Skip to content
DraconiticResearch
Search Sources API
203,203 studies31 sourcesUpdated 55 min ago
PreprintCC BY 4.0arXiv

Fast Graph-based Higher-Order Clustering Statistics on the GPU

Abstract

We present a significant update to GRAMSCI (GRAph Made Statistics for Cosmological Information; Sabiu et al. 2019), an algorithm for the fast computation of the general N-point spatial correlation function of any discrete point set. Version 2 adds several features. We replace the binary-search inner loop (O(mlog m) per hub-spoke pair, m being the mean neighbor count) with a merge-walk algorithm that reduces the inner loop to O(m). We implement a parity-decomposed 4pCF that separates the signal into even and odd channels. We estimate the disconnected 4pCF internally on the same graph to return the connected 4pCF. We add a Python/NumPy interface to the Fortran engine. Principally, we present a GPU port of the full query engine (OpenACC): the 3pCF, 4pCF, and parity-decomposed 4pCF kernels run on a single consumer GPU with measured speedups of 2.6× (3pCF) to 9× (4pCF) over a 64-thread CPU node, and out-of-core tiling handles graphs exceeding device memory. We measure a 9×109-edge BAO-scale 3pCF on a 24 GB card with ∼ 20% overhead. We validate the code against its CPU reference, against analytic injection tests, and on exactly solvable random fields (a non-Gaussian multiplicative cascade and a Gaussian field, whose full and connected 4pCF the estimators reproduce without bias), and demonstrate BAO-scale applications on the DESI DR1 LRG sample (the 3pCF and the full and connected 4pCF over the complete configuration space, both to 150 h−1 Mpc).

Related

  1. Mitigating baryonic effects in weak lensing with higher-order statistics
    Andreas Tersenov, Sacha Guerrini, Jean-Luc Starck +1
    HALPreprintarXiv licenceFull textCosmologyGeneral physicsHALarXiv
  2. Higher-order statistics of the stochastic gravitational wave background from supermassive black hole binaries
    Hinano Hisamatsu, Koutarou Kyutoku
    arXivPreprintarXiv licenceFull textGalaxiesHigh-energy astrophysicsarXiv
  3. Constraining Dynamical Dark Energy with Tomographic Galaxy and CMB Weak Lensing Through Higher-Order Statistics
    Shu-Fan Chen, J. Colin Hill, Zoltán Haiman
    arXivPreprintCC BY 4.0Full textCosmologyarXiv
  4. Climbing the N-point Ladder Part I: Information in the Higher-Order Configuration-Space Clustering of Dark Matter Halos
    Sumi Kim, Cristiano G. Sabiu, Inkyu Park
    arXivPreprintCC BY 4.0Full textCosmologyarXiv
  5. Fast and accurate false-alarm probabilities for linear detection statistics in Poisson noise
    Maayane T. Soumagnac, Eran O. Ofek, Shachar Israeli +1
    arXivPreprintarXiv licenceFull textInstrumentation & methodsarXiv
BibTeX
@misc{sabiu2026fast,
  title = {{Fast Graph-based Higher-Order Clustering Statistics on the GPU}},
  author = {Cristiano G. Sabiu},
  howpublished = {arXiv},
  year = {2026},
  month = nov,
  doi = {10.48550/arxiv.2607.06604},
  eprint = {2607.06604},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2607.06604},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - Fast Graph-based Higher-Order Clustering Statistics on the GPU
AU  - Cristiano G. Sabiu
PY  - 2026
DA  - 2026/11/04
PB  - arXiv
DO  - 10.48550/arxiv.2607.06604
UR  - https://arxiv.org/abs/2607.06604
AB  - We present a significant update to GRAMSCI (GRAph Made Statistics for Cosmological Information; Sabiu et al. 2019), an algorithm for the fast computation of the general N-point spatial correlation function of any discrete point set. Version 2 adds several features. We replace the binary-search inner loop (O(mlog m) per hub-spoke pair, m being the mean neighbor count) with a merge-walk algorithm that reduces the inner loop to O(m). We implement a parity-decomposed 4pCF that separates the signal into even and odd channels. We estimate the disconnected 4pCF internally on the same graph to return the connected 4pCF. We add a Python/NumPy interface to the Fortran engine. Principally, we present a GPU port of the full query engine (OpenACC): the 3pCF, 4pCF, and parity-decomposed 4pCF kernels run on a single consumer GPU with measured speedups of 2.6× (3pCF) to 9× (4pCF) over a 64-thread CPU node, and out-of-core tiling handles graphs exceeding device memory. We measure a 9×10^9-edge BAO-scale 3pCF on a 24 GB card with ∼ 20% overhead. We validate the code against its CPU reference, against analytic injection tests, and on exactly solvable random fields (a non-Gaussian multiplicative cascade and a Gaussian field, whose full and connected 4pCF the estimators reproduce without bias), and demonstrate BAO-scale applications on the DESI DR1 LRG sample (the 3pCF and the full and connected 4pCF over the complete configuration space, both to 150 h^−1 Mpc).
ER  -