text:
04.08472.x}}

@article{Fairbank:1967,
	Author = {Witteborn, F. C. and Fairbank, W. M.},
	Date-Added = {2012-04-28 04:24:39 +0000},
	Date-Modified = {2012-04-28 04:24:50 +0000},
	Doi = {10.1103/PhysRevLett.19.1049},
	Issue = {18},
	Journal = {Phys. Rev. Lett.},
	Month = {Oct},
	Pages = {1049--1052},
	Publisher = {American Physical Society},
	Title = {Experimental Comparison of the Gravitational Force on Freely Falling Electrons and Metallic Electrons},
	Url = {http://link.aps.org/doi/10.1103/PhysRevLett.19.1049},
	Volume = {19},
	Year = {1967},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevLett.19.1049},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevLett.19.1049}}

@inproceedings{Campbell:1965,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/1965eqae.conf..495C},
	Author = {{Campbell}, W.~H.},
	Booktitle = {Report on Equatorial Aeronomy},
	Date-Added = {2012-04-28 04:23:26 +0000},
	Date-Modified = {2012-04-28 04:23:38 +0000},
	Editor = {{de Mendon{\c c}a}, F.},
	Pages = {495},
	Title = {{Review - equatorial studies of rapid fluctuations in the earth's magnetic field}},
	Year = 1965}

@book{bass2009handbook,
	Author = {Bass, M. and Mahajan, V.N.},
	Date-Added = {2012-04-21 07:24:20 +0000},
	Date-Modified = {2012-04-21 07:24:20 +0000},
	Isbn = {9780071498890},
	Number = {v. 1},
	Publisher = {McGraw-Hill},
	Title = {Handbook of Optics: Geometrical and Physical Optics, Polarized Light, Components and Instruments},
	Url = {http://books.google.com/books?id=xmDntwAACAAJ},
	Year = {2009},
	Bdsk-Url-1 = {http://books.google.com/books?id=xmDntwAACAAJ}}

@inproceedings{Zygo:2011,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2011SPIE.8126E..29S},
	Author = {{Sykora}, D.~M. and {de Groot}, P.},
	Booktitle = {Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series},
	Date-Added = {2012-04-21 06:06:09 +0000},
	Date-Modified = {2012-04-21 06:06:18 +0000},
	Doi = {10.1117/12.894676},
	Month = sep,
	Series = {Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series},
	Title = {{Instantaneous measurement Fizeau interferometer with high spatial resolution}},
	Volume = 8126,
	Year = 2011,
	Bdsk-Url-1 = {http://dx.doi.org/10.1117/12.894676}}

@misc{Gari:Zygo,
	Author = {ZygoEPO},
	Date-Added = {2012-04-11 17:28:52 -0700},
	Date-Modified = {2012-12-31 23:40:52 -0800},
	Howpublished = {Metrology Report},
	Institution = {L3 Communications},
	Title = {{ITM04} Phasemap},
	Year = {2011}}

@misc{Takahashi:email,
	Author = {Ryutaro Takahashi},
	Date-Added = {2012-03-06 14:21:46 -0800},
	Date-Modified = {2012-03-06 14:22:30 -0800},
	Howpublished = {personal communication},
	Keywords = {email},
	Month = {March},
	Year = {2012}}

@article{Bildsten:2000,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2000MNRAS.319..902U},
	Author = {{Ushomirsky}, G. and {Cutler}, C. and {Bildsten}, L.},
	Date-Added = {2012-02-28 07:44:02 -0800},
	Date-Modified = {2012-02-28 07:44:30 -0800},
	Doi = {10.1046/j.1365-8711.2000.03938.x},
	Eprint = {arXiv:astro-ph/0001136},
	Journal = {Monthly Notices of the Royal Astronomical Society},
	Keywords = {ACCRETION, ACCRETION DISCS, DENSE MATTER, RADIATION MECHANISMS: NON-THERMAL, STARS: NEUTRON, STARS: ROTATION},
	Month = dec,
	Pages = {902-932},
	Title = {{Deformations of accreting neutron star crusts and gravitational wave emission}},
	Volume = 319,
	Year = 2000,
	Bdsk-Url-1 = {http://dx.doi.org/10.1046/j.1365-8711.2000.03938.x}}

@article{LIGO:SGR,
	Author = {Abbott, B. and Abbott, R. and Adhikari, R. and Ajith, P. and Allen, B. and Allen, G. and Amin, R. and Anderson, S. B. and Anderson, W. G. and Arain, M. A. and Araya, M. and Armandula, H. and Armor, P. and Aso, Y. and Aston, S. and Aufmuth, P. and Aulbert, C. and Babak, S. and Ballmer, S. and Bantilan, H. and Barish, B. C. and Barker, C. and Barker, D. and Barr, B. and Barriga, P. and Barton, M. A. and Bartos, I. and Bastarrika, M. and Bayer, K. and Betzwieser, J. and Beyersdorf, P. T. and Bilenko, I. A. and Billingsley, G. and Biswas, R. and Black, E. and Blackburn, K. and Blackburn, L. and Blair, D. and Bland, B. and Bodiya, T. P. and Bogue, L. and Bork, R. and Boschi, V. and Bose, S. and Brady, P. R. and Braginsky, V. B. and Brau, J. E. and Brinkmann, M. and Brooks, A. and Brown, D. A. and Brunet, G. and Bullington, A. and Buonanno, A. and Burmeister, O. and Byer, R. L. and Cadonati, L. and Cagnoli, G. and Camp, J. B. and Cannizzo, J. and Cannon, K. and Cao, J. and Cardenas, L. and Casebolt, T. and Castaldi, G. and Cepeda, C. and Chalkley, E. and Charlton, P. and Chatterji, S. and Chelkowski, S. and Chen, Y. and Christensen, N. and Clark, D. and Clark, J. and Cokelaer, T. and Conte, R. and Cook, D. and Corbitt, T. and Coyne, D. and Creighton, J. D. E. and Cumming, A. and Cunningham, L. and Cutler, R. M. and Dalrymple, J. and Danzmann, K. and Davies, G. and DeBra, D. and Degallaix, J. and Degree, M. and Dergachev, V. and Desai, S. and DeSalvo, R. and Dhurandhar, S. and D\'\iaz, M. and Dickson, J. and Dietz, A. and Donovan, F. and Dooley, K. L. and Doomes, E. E. and Drever, R. W. P. and Duke, I. and Dumas, J.-C. and Dupuis, R. J. and Dwyer, J. G. and Echols, C. and Effler, A. and Ehrens, P. and Espinoza, E. and Etzel, T. and Evans, T. and Fairhurst, S. and Fan, Y. and Fazi, D. and Fehrmann, H. and Fejer, M. M. and Finn, L. S. and Flasch, K. and Fotopoulos, N. and Freise, A. and Frey, R. and Fricke, T. and Fritschel, P. and Frolov, V. V. and Fyffe, M. and Garofoli, J. and Gholami, I. and Giaime, J. A. and Giampanis, S. and Giardina, K. D. and Goda, K. and Goetz, E. and Goggin, L. and Gonz\'alez, G. and Gossler, S. and Gouaty, R. and Grant, A. and Gras, S. and Gray, C. and Gray, M. and Greenhalgh, R. J. S. and Gretarsson, A. M. and Grimaldi, F. and Grosso, R. and Grote, H. and Grunewald, S. and Guenther, M. and Gustafson, E. K. and Gustafson, R. and Hage, B. and Hallam, J. M. and Hammer, D. and Hanna, C. and Hanson, J. and Harms, J. and Harry, G. and Harstad, E. and Hayama, K. and Hayler, T. and Heefner, J. and Heng, I. S. and Hennessy, M. and Heptonstall, A. and Hewitson, M. and Hild, S. and Hirose, E. and Hoak, D. and Hosken, D. and Hough, J. and Huttner, S. H. and Ingram, D. and Ito, M. and Ivanov, A. and Johnson, B. and Johnson, W. W. and Jones, D. I. and Jones, G. and Jones, R. and Ju, L. and Kalmus, P. and Kalogera, V. and Kamat, S. and Kanner, J. and Kasprzyk, D. and Katsavounidis, E. and Kawabe, K. and Kawamura, S. and Kawazoe, F. and Kells, W. and Keppel, D. G. and Khalili, F. Ya. and Khan, R. and Khazanov, E. and Kim, C. and King, P. and Kissel, J. S. and Klimenko, S. and Kokeyama, K. and Kondrashov, V. and Kopparapu, R. K. and Kozak, D. and Kozhevatov, I. and Krishnan, B. and Kwee, P. and Lam, P. K. and Landry, M. and Lang, M. M. and Lantz, B. and Lazzarini, A. and Lei, M. and Leindecker, N. and Leonhardt, V. and Leonor, I. and Libbrecht, K. and Lin, H. and Lindquist, P. and Lockerbie, N. A. and Lodhia, D. and Lormand, M. and Lu, P. and Lubinski, M. and Lucianetti, A. and L\"uck, H. and Machenschalk, B. and MacInnis, M. and Mageswaran, M. and Mailand, K. and Mandic, V. and M\'arka, S. and M\'arka, Z. and Markosyan, A. and Markowitz, J. and Maros, E. and Martin, I. and Martin, R. M. and Marx, J. N. and Mason, K. and Matichard, F. and Matone, L. and Matzner, R. and Mavalvala, N. and McCarthy, R. and McClelland, D. E. and McGuire, S. C. and McHugh, M. and McIntyre, G. and McIvor, G. and McKechan, D. and McKenzie, K. and Meier, T. and Melissinos, A. and Mendell, G. and Mercer, R. A. and Meshkov, S. and Messenger, C. J. and Meyers, D. and Miller, J. and Minelli, J. and Mitra, S. and Mitrofanov, V. P. and Mitselmakher, G. and Mittleman, R. and Miyakawa, O. and Moe, B. and Mohanty, S. and Moreno, G. and Mossavi, K. and MowLowry, C. and Mueller, G. and Mukherjee, S. and Mukhopadhyay, H. and M\"uller-Ebhardt, H. and Munch, J. and Murray, P. and Myers, E. and Myers, J. and Nash, T. and Nelson, J. and Newton, G. and Nishizawa, A. and Numata, K. and O'Dell, J. and Ogin, G. and O'Reilly, B. and O'Shaughnessy, R. and Ottaway, D. J. and Ottens, R. S. and Overmier, H. and Owen, B. J. and Pan, Y. and Pankow, C. and Papa, M. A. and Parameshwaraiah, V. and Patel, P. and Pedraza, M. and Penn, S. and Perreca, A. and Petrie, T. and Pinto, I. M. and Pitkin, M. and Pletsch, H. J. and Plissi, M. V. and Postiglione, F. and Principe, M. and Prix, R. and Quetschke, V. and Raab, F. and Rabeling, D. S. and Radkins, H. and Rainer, N. and Rakhmanov, M. and Ramsunder, M. and Rehbein, H. and Reid, S. and Reitze, D. H. and Riesen, R. and Riles, K. and Rivera, B. and Robertson, N. A. and Robinson, C. and Robinson, E. L. and Roddy, S. and Rodriguez, A. and Rogan, A. M. and Rollins, J. and Romano, J. D. and Romie, J. and Route, R. and Rowan, S. and R\"udiger, A. and Ruet, L. and Russell, P. and Ryan, K. and Sakata, S. and Samidi, M. and de la Jordana, L. Sancho and Sandberg, V. and Sannibale, V. and Saraf, S. and Sarin, P. and Sathyaprakash, B. S. and Sato, S. and Saulson, P. R. and Savage, R. and Savov, P. and Schediwy, S. W. and Schilling, R. and Schnabel, R. and Schofield, R. and Schutz, B. F. and Schwinberg, P. and Scott, S. M. and Searle, A. C. and Sears, B. and Seifert, F. and Sellers, D. and Sengupta, A. S. and Shawhan, P. and Shoemaker, D. H. and Sibley, A. and Siemens, X. and Sigg, D. and Sinha, S. and Sintes, A. M. and Slagmolen, B. J. J. and Slutsky, J. and Smith, J. R. and Smith, M. R. and Smith, N. D. and Somiya, K. and Sorazu, B. and Stein, L. C. and Stochino, A. and Stone, R. and Strain, K. A. and Strom, D. M. and Stuver, A. and Summerscales, T. Z. and Sun, K.-X. and Sung, M. and Sutton, P. J. and Takahashi, H. and Tanner, D. B. and Taylor, R. and Taylor, R. and Thacker, J. and Thorne, K. A. and Thorne, K. S. and Th\"uring, A. and Tokmakov, K. V. and Torres, C. and Torrie, C. and Traylor, G. and Trias, M. and Tyler, W. and Ugolini, D. and Ulmen, J. and Urbanek, K. and Vahlbruch, H. and Van Den Broeck, C. and van der Sluys, M. and Vass, S. and Vaulin, R. and Vecchio, A. and Veitch, J. and Veitch, P. and Villar, A. and Vorvick, C. and Vyachanin, S. P. and Waldman, S. J. and Wallace, L. and Ward, H. and Ward, R. and Weinert, M. and Weinstein, A. and Weiss, R. and Wen, S. and Wette, K. and Whelan, J. T. and Whitcomb, S. E. and Whiting, B. F. and Wilkinson, C. and Willems, P. A. and Williams, H. R. and Williams, L. and Willke, B. and Wilmut, I. and Winkler, W. and Wipf, C. C. and Wiseman, A. G. and Woan, G. and Wooley, R. and Worden, J. and Wu, W. and Yakushin, I. and Yamamoto, H. and Yan, Z. and Yoshida, S. and Zanolin, M. and Zhang, J. and Zhang, L. and Zhao, C. and Zotov, N. and Zucker, M. and Zweizig, J. and Barthelmy, S. and Gehrels, N. and Hurley, K. C. and Palmer, D.},
	Collaboration = {LIGO Scientific Collaboration},
	Date-Added = {2012-02-21 16:48:43 -0800},
	Date-Modified = {2012-02-21 16:48:54 -0800},
	Doi = {10.1103/PhysRevLett.101.211102},
	Issue = {21},
	Journal = {Phys. Rev. Lett.},
	Month = {Nov},
	Numpages = {6},
	Pages = {211102},
	Publisher = {American Physical Society},
	Title = {Search for Gravitational-Wave Bursts from Soft Gamma Repeaters},
	Url = {http://link.aps.org/doi/10.1103/PhysRevLett.101.211102},
	Volume = {101},
	Year = {2008},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevLett.101.211102},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevLett.101.211102}}

