\texttt{python} package SARABANDE for measuring 3 & 4 Point Correlation Functions (3/4 PCFs) in O(NglogNg)\mathcal{O}(N_{\rm g} \log N_{\rm g}) time using Fast Fourier Transforms (FFTs), with NgN_{\rm g} the number of grid points used for the FFT. SARABANDE can measure both projected and full 3 and 4 PCFs on gridded 2D and 3D datasets. 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 (ISM) to show the results and scaling of calculating both the full and projected 3/4 PCFs.

Keywords

Cite

@article{arxiv.2210.10206,
  title  = {SARABANDE: 3/4 Point Correlation Functions with Fast Fourier Transforms},
  author = {James Sunseri and Zachary Slepian and Stephen Portillo and Jiamin Hou and Sule Kahraman and Douglas P. Finkbeiner},
  journal= {arXiv preprint arXiv:2210.10206},
  year   = {2022}
}

Comments

16 Pages, 8 Figures, 8 Algorithms, 1 code package

R2 v1 2026-06-28T03:57:28.023Z