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Is there potential complementarity between LISA and pulsar timing?

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Is there potential complementarity between LISA and pulsar timing? / Pitkin, M.; Clark, J.; Hendry, M. A. et al.
In: Journal of Physics: Conference Series, Vol. 122, No. 1, 012004, 01.07.2008.

Research output: Contribution to Journal/Magazine › Journal article › peer-review

Harvard

Pitkin, M, Clark, J, Hendry, MA, Heng, IS, Messenger, C, Toher, J & Woan, G 2008, 'Is there potential complementarity between LISA and pulsar timing?', Journal of Physics: Conference Series, vol. 122, no. 1, 012004. https://doi.org/10.1088/1742-6596/122/1/012004

APA

Pitkin, M., Clark, J., Hendry, M. A., Heng, I. S., Messenger, C., Toher, J., & Woan, G. (2008). Is there potential complementarity between LISA and pulsar timing? Journal of Physics: Conference Series, 122(1), Article 012004. https://doi.org/10.1088/1742-6596/122/1/012004

Vancouver

Pitkin M, Clark J, Hendry MA, Heng IS, Messenger C, Toher J et al. Is there potential complementarity between LISA and pulsar timing? Journal of Physics: Conference Series. 2008 Jul 1;122(1):012004. doi: 10.1088/1742-6596/122/1/012004

Author

Pitkin, M. ; Clark, J. ; Hendry, M. A. et al. / Is there potential complementarity between LISA and pulsar timing?. In: Journal of Physics: Conference Series. 2008 ; Vol. 122, No. 1.

Bibtex

@article{de54e899c09f49519f1a27089875bbb4,
title = "Is there potential complementarity between LISA and pulsar timing?",
abstract = "We open the discussion into how the Laser Interferometer Space Antenna (LISA) observations of supermassive black-hole (SMBH) mergers (in the mass range ~ 106–108 M⊙) may be complementary to pulsar timing-based gravitational wave searches. We consider the toy model of determining pulsar distances by exploiting the fact that LISA SMBH inspiral observations can place tight parameter constraints on the signal present in pulsar timing observations. We also suggest, as a future path of research, the use of LISA ring-down observations from the most massive (gsim a few 107 M⊙) black-hole mergers, for which the inspiral stage will lie outside the LISA band, as both a trigger and constraint on searches within pulsar timing data for the inspiral stage of the merger.",
keywords = "Astrophysics, General Relativity and Quantum Cosmology",
author = "M. Pitkin and J. Clark and Hendry, {M. A.} and Heng, {I. S.} and C. Messenger and J. Toher and G. Woan",
year = "2008",
month = jul,
day = "1",
doi = "10.1088/1742-6596/122/1/012004",
language = "English",
volume = "122",
journal = "Journal of Physics: Conference Series",
issn = "1742-6588",
publisher = "IOP Publishing Ltd.",
number = "1",

}

RIS

TY - JOUR

T1 - Is there potential complementarity between LISA and pulsar timing?

AU - Pitkin, M.

AU - Clark, J.

AU - Hendry, M. A.

AU - Heng, I. S.

AU - Messenger, C.

AU - Toher, J.

AU - Woan, G.

PY - 2008/7/1

Y1 - 2008/7/1

N2 - We open the discussion into how the Laser Interferometer Space Antenna (LISA) observations of supermassive black-hole (SMBH) mergers (in the mass range ~ 106–108 M⊙) may be complementary to pulsar timing-based gravitational wave searches. We consider the toy model of determining pulsar distances by exploiting the fact that LISA SMBH inspiral observations can place tight parameter constraints on the signal present in pulsar timing observations. We also suggest, as a future path of research, the use of LISA ring-down observations from the most massive (gsim a few 107 M⊙) black-hole mergers, for which the inspiral stage will lie outside the LISA band, as both a trigger and constraint on searches within pulsar timing data for the inspiral stage of the merger.

AB - We open the discussion into how the Laser Interferometer Space Antenna (LISA) observations of supermassive black-hole (SMBH) mergers (in the mass range ~ 106–108 M⊙) may be complementary to pulsar timing-based gravitational wave searches. We consider the toy model of determining pulsar distances by exploiting the fact that LISA SMBH inspiral observations can place tight parameter constraints on the signal present in pulsar timing observations. We also suggest, as a future path of research, the use of LISA ring-down observations from the most massive (gsim a few 107 M⊙) black-hole mergers, for which the inspiral stage will lie outside the LISA band, as both a trigger and constraint on searches within pulsar timing data for the inspiral stage of the merger.

KW - Astrophysics

KW - General Relativity and Quantum Cosmology

U2 - 10.1088/1742-6596/122/1/012004

DO - 10.1088/1742-6596/122/1/012004

M3 - Journal article

VL - 122

JO - Journal of Physics: Conference Series

JF - Journal of Physics: Conference Series

SN - 1742-6588

IS - 1

M1 - 012004

ER -