@article{Lee:NS2001,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2001MNRAS.324.1063L},
	Author = {{Liu}, Y.~T. and {Lindblom}, L.},
	Date-Added = {2012-02-21 16:46:32 -0800},
	Date-Modified = {2012-02-21 16:46:52 -0800},
	Doi = {10.1046/j.1365-8711.2001.04395.x},
	Eprint = {arXiv:astro-ph/0012198},
	Journal = {Monthly Notices of the Royal Astronomical Society},
	Keywords = {INSTABILITIES, STARS: INTERIORS, STARS: NEUTRON, STARS: ROTATION, WHITE DWARFS},
	Month = jul,
	Pages = {1063-1073},
	Title = {{Models of rapidly rotating neutron stars: remnants of accretion-induced collapse}},
	Volume = 324,
	Year = 2001,
	Bdsk-Url-1 = {http://dx.doi.org/10.1046/j.1365-8711.2001.04395.x}}

@article{Yanbei:Local,
	Author = {Rehbein, Henning and M\"uller-Ebhardt, Helge and Somiya, Kentaro and Li, Chao and Schnabel, Roman and Danzmann, Karsten and Chen, Yanbei},
	Date-Added = {2012-02-21 15:59:48 -0800},
	Date-Modified = {2012-02-21 15:59:58 -0800},
	Doi = {10.1103/PhysRevD.76.062002},
	Issue = {6},
	Journal = {Phys. Rev. D},
	Month = {Sep},
	Numpages = {10},
	Pages = {062002},
	Publisher = {American Physical Society},
	Title = {Local readout enhancement for detuned signal-recycling interferometers},
	Url = {http://link.aps.org/doi/10.1103/PhysRevD.76.062002},
	Volume = {76},
	Year = {2007},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.76.062002},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.76.062002}}

@article{Yanbei:DoubleSpring,
	Author = {Rehbein, Henning and M\"uller-Ebhardt, Helge and Somiya, Kentaro and Danilishin, Stefan L. and Schnabel, Roman and Danzmann, Karsten and Chen, Yanbei},
	Date-Added = {2012-02-21 15:58:45 -0800},
	Date-Modified = {2012-02-21 15:59:11 -0800},
	Doi = {10.1103/PhysRevD.78.062003},
	Issue = {6},
	Journal = {Phys. Rev. D},
	Month = {Sep},
	Numpages = {11},
	Pages = {062003},
	Publisher = {American Physical Society},
	Title = {Double optical spring enhancement for gravitational-wave detectors},
	Url = {http://link.aps.org/doi/10.1103/PhysRevD.78.062003},
	Volume = {78},
	Year = {2008},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.78.062003},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.78.062003}}

