Bayesian parameter estimation in the second LISA Pathfinder mock data challenge

M. Nofrarias, C. Röver, M. Hewitson, A. Monsky, G. Heinzel, K. Danzmann, L. Ferraioli, M. Hueller, and S. Vitale
Phys. Rev. D 82, 122002 – Published 16 December 2010

Abstract

A main scientific output of the LISA Pathfinder mission is to provide a noise model that can be extended to the future gravitational wave observatory, LISA. The success of the mission depends thus upon a deep understanding of the instrument, especially the ability to correctly determine the parameters of the underlying noise model. In this work we estimate the parameters of a simplified model of the LISA Technology Package instrument. We describe the LISA Technology Package by means of a closed-loop model that is used to generate the data, both injected signals and noise. Then, parameters are estimated using a Bayesian framework, and it is shown that this method reaches the optimal attainable error, the Cramér-Rao bound. We also address an important issue for the mission: how to efficiently combine the results of different experiments to obtain a unique set of parameters describing the instrument.

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  • Received 1 September 2010

DOI:https://doi.org/10.1103/PhysRevD.82.122002

© 2010 The American Physical Society

Authors & Affiliations

M. Nofrarias*, C. Röver, M. Hewitson, A. Monsky, G. Heinzel, and K. Danzmann

  • Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut) and Leibniz Universität Hannover, 30167 Hannover, Germany

L. Ferraioli, M. Hueller, and S. Vitale

  • Dipartimento di Fisica, Università di Trento, and I.N.F.N., Gruppo di Trento, 38050 Povo, Italy

  • *miquel.nofrarias@aei.mpg.de

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Vol. 82, Iss. 12 — 15 December 2010

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