Built on

Misner, C.W., Thorne, K.S., & Wheeler, J.A. 1973, Gravitation, W.H. Freeman, San Francisco
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Earlier work this paper cites.
Abadie, J. et al. 2010, Phys. Rev. D 81, 2001
2001
Earlier work this paper cites.
Kovács, G., Zucker, S., & Mazeh, T. 2002, A&A, 391, 369
2002
Earlier work this paper cites.

Similar

Salim, S. & Gould, A. 2003, ApJ, 582, 1011
2003
Cited alongside, same era.
Prince, T. 2007, LISA: Probing the Universe with Gravitational Waves, lisa.gsfc.nasa.gov/Documentation/LISA-LIST-RP-436_v1.2.pdf
2007
Cited alongside, same era.

Then

Abell, P.A., et al. 2009, LSST Science Book Version 2.0, arXiv:0912.0201
Original
2009
Later among the works it cites.
Thompson, T.A. 2011, ApJ, submitted, arXiv1011.4322
Original
2011
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2010

Gravitational Pulse Astronomy

Gould, Andrew

Understand

Thompson has argued that the Kozai mechanism is primarily responsible for driving white-dwarf binary mergers and so generating type Ia supernovae (SNe).

If so, the gravitational wave signal from these systems will be characterized by isolated repeating pulses that are well approximated by parabolic encounters.
I show that it is impossible to detect these with searches based on standard assumptions of circular binaries, nor could they be detected by analogs of the repeating-pulse searches that have been carried out at higher frequencies, even if these were modified to barycentric time as a function of putative sky position.
Rather, new search algorithms are required that take account of the intrinsic 3-body motion of the source as well as the motion of the Earth.