@article{LSC:rates,
	Abstract = {We present an up-to-date, comprehensive summary of the rates for all types of compact binary coalescence sources detectable by the initial and advanced versions of the ground-based gravitational-wave detectors LIGO and Virgo. Astrophysical estimates for compact-binary coalescence rates depend on a number of assumptions and unknown model parameters and are still uncertain. The most confident among these estimates are the rate predictions for coalescing binary neutron stars which are based on extrapolations from observed binary pulsars in our galaxy. These yield a likely coalescence rate of 100 Myr −1 per Milky Way Equivalent Galaxy (MWEG), although the rate could plausibly range from 1 Myr −1 MWEG −1 to 1000 Myr −1 MWEG −1 (Kalogera et al 2004 Astrophys. J. 601 L179; Kalogera et al 2004 Astrophys. J. 614 L137 (erratum)). We convert coalescence rates into detection rates based on data from the LIGO S5 and Virgo VSR2 science runs and projected sensitivities for our advanced detectors. Using the detector sensitivities derived from these data, we find a likely detection rate of 0.02 per year for Initial LIGO--Virgo interferometers, with a plausible range between 2 × 10 −4 and 0.2 per year. The likely binary neutron--star detection rate for the Advanced LIGO--Virgo network increases to 40 events per year, with a range between 0.4 and 400 per year.},
	Author = {J Abadie and B P Abbott and R Abbott and M Abernathy and T Accadia and F Acernese and C Adams and R Adhikari and P Ajith and B Allen and G Allen and E Amador Ceron and R S Amin and S B Anderson and W G Anderson and F Antonucci and S Aoudia and M A Arain and M Araya and M Aronsson and K G Arun and Y Aso and S Aston and P Astone and D E Atkinson and P Aufmuth and C Aulbert and S Babak and P Baker and G Ballardin and S Ballmer and D Barker and S Barnum and F Barone and B Barr and P Barriga and L Barsotti and M Barsuglia and M A Barton and I Bartos and R Bassiri and M Bastarrika and J Bauchrowitz and Th S Bauer and B Behnke and M G Beker and M Benacquista and A Bertolini and J Betzwieser and N Beveridge and P T Beyersdorf and S Bigotta and I A Bilenko and G Billingsley and J Birch and S Birindelli and R Biswas and M Bitossi and M A Bizouard and E Black and J K Blackburn and L Blackburn and D Blair and B Bland and M Blom and A Blomberg and C Boccara and O Bock and T P Bodiya and R Bondarescu and F Bondu and L Bonelli and R Bork and M Born and S Bose and L Bosi and M Boyle and S Braccini and C Bradaschia and P R Brady and V B Braginsky and J E Brau and J Breyer and D O Bridges and A Brillet and M Brinkmann and V Brisson and M Britzger and A F Brooks and D A Brown and R Budzy{\'n}ski and T Bulik and H J Bulten and A Buonanno and J Burguet-Castell and O Burmeister and D Buskulic and R L Byer and L Cadonati and G Cagnoli and E Calloni and J B Camp and E Campagna and P Campsie and J Cannizzo and K C Cannon and B Canuel and J Cao and C Capano and F Carbognani and S Caride and S Caudill and M Cavagli{\`a} and F Cavalier and R Cavalieri and G Cella and C Cepeda and E Cesarini and T Chalermsongsak and E Chalkley and P Charlton and E Chassande Mottin and S Chelkowski and Y Chen and A Chincarini and N Christensen and S S Y Chua and C T Y Chung and D Clark and J Clark and J H Clayton and F Cleva and E Coccia and C N Colacino and J Colas and A Colla and M Colombini and R Conte and D Cook and T R Corbitt and C Corda and N Cornish and A Corsi and C A Costa and J P Coulon and D Coward and D C Coyne and J D E Creighton and T D Creighton and A M Cruise and R M Culter and A Cumming and L Cunningham and E Cuoco and K Dahl and S L Danilishin and R Dannenberg and S D'Antonio and K Danzmann and A Dari and K Das and V Dattilo and B Daudert and M Davier and G Davies and A Davis and E J Daw and R Day and T Dayanga and R De Rosa and D DeBra and J Degallaix and M del Prete and V Dergachev and R DeRosa and R DeSalvo and P Devanka and S Dhurandhar and L Di Fiore and A Di Lieto and I Di Palma and M Di Paolo Emilio and A Di Virgilio and M D{\'\i}az and A Dietz and F Donovan and K L Dooley and E E Doomes and S Dorsher and E S D Douglas and M Drago and R W P Drever and J C Driggers and J Dueck and J C Dumas and T Eberle and M Edgar and M Edwards and A Effler and P Ehrens and R Engel and T Etzel and M Evans and T Evans and V Fafone and S Fairhurst and Y Fan and B F Farr and D Fazi and H Fehrmann and D Feldbaum and I Ferrante and F Fidecaro and L S Finn and I Fiori and R Flaminio and M Flanigan and K Flasch and S Foley and C Forrest and E Forsi and N Fotopoulos and J D Fournier and J Franc and S Frasca and F Frasconi and M Frede and M Frei and Z Frei and A Freise and R Frey and T T Fricke and D Friedrich and P Fritschel and V V Frolov and P Fulda and M Fyffe and L Gammaitoni and J A Garofoli and F Garufi and G Gemme and E Genin and A Gennai and I Gholami and S Ghosh and J A Giaime and S Giampanis and K D Giardina and A Giazotto and C Gill and E Goetz and L M Goggin and G Gonz{\'a}lez and M L Gorodetsky and S Go{\ss}ler and R Gouaty and C Graef and M Granata and A Grant and S Gras and C Gray and R J S Greenhalgh and A M Gretarsson and C Greverie and R Grosso and H Grote and S Grunewald and G M Guidi and E K Gustafson and R Gustafson and B Hage and P Hall and J M Hallam and D Hammer and G Hammond and J Hanks and C Hanna and J Hanson and J Harms and G M Harry and I W Harry and E D Harstad and K Haughian and K Hayama and J Heefner and H Heitmann and P Hello and I S Heng and A Heptonstall and M Hewitson and S Hild and E Hirose and D Hoak and K A Hodge and K Holt and D J Hosken and J Hough and E Howell and D Hoyland and D Huet and B Hughey and S Husa and S H Huttner and T Huynh-Dinh and D R Ingram and R Inta and T Isogai and A Ivanov and P Jaranowski and W W Johnson and D I Jones and G Jones and R Jones and L Ju and P Kalmus and V Kalogera and S Kandhasamy and J Kanner and E Katsavounidis and K Kawabe and S Kawamura and F Kawazoe and W Kells and D G Keppel and A Khalaidovski and F Y Khalili and E A Khazanov and C Kim and H Kim and P J King and D L Kinzel and J S Kissel and S Klimenko and V Kondrashov and R Kopparapu and S Koranda and I Kowalska and D Kozak and T Krause and V Kringel and S Krishnamurthy and B Krishnan and A Kr{\'o}lak and G Kuehn and J Kullman and R Kumar and P Kwee and M Landry and M Lang and B Lantz and N Lastzka and A Lazzarini and P Leaci and J Leong and I Leonor and N Leroy and N Letendre and J Li and T G F Li and H Lin and P E Lindquist and N A Lockerbie and D Lodhia and M Lorenzini and V Loriette and M Lormand and G Losurdo and P Lu and J Luan and M Lubinski and A Lucianetti and H L{\"u}ck and A Lundgren and B Machenschalk and M MacInnis and J M Mackowski and M Mageswaran and K Mailand and E Majorana and C Mak and N Man and I Mandel and V Mandic and M Mantovani and F Marchesoni and F Marion and S M{\'a}rka and Z M{\'a}rka and E Maros and J Marque and F Martelli and I W Martin and R M Martin and J N Marx and K Mason and A Masserot and F Matichard and L Matone and R A Matzner and N Mavalvala and R McCarthy and D E McClelland and S C McGuire and G McIntyre and G McIvor and D J A McKechan and G Meadors and M Mehmet and T Meier and A Melatos and A C Melissinos and G Mendell and D F Men{\'e}ndez and R A Mercer and L Merill and S Meshkov and C Messenger and M S Meyer and H Miao and C Michel and L Milano and J Miller and Y Minenkov and Y Mino and S Mitra and V P Mitrofanov and G Mitselmakher and R Mittleman and B Moe and M Mohan and S D Mohanty and S R P Mohapatra and D Moraru and J Moreau and G Moreno and N Morgado and A Morgia and T Morioka and K Mors and S Mosca and V Moscatelli and K Mossavi and B Mours and C MowLowry and G Mueller and S Mukherjee and A Mullavey and H M{\"u}ller-Ebhardt and J Munch and P G Murray and T Nash and R Nawrodt and J Nelson and I Neri and G Newton and A Nishizawa and F Nocera and D Nolting and E Ochsner and J O'Dell and G H Ogin and R G Oldenburg and B O'Reilly and R O'Shaughnessy and C Osthelder and D J Ottaway and R S Ottens and H Overmier and B J Owen and A Page and G Pagliaroli and L Palladino and C Palomba and Y Pan and C Pankow and F Paoletti and M A Papa and S Pardi and M Pareja and M Parisi and A Pasqualetti and R Passaquieti and D Passuello and P Patel and M Pedraza and L Pekowsky and S Penn and C Peralta and A Perreca and G Persichetti and M Pichot and M Pickenpack and F Piergiovanni and M Pietka and L Pinard and I M Pinto and M Pitkin and H J Pletsch and M V Plissi and R Poggiani and F Postiglione and M Prato and V Predoi and L R Price and M Prijatelj and M Principe and S Privitera and R Prix and G A Prodi and L Prokhorov and O Puncken and M Punturo and P Puppo and V Quetschke and F J Raab and O Rabaste and D S Rabeling and T Radke and H Radkins and P Raffai and M Rakhmanov and B Rankins and P Rapagnani and V Raymond and V Re and C M Reed and T Reed and T Regimbau and S Reid and D H Reitze and F Ricci and R Riesen and K Riles and P Roberts and N A Robertson and F Robinet and C Robinson and E L Robinson and A Rocchi and S Roddy and C R{\"o}ver and S Rogstad and L Rolland and J Rollins and J D Romano and R Romano and J H Romie and D Rosi{\'n}ska and S Rowan and A R{\"u}diger and P Ruggi and K Ryan and S Sakata and M Sakosky and F Salemi and L Sammut and L Sancho de la Jordana and V Sandberg and V Sannibale and L Santamar{\'\i}a and G Santostasi and S Saraf and B Sassolas and B S Sathyaprakash and S Sato and M Satterthwaite and P R Saulson and R Savage and R Schilling and R Schnabel and R Schofield and B Schulz and B F Schutz and P Schwinberg and J Scott and S M Scott and A C Searle and F Seifert and D Sellers and A S Sengupta and D Sentenac and A Sergeev and D A Shaddock and B Shapiro and P Shawhan and D H Shoemaker and A Sibley and X Siemens and D Sigg and A Singer and A M Sintes and G Skelton and B J J Slagmolen and J Slutsky and J R Smith and M R Smith and N D Smith and K Somiya and B Sorazu and F C Speirits and A J Stein and L C Stein and S Steinlechner and S Steplewski and A Stochino and R Stone and K A Strain and S Strigin and A Stroeer and R Sturani and A L Stuver and T Z Summerscales and M Sung and S Susmithan and P J Sutton and B Swinkels and D Talukder and D B Tanner and S P Tarabrin and J R Taylor and R Taylor and P Thomas and K A Thorne and K S Thorne and E Thrane and A Th{\"u}ring and C Titsler and K V Tokmakov and A Toncelli and M Tonelli and C Torres and C I Torrie and E Tournefier and F Travasso and G Traylor and M Trias and J Trummer and K Tseng and D Ugolini and K Urbanek and H Vahlbruch and B Vaishnav and G Vajente and M Vallisneri and J F J van den Brand and C Van Den Broeck and S van der Putten and M V van der Sluys and A A van Veggel and S Vass and R Vaulin and M Vavoulidis and A Vecchio and G Vedovato and J Veitch and P J Veitch and C Veltkamp and D Verkindt and F Vetrano and A Vicer{\'e} and A Villar and J-Y Vinet and H Vocca and C Vorvick and S P Vyachanin and S J Waldman and L Wallace and A Wanner and R L Ward and M Was and P Wei and M Weinert and A J Weinstein and R Weiss and L Wen and S Wen and P Wessels and M West and T Westphal and K Wette and J T Whelan and S E Whitcomb and D J White and B F Whiting and C Wilkinson and P A Willems and L Williams and B Willke and L Winkelmann and W Winkler and C C Wipf and A G Wiseman and G Woan and R Wooley and J Worden and I Yakushin and H Yamamoto and K Yamamoto and D Yeaton-Massey and S Yoshida and P P Yu and M Yvert and M Zanolin and L Zhang and Z Zhang and C Zhao and N Zotov and M E Zucker and J Zweizig and The LIGO Scientific Collaboration and the Virgo Collaboration and K Belczynski},
	Date-Added = {2012-02-21 14:58:31 -0800},
	Date-Modified = {2012-02-21 14:58:31 -0800},
	Journal = {Classical and Quantum Gravity},
	Number = {17},
	Pages = {173001},
	Title = {Predictions for the rates of compact binary coalescences observable by ground-based gravitational-wave detectors},
	Volume = {27},
	Year = {2010},
	Bdsk-Url-1 = {http://stacks.iop.org/0264-9381/27/i=17/a=173001}}

