Reconstructing the sky location of gravitational-wave detected compact binary systems: Methodology for testing and comparison

T. Sidery, B. Aylott, N. Christensen, B. Farr, W. Farr, F. Feroz, J. Gair, K. Grover, P. Graff, C. Hanna, V. Kalogera, I. Mandel, R. O'Shaughnessy, M. Pitkin, L. Price, V. Raymond, C. Röver, L. Singer, M. Van Der Sluys, R. J.E. SmithA. Vecchio, J. Veitch, S. Vitale

Research output: Contribution to journalArticle

33 Citations (Scopus)

Abstract

The problem of reconstructing the sky position of compact binary coalescences detected via gravitational waves is a central one for future observations with the ground-based network of gravitational-wave laser interferometers, such as Advanced LIGO and Advanced Virgo. Different techniques for sky localization have been independently developed. They can be divided in two broad categories: fully coherent Bayesian techniques, which are high latency and aimed at in-depth studies of all the parameters of a source, including sky position, and "triangulation-based" techniques, which exploit the data products from the search stage of the analysis to provide an almost real-time approximation of the posterior probability density function of the sky location of a detection candidate. These techniques have previously been applied to data collected during the last science runs of gravitational-wave detectors operating in the so-called initial configuration. Here, we develop and analyze methods for assessing the self consistency of parameter estimation methods and carrying out fair comparisons between different algorithms, addressing issues of efficiency and optimality. These methods are general, and can be applied to parameter estimation problems other than sky localization. We apply these methods to two existing sky localization techniques representing the two above-mentioned categories, using a set of simulated inspiral-only signals from compact binary systems with a total mass of ≤20M and nonspinning components. We compare the relative advantages and costs of the two techniques and show that sky location uncertainties are on average a factor ≈20 smaller for fully coherent techniques than for the specific variant of the triangulation-based technique used during the last science runs, at the expense of a factor ≈1000 longer processing time.

Original languageEnglish (US)
Article number084060
JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
Volume89
Issue number8
DOIs
StatePublished - Apr 18 2014

Fingerprint

gravitational waves
sky
methodology
triangulation
data products
LIGO (observatory)
probability density functions
coalescing
interferometers
costs
detectors
configurations
approximation
lasers

All Science Journal Classification (ASJC) codes

  • Nuclear and High Energy Physics
  • Physics and Astronomy (miscellaneous)

Cite this

Sidery, T. ; Aylott, B. ; Christensen, N. ; Farr, B. ; Farr, W. ; Feroz, F. ; Gair, J. ; Grover, K. ; Graff, P. ; Hanna, C. ; Kalogera, V. ; Mandel, I. ; O'Shaughnessy, R. ; Pitkin, M. ; Price, L. ; Raymond, V. ; Röver, C. ; Singer, L. ; Van Der Sluys, M. ; Smith, R. J.E. ; Vecchio, A. ; Veitch, J. ; Vitale, S. / Reconstructing the sky location of gravitational-wave detected compact binary systems : Methodology for testing and comparison. In: Physical Review D - Particles, Fields, Gravitation and Cosmology. 2014 ; Vol. 89, No. 8.
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Sidery, T, Aylott, B, Christensen, N, Farr, B, Farr, W, Feroz, F, Gair, J, Grover, K, Graff, P, Hanna, C, Kalogera, V, Mandel, I, O'Shaughnessy, R, Pitkin, M, Price, L, Raymond, V, Röver, C, Singer, L, Van Der Sluys, M, Smith, RJE, Vecchio, A, Veitch, J & Vitale, S 2014, 'Reconstructing the sky location of gravitational-wave detected compact binary systems: Methodology for testing and comparison', Physical Review D - Particles, Fields, Gravitation and Cosmology, vol. 89, no. 8, 084060. https://doi.org/10.1103/PhysRevD.89.084060

Reconstructing the sky location of gravitational-wave detected compact binary systems : Methodology for testing and comparison. / Sidery, T.; Aylott, B.; Christensen, N.; Farr, B.; Farr, W.; Feroz, F.; Gair, J.; Grover, K.; Graff, P.; Hanna, C.; Kalogera, V.; Mandel, I.; O'Shaughnessy, R.; Pitkin, M.; Price, L.; Raymond, V.; Röver, C.; Singer, L.; Van Der Sluys, M.; Smith, R. J.E.; Vecchio, A.; Veitch, J.; Vitale, S.

