CaltechAUTHORS
  A Caltech Library Service

Massively parallel Bayesian inference for transient gravitational-wave astronomy

Smith, Rory J. E. and Ashton, Gregory and Vajpeyi, Avi and Talbot, Colm (2020) Massively parallel Bayesian inference for transient gravitational-wave astronomy. Monthly Notices of the Royal Astronomical Society, 498 (3). pp. 4492-4502. ISSN 0035-8711. https://resolver.caltech.edu/CaltechAUTHORS:20201204-161632172

[img]
Preview
PDF - Published Version
See Usage Policy.

627kB
[img] PDF - Submitted Version
See Usage Policy.

1MB

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20201204-161632172

Abstract

Understanding the properties of transient gravitational waves (GWs) and their sources is of broad interest in physics and astronomy. Bayesian inference is the standard framework for astrophysical measurement in transient GW astronomy. Usually, stochastic sampling algorithms are used to estimate posterior probability distributions over the parameter spaces of models describing experimental data. The most physically accurate models typically come with a large computational overhead which can render data analsis extremely time consuming, or possibly even prohibitive. In some cases highly specialized optimizations can mitigate these issues, though they can be difficult to implement, as well as to generalize to arbitrary models of the data. Here, we investigate an accurate, flexible, and scalable method for astrophysical inference: parallelized nested sampling. The reduction in the wall-time of inference scales almost linearly with the number of parallel processes running on a high-performance computing cluster. By utilizing a pool of several hundreds or thousands of CPUs in a high-performance cluster, the large wall times of many astrophysical inferences can be alleviated while simultaneously ensuring that any GW signal model can be used ‘out of the box’, i.e. without additional optimization or approximation. Our method will be useful to both the LIGO-Virgo-KAGRA collaborations and the wider scientific community performing astrophysical analyses on GWs. An implementation is available in the open source gravitational-wave inference library pBilby (parallel bilby).


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1093/mnras/staa2483DOIArticle
https://arxiv.org/abs/1909.11873arXivDiscussion Paper
https://git.ligo.org/lscsoft/parallel_bilbyRelated ItempBilby Software Library
ORCID:
AuthorORCID
Smith, Rory J. E.0000-0001-8516-3324
Talbot, Colm0000-0003-2053-5582
Alternate Title:Expediting Astrophysical Discovery with Gravitational-Wave Transients Through Massively Parallel Nested Sampling
Additional Information:© 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. This article is published and distributed under the terms of the Oxford University Press, Standard Journals Publication Model (https://academic.oup.com/journals/pages/open_access/funder_policies/chorus/standard_publication_model). Accepted 2020 August 13. Received 2020 August 4; in original form 2020 April 26. This work is supported through Australian Research Council (ARC) Centre of Excellence CE170100004. The analyses presented in this paper were performed using the supercomputer cluster at the Swinburne University of Technology (SSTAR). This document has LIGO Document number P1900255-v1. We would like to thank Mathew Pitkin, Roberto Cotesta, Simon Stevenson, Serguei Ossokine, and Scott Coughlin for extensive testing of pBilby, and Eve Chase for providing information about the GWTC-1 analyses performed using SEOBNRv3. Additional thanks to Colin Capano for reviewing this manuscript. Thanks also to the SSTAR system admins for their support with all things MPI and for their patience. We are grateful for insightful comments from Vivien Raymond, Eve Chase, Richard O’Shaughnessy, Moritz Hubner, Michele Vallisneri, Alessandra Buonanno, Vicky Kalogera, and the LIGO-Virgo Parameter Estimation and Coalescing Compact Binary working groups. Additional thanks to Joshua Speagle for pointing out the scaling relation for parallel nested sampling. This research has made use of data, software and/or web tools obtained from the Gravitational Wave Open Science Center (https://www.gw-openscience.org), a service of LIGO Laboratory, the LIGO Scientific Collaboration and the Virgo Collaboration. LIGO is funded by the U.S. National Science Foundation. Virgo is funded by the French Centre National de Recherche Scientifique (CNRS), the Italian Istituto Nazionale della Fisica Nucleare (INFN) and the Dutch Nikhef, with contributions by Polish and Hungarian institutes. DATA AVAILABILITY. The pBilby software library is available at https://git.ligo.org/lscsoft/parallel_bilby/.
Group:LIGO
Funders:
Funding AgencyGrant Number
Australian Research CouncilCE170100004
NSFUNSPECIFIED
Centre National de la Recherche Scientifique (CNRS)UNSPECIFIED
Istituto Nazionale di Fisica Nucleare (INFN)UNSPECIFIED
NikhefUNSPECIFIED
Subject Keywords:gravitational waves, methods: data analysis
Other Numbering System:
Other Numbering System NameOther Numbering System ID
LIGO DocumentP1900255-v1
Issue or Number:3
Record Number:CaltechAUTHORS:20201204-161632172
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20201204-161632172
Official Citation:Rory J E Smith, Gregory Ashton, Avi Vajpeyi, Colm Talbot, Massively parallel Bayesian inference for transient gravitational-wave astronomy, Monthly Notices of the Royal Astronomical Society, Volume 498, Issue 3, November 2020, Pages 4492–4502, https://doi.org/10.1093/mnras/staa2483
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:106926
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:05 Dec 2020 02:13
Last Modified:20 May 2021 19:01

Repository Staff Only: item control page