@article{Go:40m,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2008NatPh...4..472G},
	Archiveprefix = {arXiv},
	Author = {{Goda}, K. and {Miyakawa}, O. and {Mikhailov}, E.~E. and {Saraf}, S. and {Adhikari}, R. and {McKenzie}, K. and {Ward}, R. and {Vass}, S. and {Weinstein}, A.~J. and {Mavalvala}, N.},
	Date-Added = {2012-02-21 14:52:31 -0800},
	Date-Modified = {2012-02-21 14:52:40 -0800},
	Doi = {10.1038/nphys920},
	Eprint = {0802.4118},
	Journal = {Nature Physics},
	Month = mar,
	Pages = {472-476},
	Primaryclass = {quant-ph},
	Title = {{A quantum-enhanced prototype gravitational-wave detector}},
	Volume = 4,
	Year = 2008,
	Bdsk-Url-1 = {http://dx.doi.org/10.1038/nphys920}}

@phdthesis{KirksThesis,
	Author = {Mckenzie, Kirk},
	Citeulike-Article-Id = {4725019},
	Date-Added = {2012-02-21 14:50:09 -0800},
	Date-Modified = {2012-02-21 14:50:09 -0800},
	Day = {6},
	Keywords = {ligo, quantum-optics},
	Month = feb,
	Posted-At = {2009-06-03 00:04:22},
	Priority = {2},
	School = {Australian National University},
	Title = {{Squeezing in the Audio Gravitational Wave Detection Band}},
	Year = {2008}}

@article{Henning:PRL2006,
	Author = {Vahlbruch, Henning and Chelkowski, Simon and Hage, Boris and Franzen, Alexander and Danzmann, Karsten and Schnabel, Roman},
	Date-Added = {2012-02-21 14:48:35 -0800},
	Date-Modified = {2012-02-21 14:48:55 -0800},
	Doi = {10.1103/PhysRevLett.97.011101},
	Issue = {1},
	Journal = {Phys. Rev. Lett.},
	Month = {Jul},
	Numpages = {4},
	Pages = {011101},
	Publisher = {American Physical Society},
	Title = {Coherent Control of Vacuum Squeezing in the Gravitational-Wave Detection Band},
	Url = {http://link.aps.org/doi/10.1103/PhysRevLett.97.011101},
	Volume = {97},
	Year = {2006},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevLett.97.011101},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevLett.97.011101}}

@article{Kirk:2004,
	Author = {McKenzie, Kirk and Grosse, Nicolai and Bowen, Warwick P. and Whitcomb, Stanley E. and Gray, Malcolm B. and McClelland, David E. and Lam, Ping Koy},
	Date-Added = {2012-02-21 14:48:02 -0800},
	Date-Modified = {2012-02-21 14:48:13 -0800},
	Doi = {10.1103/PhysRevLett.93.161105},
	Issue = {16},
	Journal = {Phys. Rev. Lett.},
	Month = {Oct},
	Numpages = {4},
	Pages = {161105},
	Publisher = {American Physical Society},
	Title = {Squeezing in the Audio Gravitational-Wave Detection Band},
	Url = {http://link.aps.org/doi/10.1103/PhysRevLett.93.161105},
	Volume = {93},
	Year = {2004},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevLett.93.161105},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevLett.93.161105}}

@article{Kimble:1986,
	Author = {Wu, Ling-An and Kimble, H. J. and Hall, J. L. and Wu, Huifa},
	Date-Added = {2012-02-21 14:45:17 -0800},
	Date-Modified = {2012-02-21 14:45:29 -0800},
	Doi = {10.1103/PhysRevLett.57.2520},
	Issue = {20},
	Journal = {Phys. Rev. Lett.},
	Month = {Nov},
	Pages = {2520--2523},
	Publisher = {American Physical Society},
	Title = {Generation of Squeezed States by Parametric Down Conversion},
	Url = {http://link.aps.org/doi/10.1103/PhysRevLett.57.2520},
	Volume = {57},
	Year = {1986},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevLett.57.2520},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevLett.57.2520}}

@article{Dim:PRD2011,
	Author = {Dimopoulos, Savas and Graham, Peter W. and Hogan, Jason M. and Kasevich, Mark A. and Rajendran, Surjeet},
	Date-Added = {2012-02-21 13:39:38 -0800},
	Date-Modified = {2012-02-21 13:39:53 -0800},
	Doi = {10.1103/PhysRevD.84.028102},
	Issue = {2},
	Journal = {Phys. Rev. D},
	Month = {Jul},
	Numpages = {2},
	Pages = {028102},
	Publisher = {American Physical Society},
	Title = {Reply to ``Comment on `Atomic gravitational wave interferometric sensor' ''},
	Url = {http://link.aps.org/doi/10.1103/PhysRevD.84.028102},
	Volume = {84},
	Year = {2011},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.84.028102},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.84.028102}}

@article{Bender:PRD2011,
	Author = {Bender, Peter L.},
	Date-Added = {2012-02-21 13:38:14 -0800},
	Date-Modified = {2012-02-21 13:38:27 -0800},
	Doi = {10.1103/PhysRevD.84.028101},
	Issue = {2},
	Journal = {Phys. Rev. D},
	Month = {Jul},
	Numpages = {3},
	Pages = {028101},
	Publisher = {American Physical Society},
	Title = {Comment on ``Atomic gravitational wave interferometric sensor''},
	Url = {http://link.aps.org/doi/10.1103/PhysRevD.84.028101},
	Volume = {84},
	Year = {2011},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.84.028101},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.84.028101}}

@book{300:years,
	Date-Added = {2012-02-21 05:23:43 -0800},
	Date-Modified = {2013-01-17 07:38:19 +0000},
	Editor = {Hawking, S.W. and Israel, W.},
	Isbn = {9780521379762},
	Publisher = {Cambridge University Press},
	Series = {Philosophiae Naturalis, Principia Mathematica},
	Title = {{Three Hundred Years of Gravitation}},
	Year = {1989},
	Bdsk-Url-1 = {http://books.google.com/books?id=Vq787qC5PWQC}}

@article{Yagi:DECIGOalt,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2010PThPh.123.1069Y},
	Archiveprefix = {arXiv},
	Author = {{Yagi}, K. and {Tanaka}, T.},
	Date-Added = {2012-02-21 04:43:37 -0800},
	Date-Modified = {2012-02-21 04:44:06 -0800},
	Eprint = {0908.3283},
	Journal = {Progress of Theoretical Physics},
	Month = jun,
	Pages = {1069-1078},
	Primaryclass = {gr-qc},
	Title = {{DECIGO/BBO as a Probe to Constrain Alternative Theories of Gravity}},
	Volume = 123,
	Year = 2010}

@article{Cutler:2009,
	Author = {Cutler, Curt and Holz, Daniel E.},
	Date-Added = {2012-02-21 04:42:19 -0800},
	Date-Modified = {2012-02-21 04:42:34 -0800},
	Doi = {10.1103/PhysRevD.80.104009},
	Issue = {10},
	Journal = {Phys. Rev. D},
	Month = {Nov},
	Numpages = {15},
	Pages = {104009},
	Publisher = {American Physical Society},
	Title = {Ultrahigh precision cosmology from gravitational waves},
	Url = {http://link.aps.org/doi/10.1103/PhysRevD.80.104009},
	Volume = {80},
	Year = {2009},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.80.104009},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.80.104009}}

