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The principal goal of this whitepaper is not so much to demonstrate that gravitational wave detectors like LIGO and LISA will help answer many central questions in astronomy and astrophysics, but to make the case that they can help answer a far greater range of questions if we prepare to make the (sometimes substantial) effort to identify electromagnetic counterparts to the gravitational wave sources.
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A. Stroeer, A. Vecchio & G. Nelemans “LISA astronomy of double white dwarf binary systems” ApJ 633, L33 (2005) http://arxiv.org/abs/astro-ph/0509632
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M. Milosavljevic, E.S. Phinney “The Afterglow of Massive Black Hole Coalescence” ApJ 622, L93 (2005) http://arxiv.org/abs/astro-ph/0410343
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T. Prince et al, “The Promise of Low-Frequency Gravitational Wave Astronomy”, Astro2010 WP (2009)
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B. Schutz et al “Will Einstein Have the Last Word on Gravity?”, Astro2010 WP (2009)
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S.E. Whitcomb et al “Probing Gravity and Cosmology with Gravitational Waves”, Astro2010 WP (2009)
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P. Madau et al, “Massive Black Holes Across Cosmic Time”, Astro2010 WP (2009)
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M.C. Miller et al “Probing Stellar Dynamics in Galactic Nuclei”, Astro2010 WP (2009)
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G. Nelemans et al, “The Astrophysics of Ultra-Compact Binaries”, Astro2010 WP (2009)
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“Advanced LIGO: Reference Design and Astrophysical Targets” http://www.ligo.caltech.edu/advLIGO
Cited in the paper.
2009
Closest in time.
M. Vallisneri “A LISA Data-Analysis Primer”, http://arXiv.org/abs/0812.0751 (2009)
2009
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2009
Closest in time.
2031
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LISA Mission and Science Documents, including the science case document are at http://www.lisa-science.org/resources/mission/mission_body
Cited in the paper.
C. Hogan et al, “Precision Cosmology with Gravitational Waves”, Astro2010 WP (2009a)
Cited in the paper.