In: Physical Review D - Particles, Fields, Gravitation and Cosmology, Vol. 89, No. 8, 084060, 18.04.2014.

Research output: Contribution to journalArticle

TY - JOUR

T1 - Reconstructing the sky location of gravitational-wave detected compact binary systems

T2 - Methodology for testing and comparison

AU - Sidery, T.

AU - Aylott, B.

AU - Christensen, N.

AU - Farr, B.

AU - Farr, W.

AU - Feroz, F.

AU - Gair, J.

AU - Grover, K.

AU - Graff, P.

AU - Hanna, C.

AU - Kalogera, V.

AU - Mandel, I.

AU - O'Shaughnessy, R.

AU - Pitkin, M.

AU - Price, L.

AU - Raymond, V.

AU - Röver, C.

AU - Singer, L.

AU - Van Der Sluys, M.

AU - Smith, R. J.E.

AU - Vecchio, A.

AU - Veitch, J.

AU - Vitale, S.

PY - 2014/4/18

Y1 - 2014/4/18

N2 - The problem of reconstructing the sky position of compact binary coalescences detected via gravitational waves is a central one for future observations with the ground-based network of gravitational-wave laser interferometers, such as Advanced LIGO and Advanced Virgo. Different techniques for sky localization have been independently developed. They can be divided in two broad categories: fully coherent Bayesian techniques, which are high latency and aimed at in-depth studies of all the parameters of a source, including sky position, and "triangulation-based" techniques, which exploit the data products from the search stage of the analysis to provide an almost real-time approximation of the posterior probability density function of the sky location of a detection candidate. These techniques have previously been applied to data collected during the last science runs of gravitational-wave detectors operating in the so-called initial configuration. Here, we develop and analyze methods for assessing the self consistency of parameter estimation methods and carrying out fair comparisons between different algorithms, addressing issues of efficiency and optimality. These methods are general, and can be applied to parameter estimation problems other than sky localization. We apply these methods to two existing sky localization techniques representing the two above-mentioned categories, using a set of simulated inspiral-only signals from compact binary systems with a total mass of ≤20M and nonspinning components. We compare the relative advantages and costs of the two techniques and show that sky location uncertainties are on average a factor ≈20 smaller for fully coherent techniques than for the specific variant of the triangulation-based technique used during the last science runs, at the expense of a factor ≈1000 longer processing time.

AB - The problem of reconstructing the sky position of compact binary coalescences detected via gravitational waves is a central one for future observations with the ground-based network of gravitational-wave laser interferometers, such as Advanced LIGO and Advanced Virgo. Different techniques for sky localization have been independently developed. They can be divided in two broad categories: fully coherent Bayesian techniques, which are high latency and aimed at in-depth studies of all the parameters of a source, including sky position, and "triangulation-based" techniques, which exploit the data products from the search stage of the analysis to provide an almost real-time approximation of the posterior probability density function of the sky location of a detection candidate. These techniques have previously been applied to data collected during the last science runs of gravitational-wave detectors operating in the so-called initial configuration. Here, we develop and analyze methods for assessing the self consistency of parameter estimation methods and carrying out fair comparisons between different algorithms, addressing issues of efficiency and optimality. These methods are general, and can be applied to parameter estimation problems other than sky localization. We apply these methods to two existing sky localization techniques representing the two above-mentioned categories, using a set of simulated inspiral-only signals from compact binary systems with a total mass of ≤20M and nonspinning components. We compare the relative advantages and costs of the two techniques and show that sky location uncertainties are on average a factor ≈20 smaller for fully coherent techniques than for the specific variant of the triangulation-based technique used during the last science runs, at the expense of a factor ≈1000 longer processing time.

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