@article{ELO,
	Abstract = {In this paper the authors will give an overview of the epitaxial lift-off (ELO) technique and its applications. This first part will describe the basic technology, which includes chemical lift-off, handling bonding, stress, alignment, etc. The second part will give an overview of device results obtained with ELO (LED and lasers on Si, MESFETs on InP, OEICs etc).},
	Author = {P Demeester and I Pollentier and P De Dobbelaere and C Brys and P Van Daele},
	Date-Added = {2012-02-21 01:51:42 -0800},
	Date-Modified = {2012-02-21 01:51:52 -0800},
	Journal = {Semiconductor Science and Technology},
	Number = {6},
	Pages = {1124},
	Title = {Epitaxial lift-off and its applications},
	Url = {http://stacks.iop.org/0268-1242/8/i=6/a=021},
	Volume = {8},
	Year = {1993},
	Bdsk-Url-1 = {http://stacks.iop.org/0268-1242/8/i=6/a=021}}

@misc{Aso:Seismic,
	Author = {Yoichi Aso and Akito Araya},
	Date-Added = {2012-02-20 23:16:11 -0800},
	Date-Modified = {2012-02-20 23:17:48 -0800},
	Howpublished = {personal communication},
	Month = {January},
	Title = {Kamioka seismic data},
	Year = {2012}}

@article{LIGO:SGWB2009,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2009Natur.460..990A},
	Archiveprefix = {arXiv},
	Author = {{Abbott}, B.~P. and {Abbott}, R. and {Acernese}, F. and {Adhikari}, R. and {Ajith}, P. and {Allen}, B. and {Allen}, G. and {Alshourbagy}, M. and {Amin}, R.~S. and {Anderson}, S.~B. and et al.},
	Date-Added = {2012-02-20 15:57:26 -0800},
	Date-Modified = {2012-02-20 15:58:04 -0800},
	Doi = {10.1038/nature08278},
	Eprint = {0910.5772},
	Journal = {Nature},
	Month = aug,
	Pages = {990-994},
	Primaryclass = {astro-ph.CO},
	Title = {{An upper limit on the stochastic gravitational-wave background of cosmological origin}},
	Volume = 460,
	Year = 2009,
	Bdsk-Url-1 = {http://dx.doi.org/10.1038/nature08278}}

@article{AntaresLVC,
	Author = {{The ANTARES Collaboration} and {the LIGO Scientific Collaboration} and {the Virgo Collaboration}},
	Date-Added = {2012-02-20 15:50:31 -0800},
	Date-Modified = {2012-02-20 15:50:31 -0800},
	Journal = {in preparation},
	Note = {(LIGO-P1200006)},
	Title = {A first search for coincident gravitational waves and high energy neutrinos using LIGO, Virgo and Antares Data from 2007},
	Year = {2012}}

@article{GWHENreview,
	Author = {Ando, S. and Baret, B. and Bouhou, B. and Chassande-Motting, E. and Kouchner, A. and Moscoso, L. and Van Elewyck, V. and Bartos, I. and Marka, S. and Marka, Z. and Corsi, A. and Di Palma, I. and Papa, M.A. and Dietz, A. and Donzaud, C. and Eichler, D. and Finley, C. and Guetta, D. and Halzen, F. and Jones, G. and Sutton, P. and Kandhasamy, S. and Mandic, V. and Thrane, E. and Kotake, K. and Piran, T. and Pradier, T. and Romero, G.E. and Waxman, E.},
	Date-Added = {2012-02-20 15:50:17 -0800},
	Date-Modified = {2012-02-20 15:50:17 -0800},
	Journal = {submitted to RMP},
	Note = {(LIGO-P1100194)},
	Title = {Multimessenger astronomy with gravitational waves and high-energy neutrinos},
	Year = {2012}}

@article{Szabi:HEN2011,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2011PhRvL.107y1101B},
	Archiveprefix = {arXiv},
	Author = {{Bartos}, I. and {Finley}, C. and {Corsi}, A. and {M{\'a}rka}, S.},
	Date-Added = {2012-02-20 15:49:26 -0800},
	Date-Modified = {2012-02-20 15:49:46 -0800},
	Doi = {10.1103/PhysRevLett.107.251101},
	Eid = {251101},
	Eprint = {1108.3001},
	Journal = {Physical Review Letters},
	Keywords = {Gravitational radiation, magnetic fields, and other observations, Neutrino, muon, pion, and other elementary particles; cosmic rays, Supernovae, gamma-ray sources; gamma-ray bursts},
	Month = dec,
	Number = 25,
	Pages = {251101},
	Primaryclass = {astro-ph.HE},
	Title = {{Observational Constraints on Multimessenger Sources of Gravitational Waves and High-Energy Neutrinos}},
	Volume = 107,
	Year = 2011,
	Bdsk-Url-1 = {http://dx.doi.org/10.1103/PhysRevLett.107.251101}}

@book{Peebles:Cosmo,
	Author = {Peebles, P. J. E.},
	Date-Added = {2012-02-20 03:29:02 -0800},
	Date-Modified = {2013-01-15 10:11:28 +0000},
	Isbn = {9780691019338},
	Lccn = {92033370},
	Publisher = {Princeton University Press},
	Rating = {5},
	Read = {1},
	Series = {Princeton series in physics},
	Title = {{Principles of Physical Cosmology}},
	Url = {http://books.google.com/books?id=AmlEt6TJ6jAC},
	Year = {1993},
	Bdsk-Url-1 = {http://books.google.com/books?id=AmlEt6TJ6jAC}}

@article{Sathya:LRR,
	Author = {B.S. Sathyaprakash and Bernard F. Schutz},
	Date-Added = {2012-02-20 02:53:09 -0800},
	Date-Modified = {2012-02-20 02:53:18 -0800},
	Journal = {Living Reviews in Relativity},
	Keywords = {Gravitational wave sources, Gravitational wave detectors, Data analysis, Gravitational waves},
	Number = {2},
	Title = {Physics, Astrophysics and Cosmology with Gravitational Waves},
	Url = {http://www.livingreviews.org/lrr-2009-2},
	Volume = {12},
	Year = {2009},
	Bdsk-Url-1 = {http://www.livingreviews.org/lrr-2009-2}}

@article{Sterl:Minimal,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/1991ApJ...380L..17P},
	Author = {{Phinney}, E.~S.},
	Date-Added = {2012-02-20 02:31:20 -0800},
	Date-Modified = {2012-02-20 02:31:52 -0800},
	Doi = {10.1086/186163},
	Journal = {Astrophysical Journal Letters},
	Month = oct,
	Pages = {L17-L21},
	Title = {{The rate of neutron star binary mergers in the universe - Minimal predictions for gravity wave detectors}},
	Volume = 380,
	Year = 1991,
	Bdsk-Url-1 = {http://dx.doi.org/10.1086/186163}}

@article{CuTh2002,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2002gr.qc.....4090C},
	Author = {{Cutler}, C. and {Thorne}, K.~S.},
	Date-Added = {2012-02-20 01:59:38 -0800},
	Date-Modified = {2012-02-20 02:00:07 -0800},
	Eprint = {arXiv:gr-qc/0204090},
	Journal = {ArXiv General Relativity and Quantum Cosmology e-prints},
	Keywords = {General Relativity and Quantum Cosmology, Astrophysics},
	Month = apr,
	Title = {{An Overview of Gravitational-Wave Sources}},
	Year = 2002}

@article{Bruce:1988,
	Author = {Allen, B.},
	Date-Added = {2012-02-20 01:43:18 -0800},
	Date-Modified = {2012-02-20 01:43:33 -0800},
	Doi = {10.1103/PhysRevD.37.2078},
	Issue = {8},
	Journal = {Phys. Rev. D},
	Month = {Apr},
	Pages = {2078--2085},
	Publisher = {American Physical Society},
	Rating = {4},
	Read = {1},
	Title = {Stochastic gravity-wave background in inflationary-universe models},
	Url = {http://link.aps.org/doi/10.1103/PhysRevD.37.2078},
	Volume = {37},
	Year = {1988},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.37.2078},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.37.2078}}

@article{Lada:2006,
	Abstract = {In this Letter I compare recent findings suggesting a low binary star fraction for late-type stars with knowledge concerning the forms of the stellar initial and present-day mass functions for masses down to the hydrogen-burning limit. This comparison indicates that most stellar systems formed in the Galaxy are likely single and not binary, as has been often asserted. Indeed, in the current epoch two-thirds of all main-sequence stellar systems in the Galactic disk are composed of single stars. Some implications of this realization for understanding the star and planet formation process are briefly mentioned.},
	Author = {Charles J. Lada},
	Date-Added = {2012-02-20 01:20:43 -0800},
	Date-Modified = {2012-02-20 01:20:52 -0800},
	Journal = {The Astrophysical Journal Letters},
	Number = {1},
	Pages = {L63},
	Title = {Stellar Multiplicity and the Initial Mass Function: Most Stars Are Single},
	Url = {http://stacks.iop.org/1538-4357/640/i=1/a=L63},
	Volume = {640},
	Year = {2006},
	Bdsk-Url-1 = {http://stacks.iop.org/1538-4357/640/i=1/a=L63}}

@article{Owen:2005,
	Author = {Owen, Benjamin J.},
	Date-Added = {2012-02-20 00:26:13 -0800},
	Date-Modified = {2012-02-20 00:26:24 -0800},
	Doi = {10.1103/PhysRevLett.95.211101},
	Issue = {21},
	Journal = {Phys. Rev. Lett.},
	Month = {Nov},
	Numpages = {4},
	Pages = {211101},
	Publisher = {American Physical Society},
	Title = {Maximum Elastic Deformations of Compact Stars with Exotic Equations of State},
	Url = {http://link.aps.org/doi/10.1103/PhysRevLett.95.211101},
	Volume = {95},
	Year = {2005},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevLett.95.211101},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevLett.95.211101}}

@article{Somiya:2011tb,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2011arXiv1111.7185S},
	Archiveprefix = {arXiv},
	Author = {{Somiya}, K.},
	Date-Added = {2012-02-20 00:15:47 -0800},
	Date-Modified = {2013-01-03 03:36:19 -0800},
	Eprint = {1111.7185},
	Journal = {ArXiv e-prints},
	Keywords = {General Relativity and Quantum Cosmology, Physics - Instrumentation and Detectors},
	Month = nov,
	Primaryclass = {gr-qc},
	Title = {{Detector configuration of LCGT - the Japanese cryogenic gravitational-wave detector}},
	Year = 2011}

@misc{Ken:GEOseismic,
	Author = {Ken A. Strain},
	Date-Added = {2012-02-20 00:04:10 -0800},
	Date-Modified = {2013-01-15 10:12:24 +0000},
	Howpublished = {personal communication},
	Month = {January},
	Rating = {5},
	Year = {2012}}

@article{Ed:MSFF,
	Author = {J. A. Giaime and E. J. Daw and M. Weitz and R. Adhikari and P. Fritschel and R. Abbott and R. Bork and J. Heefner},
	Date-Added = {2012-02-19 22:28:41 -0800},
	Date-Modified = {2012-02-19 22:28:56 -0800},
	Doi = {10.1063/1.1524717},
	Journal = {Review of Scientific Instruments},
	Keywords = {ocean waves; gravitational wave detectors; interferometers; Fabry-Perot resonators; standing wave meters; surface waves (fluid)},
	Number = {1},
	Pages = {218-224},
	Publisher = {AIP},
	Title = {Feedforward reduction of the microseism disturbance in a long-base-line interferometric gravitational-wave detector},
	Url = {http://link.aip.org/link/?RSI/74/218/1},
	Volume = {74},
	Year = {2003},
	Bdsk-Url-1 = {http://link.aip.org/link/?RSI/74/218/1},
	Bdsk-Url-2 = {http://dx.doi.org/10.1063/1.1524717}}

@article{Andri:Surface,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2000PhLA..270..108G},
	Author = {{Gretarsson}, A.~M. and {Harry}, G.~M. and {Penn}, S.~D. and {Saulson}, P.~R. and {Startin}, W.~J. and {Rowan}, S. and {Cagnoli}, G. and {Hough}, J.},
	Date-Added = {2012-02-19 03:30:54 -0800},
	Date-Modified = {2012-02-19 03:31:08 -0800},
	Doi = {10.1016/S0375-9601(00)00295-4},
	Eprint = {arXiv:gr-qc/9912057},
	Journal = {Physics Letters A},
	Month = may,
	Pages = {108-114},
	Title = {{Pendulum mode thermal noise in advanced interferometers: a comparison of fused silica fibers and ribbons in the presence of surface loss}},
	Volume = 270,
	Year = 2000,
	Bdsk-Url-1 = {http://dx.doi.org/10.1016/S0375-9601(00)00295-4}}

@article{Phil:Nonlinear,
	Author = {Cagnoli, G. and Willems, P. A.},
	Date-Added = {2012-02-19 03:11:21 -0800},
	Date-Modified = {2012-02-19 03:11:36 -0800},
	Doi = {10.1103/PhysRevB.65.174111},
	Issue = {17},
	Journal = {Phys. Rev. B},
	Month = {Apr},
	Numpages = {9},
	Pages = {174111},
	Publisher = {American Physical Society},
	Title = {Effects of nonlinear thermoelastic damping in highly stressed fibers},
	Url = {http://link.aps.org/doi/10.1103/PhysRevB.65.174111},
	Volume = {65},
	Year = {2002},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevB.65.174111},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevB.65.174111}}

@article{Vuk:PreBigBang,
	Author = {Mandic, Vuk and Buonanno, Alessandra},
	Date-Added = {2012-02-17 20:52:03 -0800},
	Date-Modified = {2012-02-17 20:52:18 -0800},
	Doi = {10.1103/PhysRevD.73.063008},
	Issue = {6},
	Journal = {Phys. Rev. D},
	Month = {Mar},
	Numpages = {8},
	Pages = {063008},
	Publisher = {American Physical Society},
	Rating = {1},
	Title = {Accessibility of the pre-big-bang models to LIGO},
	Url = {http://link.aps.org/doi/10.1103/PhysRevD.73.063008},
	Volume = {73},
	Year = {2006},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.73.063008},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.73.063008}}

@article{Woodard:HFGW,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2011CQGra..28g5013R},
	Archiveprefix = {arXiv},
	Author = {{Woodard}, R.~P. and {Romania}, M.~G. and {Tsamis}, N.~C.},
	Date-Added = {2012-02-17 20:37:33 -0800},
	Date-Modified = {2012-12-31 01:01:26 -0800},
	Doi = {10.1088/0264-9381/28/7/075013},
	Eprint = {1006.5150},
	Journal = {Classical and Quantum Gravity},
	Month = apr,
	Number = 7,
	Pages = {075013},
	Primaryclass = {gr-qc},
	Rating = {3},
	Title = {{Possible enhancement of high frequency gravitational waves}},
	Volume = 28,
	Year = 2011,
	Bdsk-Url-1 = {http://dx.doi.org/10.1088/0264-9381/28/7/075013}}

@article{Armstrong:LRR,
	Author = {John W. Armstrong},
	Date-Added = {2012-02-15 00:54:24 -0800},
	Date-Modified = {2012-02-15 00:54:51 -0800},
	Journal = {Living Reviews in Relativity},
	Keywords = {Cassini, Doppler stability, Doppler tracking, frequency stability, gravitational wave detectors, radio},
	Number = {1},
	Rating = {4},
	Title = {Low-Frequency Gravitational Wave Searches Using Spacecraft Doppler Tracking},
	Url = {http://www.livingreviews.org/lrr-2006-1},
	Volume = {9},
	Year = {2006},
	Bdsk-Url-1 = {http://www.livingreviews.org/lrr-2006-1}}

@article{SUS:FEA2009,
	Abstract = {Detection of gravitational waves remains one of the most challenging problems faced by experimental physicists. One of the most significant limits to the sensitivity of current, and future, long-baseline interferometric gravitational wave detectors is thermal displacement noise of the test masses and their suspensions. Detector suspension thermal noise will be an important noise source at operating frequencies between approximately 10 and 30 Hz, and results from a combination of thermoelastic damping, surface and bulk losses associated with the suspension fibres. However its effects can be reduced by minimizing the thermoelastic loss and optimization of pendulum dilution factor via appropriate choice of suspension fibre and attachment geometry. This paper will discuss finite element modelling and associated analysis of the loss in quasi-monolithic silica fibre suspensions for future advanced gravitational wave detectors.},
	Author = {A Cumming and A Heptonstall and R Kumar and W Cunningham and C Torrie and M Barton and K A Strain and J Hough and S Rowan},
	Date-Added = {2012-02-15 00:11:39 -0800},
	Date-Modified = {2012-02-15 00:11:51 -0800},
	Journal = {Classical and Quantum Gravity},
	Number = {21},
	Pages = {215012},
	Title = {Finite element modelling of the mechanical loss of silica suspension fibres for advanced gravitational wave detectors},
	Url = {http://stacks.iop.org/0264-9381/26/i=21/a=215012},
	Volume = {26},
	Year = {2009},
	Bdsk-Url-1 = {http://stacks.iop.org/0264-9381/26/i=21/a=215012}}

@article{SUS:2012,
	Abstract = {The detection of gravitational waves remains one of the most challenging prospects faced by experimental physicists. One of the most significant limits to the sensitivity of current, and future, long-baseline interferometric gravitational wave detectors is thermal displacement noise of the test masses and their suspensions. Suspension thermal noise will be an important noise source at operating frequencies between approximately 10 and 30 Hz, and it results from a combination of thermoelastic damping, surface loss and bulk loss associated with the suspension fibres, and weld loss from their attachment. Its effects can be reduced by minimizing thermoelastic loss and optimizing pendulum dilution factor via the appropriate choice of geometry of the suspension fibre and attachment geometry. This paper will discuss the design and fabrication of a prototype of the fused silica suspension stage for use in the advanced LIGO (aLIGO) detector network, analysing in detail the design of the fused silica attachment pieces (ears), together with the suspension assembly techniques. We also present a full thermal noise analysis of the prototype suspension, taking into account for the first time the precise shape of the actual fibres used, and weld loss. We shall demonstrate the suitability of this suspension for installation into aLIGO.},
	Author = {A V Cumming and A S Bell and L Barsotti and M A Barton and G Cagnoli and D Cook and L Cunningham and M Evans and G D Hammond and G M Harry and A Heptonstall and J Hough and R Jones and R Kumar and R Mittleman and N A Robertson and S Rowan and B Shapiro and K A Strain and K Tokmakov and C Torrie and A A van Veggel},
	Date-Added = {2012-02-15 00:10:08 -0800},
	Date-Modified = {2015-03-30 03:51:06 +0000},
	Journal = {Classical and Quantum Gravity},
	Number = {3},
	Pages = {035003},
	Title = {Design and development of the {Advanced LIGO} monolithic fused silica suspension},
	Url = {http://stacks.iop.org/0264-9381/29/i=3/a=035003},
	Volume = {29},
	Year = {2012},
	Bdsk-Url-1 = {http://stacks.iop.org/0264-9381/29/i=3/a=035003}}

@article{SUS:2002,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2002CQGra..19.4043R},
	Author = {{Robertson}, N.~A. and {Cagnoli}, G. and {Crooks}, D.~R.~M. and {Elliffe}, E. and {Faller}, J.~E. and {Fritschel}, P. and {Go{\ss}ler}, S. and {Grant}, A. and {Heptonstall}, A. and {Hough}, J. and {L{\"u}ck}, H. and {Mittleman}, R. and {Perreur-Lloyd}, M. and {Plissi}, M.~V. and {Rowan}, S. and {Shoemaker}, D.~H. and {Sneddon}, P.~H. and {Strain}, K.~A. and {Torrie}, C.~I. and {Ward}, H. and {Willems}, P.},
	Date-Added = {2012-02-15 00:08:16 -0800},
	Date-Modified = {2012-02-15 00:08:33 -0800},
	Doi = {10.1088/0264-9381/19/15/311},
	Journal = {Classical and Quantum Gravity},
	Month = aug,
	Pages = {4043-4058},
	Title = {{Quadruple suspension design for Advanced LIGO}},
	Volume = 19,
	Year = 2002,
	Bdsk-Url-1 = {http://dx.doi.org/10.1088/0264-9381/19/15/311}}

@article{Benno:2008,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2008CQGra..25k4040W},
	Author = {{Willke}, B. and {Danzmann}, K. and {Frede}, M. and {King}, P. and {Kracht}, D. and {Kwee}, P. and {Puncken}, O. and {Savage}, Jr., R.~L. and {Schulz}, B. and {Seifert}, F. and {Veltkamp}, C. and {Wagner}, S. and {We{\ss}els}, P. and {Winkelmann}, L.},
	Date-Added = {2012-02-14 23:35:08 -0800},
	Date-Modified = {2012-02-14 23:35:16 -0800},
	Doi = {10.1088/0264-9381/25/11/114040},
	Journal = {Classical and Quantum Gravity},
	Month = jun,
	Number = 11,
	Pages = {114040},
	Title = {{Stabilized lasers for advanced gravitational wave detectors}},
	Volume = 25,
	Year = 2008,
	Bdsk-Url-1 = {http://dx.doi.org/10.1088/0264-9381/25/11/114040}}

@article{Kwee:09,
	Abstract = {The output power of a cw Nd:YAG laser was stabilized in a dc-coupled feedback loop with a low-noise multiphotodiode detector and an electro-optic amplitude modulator in the frequency band from 1 Hz to 1 kHz. For the first time, to our knowledge, an independently measured relative power noise of2.4{\texttimes}10{\textminus}9 Hz{\textminus}1/2 at 10 Hz was achieved, fulfilling the power stability requirements of the Advanced LIGO (Laser Interferometer Gravitational-Wave Observatory) gravitational wave detector.},
	Author = {Patrick Kwee and Benno Willke and Karsten Danzmann},
	Date-Added = {2012-02-14 23:33:19 -0800},
	Date-Modified = {2012-02-14 23:33:19 -0800},
	Doi = {10.1364/OL.34.002912},
	Journal = {Opt. Lett.},
	Keywords = {Photodetectors; Laser stabilization},
	Month = {Oct},
	Number = {19},
	Pages = {2912--2914},
	Publisher = {OSA},
	Title = {Shot-noise-limited laser power stabilization with a high-power photodiode array},
	Url = {http://ol.osa.org/abstract.cfm?URI=ol-34-19-2912},
	Volume = {34},
	Year = {2009},
	Bdsk-Url-1 = {http://ol.osa.org/abstract.cfm?URI=ol-34-19-2912},
	Bdsk-Url-2 = {http://dx.doi.org/10.1364/OL.34.002912}}

@book{Siegman:Lasers,
	Author = {Siegman, A.E.},
	Date-Added = {2012-02-14 02:05:47 -0800},
	Date-Modified = {2012-04-29 20:59:21 -0700},
	Isbn = {9780935702118},
	Lccn = {81051269},
	Publisher = {University Science Books},
	Rating = {5},
	Read = {1},
	Title = {Lasers},
	Year = {1986},
	Bdsk-Url-1 = {http://books.google.com/books?id=1BZVwUZLTkAC}}

@article{Walsh:99,
	Abstract = {The power spectral density of surface-relief variations on polished optical surfaces across microscopic through to macroscopic spatial scales is calculated from measurements on substrates that are being produced for the Laser Interferometer Gravitational-Wave Observatory (LIGO). These spectra give a guide to the scattering properties of the surface, which in turn critically influence the performance of LIGO. Measurements obtained by use of a full-aperture interferometer and an interference microscope with two different objectives are combined to produce one-dimensional power spectral density representations of the surfaces across spatial frequencies ranging from 0.1 to 8000 cm{\textminus}1. These measurements from different instruments are in good agreement with an analytic power spectrum that varies as $\nu${\textminus}1.5, where $\nu$ is the spatial frequency. Some anomalies in the power spectral density spectra can be related to aspects of the polishing process.},
	Author = {Christopher J. Walsh and Achim J. Leistner and Bozenko F. Oreb},
	Date-Added = {2012-02-14 01:19:59 -0800},
	Date-Modified = {2012-02-14 01:19:59 -0800},
	Doi = {10.1364/AO.38.004790},
	Journal = {Appl. Opt.},
	Keywords = {Roughness; Optical standards and testing; Surface measurements, roughness; Testing ; Polishing; Roughness},
	Month = {Aug},
	Number = {22},
	Pages = {4790--4801},
	Publisher = {OSA},
	Title = {Power Spectral Density Analysis of Optical Substrates for Gravitational-Wave Interferometry},
	Url = {http://ao.osa.org/abstract.cfm?URI=ao-38-22-4790},
	Volume = {38},
	Year = {1999},
	Bdsk-Url-1 = {http://ao.osa.org/abstract.cfm?URI=ao-38-22-4790},
	Bdsk-Url-2 = {http://dx.doi.org/10.1364/AO.38.004790}}

@misc{Hiro,
	Author = {Hiroaki Yamamoto},
	Date-Added = {2012-02-14 00:38:56 -0800},
	Date-Modified = {2012-02-14 00:40:01 -0800},
	Howpublished = {personal communication},
	Year = {2007}}

@article{Callen:1959,
	Author = {Bernard, William and Callen, Herbert B.},
	Date-Added = {2012-02-12 23:28:01 -0800},
	Date-Modified = {2012-02-12 23:43:24 -0800},
	Doi = {10.1103/RevModPhys.31.1017},
	Issue = {4},
	Journal = {Rev. Mod. Phys.},
	Month = {Oct},
	Pages = {1017--1044},
	Publisher = {American Physical Society},
	Rating = {5},
	Title = {Irreversible Thermodynamics of Nonlinear Processes and Noise in Driven Systems},
	Url = {http://link.aps.org/doi/10.1103/RevModPhys.31.1017},
	Volume = {31},
	Year = {1959},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/RevModPhys.31.1017},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/RevModPhys.31.1017}}

@article{Romero:1981,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/1981ZNatA..36..948R},
	Author = {{Romero}, F. and {Dehnen}, H.},
	Date-Added = {2012-02-09 23:15:21 -0800},
	Date-Modified = {2012-02-09 23:15:39 -0800},
	Journal = {Zeitschrift Naturforschung Teil A},
	Keywords = {ASTROPHYSICS, GRAVITATIONAL WAVES, WAVE GENERATION, DIATOMIC MOLECULES, FREE VIBRATION, PIEZOELECTRIC CRYSTALS, RADIATION DISTRIBUTION},
	Month = sep,
	Pages = {948-955},
	Title = {{Generation of gravitational radiation in the laboratory}},
	Volume = 36,
	Year = 1981}

@article{Phillips:1987,
	Abstract = {This review covers a wide range of experimental and theoretical studies of two-level or tunnelling states in glasses. Emphasis is on fundamental physics rather than a detailed comparison of experiment and theory. Sections cover the static and dynamic properties of tunnelling states, their contribution to thermal properties and their response to weak and strong electric and acoustic fields, both steady state and pulsed. A section on metallic glasses focuses on the importance of electron tunnelling-state interactions, and a final section illustrates approaches to a microscopic description by means of selected examples.},
	Author = {W A Phillips},
	Date-Added = {2012-01-29 21:34:13 -0800},
	Date-Modified = {2012-01-29 21:34:26 -0800},
	Journal = {Reports on Progress in Physics},
	Number = {12},
	Pages = {1657},
	Title = {Two-level states in glasses},
	Url = {http://stacks.iop.org/0034-4885/50/i=12/a=003},
	Volume = {50},
	Year = {1987},
	Bdsk-Url-1 = {http://stacks.iop.org/0034-4885/50/i=12/a=003}}

@article{Yuri:PulsarTiming2009,
	Author = {Van Haasteren, Rutger and Levin, Yuri and McDonald, Patrick and Lu, Tingting},
	Date-Added = {2012-01-29 18:12:43 -0800},
	Date-Modified = {2012-01-29 18:12:58 -0800},
	Doi = {10.1111/j.1365-2966.2009.14590.x},
	Issn = {1365-2966},
	Journal = {Monthly Notices of the Royal Astronomical Society},
	Keywords = {gravitational waves, methods: data analysis, pulsars: general},
	Number = {2},
	Pages = {1005--1014},
	Publisher = {Blackwell Publishing Ltd},
	Title = {On measuring the gravitational-wave background using Pulsar Timing Arrays},
	Url = {http://dx.doi.org/10.1111/j.1365-2966.2009.14590.x},
	Volume = {395},
	Year = {2009},
	Bdsk-Url-1 = {http://dx.doi.org/10.1111/j.1365-2966.2009.14590.x}}

@article{Larry:PulsarTiming2009,
	Author = {Anholm, Melissa and Ballmer, Stefan and Creighton, Jolien D. E. and Price, Larry R. and Siemens, Xavier},
	Date-Added = {2012-01-29 18:11:00 -0800},
	Date-Modified = {2012-01-29 18:11:20 -0800},
	Doi = {10.1103/PhysRevD.79.084030},
	Issue = {8},
	Journal = {Phys. Rev. D},
	Month = {Apr},
	Numpages = {19},
	Pages = {084030},
	Publisher = {American Physical Society},
	Title = {Optimal strategies for gravitational wave stochastic background searches in pulsar timing data},
	Url = {http://link.aps.org/doi/10.1103/PhysRevD.79.084030},
	Volume = {79},
	Year = {2009},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.79.084030},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.79.084030}}

@book{Gruyter:1997,
	Author = {Poenaru, D.N. and Greiner, W.},
	Date-Added = {2012-01-24 23:00:19 -0800},
	Date-Modified = {2012-01-24 23:00:50 -0800},
	Isbn = {9783110144673},
	Lccn = {97019524},
	Publisher = {Walter de Gruyter},
	Title = {Experimental techniques in nuclear physics},
	Url = {http://books.google.com/books?id=7yq7ZV2G5D8C},
	Year = {1997},
	Bdsk-Url-1 = {http://books.google.com/books?id=7yq7ZV2G5D8C}}

@article{Ott:SN2009,
	Abstract = {We review the ensemble of anticipated gravitational-wave (GW) emission processes in stellar core collapse and postbounce core-collapse supernova evolution. We discuss recent progress in the modeling of these processes and summarize most recent GW signal estimates. In addition, we present new results on the GW emission from postbounce convective overturn and protoneutron star g -mode pulsations based on axisymmetric radiation-hydrodynamic calculations. Galactic core-collapse supernovae are very rare events, but within 3--5 Mpc from Earth, the rate jumps to 1 in ~2 years. Using the set of currently available theoretical gravitational waveforms, we compute upper-limit optimal signal-to-noise ratios based on current and advanced LIGO/GEO600/VIRGO noise curves for the recent SN 2008bk which exploded at ~3.9 Mpc. While initial LIGOs cannot detect GWs emitted by core-collapse events at such a distance, we find that advanced LIGO-class detectors could put significant upper limits on the GW emission strength for such events. We study the potential occurrence of the various GW emission processes in particular supernova explosion scenarios and argue that the GW signatures of neutrino-driven, magneto-rotational, and acoustically-driven core-collapse SNe may be mutually exclusive. We suggest that even initial LIGOs could distinguish these explosion mechanisms based on the detection (or non-detection) of GWs from a galactic core-collapse supernova.},
	Author = {Christian D Ott},
	Date-Added = {2012-01-24 21:39:45 -0800},
	Date-Modified = {2012-01-24 21:39:59 -0800},
	Journal = {Classical and Quantum Gravity},
	Number = {6},
	Pages = {063001},
	Title = {The gravitational-wave signature of core-collapse supernovae},
	Url = {http://stacks.iop.org/0264-9381/26/i=6/a=063001},
	Volume = {26},
	Year = {2009},
	Bdsk-Url-1 = {http://stacks.iop.org/0264-9381/26/i=6/a=063001}}

@article{EatH:2011,
	Abstract = {We report the discovery of the 20.7 ms binary pulsar J1952+2630, made using the distributed computing project Einstein@Home in Pulsar ALFA survey observations with the Arecibo telescope. Follow-up observations with the Arecibo telescope confirm the binary nature of the system. We obtain a circular orbital solution with an orbital period of 9.4 hr, a projected orbital radius of 2.8 lt-s, and a mass function of f = 0.15 M ☉ by analysis of spin period measurements. No evidence of orbital eccentricity is apparent; we set a 2σ upper limit e ##IMG## [http://ej.iop.org/icons/Entities/lsim.gif] {lsim} 1.7 × 10 --3 . The orbital parameters suggest a massive white dwarf companion with a minimum mass of 0.95 M ☉ , assuming a pulsar mass of 1.4 M ☉ . Most likely, this pulsar belongs to the rare class of intermediate-mass binary pulsars. Future timing observations will aim to determine the parameters of this system further, measure relativistic effects, and elucidate the nature of the companion star.},
	Author = {B. Knispel and P. Lazarus and B. Allen and D. Anderson and C. Aulbert and N. D. R. Bhat and O. Bock and S. Bogdanov and A. Brazier and F. Camilo and S. Chatterjee and J. M. Cordes and F. Crawford and J. S. Deneva and G. Desvignes and H. Fehrmann and P. C. C. Freire and D. Hammer and J. W. T. Hessels and F. A. Jenet and V. M. Kaspi and M. Kramer and J. van Leeuwen and D. R. Lorimer and A. G. Lyne and B. Machenschalk and M. A. McLaughlin and C. Messenger and D. J. Nice and M. A. Papa and H. J. Pletsch and R. Prix and S. M. Ransom and X. Siemens and I. H. Stairs and B. W. Stappers and K. Stovall and A. Venkataraman},
	Date-Added = {2012-01-24 21:28:43 -0800},
	Date-Modified = {2012-01-24 21:29:11 -0800},
	Journal = {The Astrophysical Journal Letters},
	Number = {1},
	Pages = {L1},
	Title = {Arecibo PALFA Survey and Einstein@Home: Binary Pulsar Discovery by Volunteer Computing},
	Url = {http://stacks.iop.org/2041-8205/732/i=1/a=L1},
	Volume = {732},
	Year = {2011},
	Bdsk-Url-1 = {http://stacks.iop.org/2041-8205/732/i=1/a=L1}}

@webpage{EatHweb,
	Author = {{Einstein @ Home}},
	Date-Added = {2012-01-24 21:22:15 -0800},
	Date-Modified = {2012-02-17 20:32:00 -0800},
	Url = {http://einstein.phys.uwm.edu/},
	Year = {2012},
	Bdsk-Url-1 = {http://einstein.phys.uwm.edu/}}

@article{S5:Pulsars,
	Author = {Abbott, B. P. and Abbott, R. and Adhikari, R. and Ajith, P. and Allen, B. and Allen, G. and Amin, R. S. and Anderson, S. B. and Anderson, W. G. and Arain, M. A. and Araya, M. and Armandula, H. and Armor, P. and Aso, Y. and Aston, S. and Aufmuth, P. and Aulbert, C. and Babak, S. and Baker, P. and Ballmer, S. and Bantilan, H. and Barish, B. C. and Barker, C. and Barker, D. and Barr, B. and Barriga, P. and Barsotti, L. and Barton, M. A. and Bartos, I. and Bassiri, R. and Bastarrika, M. and Behnke, B. and Benacquista, M. and Betzwieser, J. and Beyersdorf, P. T. and Bilenko, I. A. and Billingsley, G. and Biswas, R. and Black, E. and Blackburn, J. K. and Blackburn, L. and Blair, D. and Bland, B. and Bodiya, T. P. and Bogue, L. and Bork, R. and Boschi, V. and Bose, S. and Brady, P. R. and Braginsky, V. B. and Brau, J. E. and Brinkmann, M. and Brooks, A. F. and Brown, D. A. and Brunet, G. and Bullington, A. and Buonanno, A. and Burmeister, O. and Byer, R. L. and Cadonati, L. and Cagnoli, G. and Camp, J. B. and Cannizzo, J. and Cannon, K. C. and Cao, J. and Cardenas, L. and Cardoso, V. and Caride, S. and Casebolt, T. and Castaldi, G. and Caudill, S. and Cavagli\`a, M. and Cepeda, C. and Chalkley, E. and Charlton, P. and Chatterji, S. and Chelkowski, S. and Chen, Y. and Christensen, N. and Clark, D. and Clark, J. and Clayton, J. H. and Cokelaer, T. and Conte, R. and Cook, D. and Corbitt, T. R. C. and Cornish, N. and Coyne, D. C. and Creighton, J. D. E. and Creighton, T. D. and Cruise, A. M. and Cumming, A. and Cunningham, L. and Cutler, R. M. and Danzmann, K. and Daudert, B. and Davies, G. and DeBra, D. and Degallaix, J. and Dergachev, V. and Desai, S. and DeSalvo, R. and Dhurandhar, S. and D\'\iaz, M. and Dickson, J. and Dietz, A. and Donovan, F. and Dooley, K. L. and Doomes, E. E. and Drever, R. W. P. and Duke, I. and Dumas, J.-C. and Dwyer, J. and Echols, C. and Edgar, M. and Effler, A. and Ehrens, P. and Ely, G. and Espinoza, E. and Etzel, T. and Evans, M. and Evans, T. and Fairhurst, S. and Faltas, Y. and Fan, Y. and Fazi, D. and Fejer, M. M. and Finn, L. S. and Flasch, K. and Foley, S. and Forrest, C. and Fotopoulos, N. and Franzen, A. and Frei, Z. and Freise, A. and Frey, R. and Fricke, T. T. and Fritschel, P. and Frolov, V. V. and Fyffe, M. and Garofoli, J. A. and Gholami, I. and Giaime, J. A. and Giampanis, S. and Giardina, K. D. and Goda, K. and Goetz, E. and Goggin, L. M. and Gonz\'alez, G. and Gossler, S. and Gouaty, R. and Grant, A. and Gras, S. and Gray, C. and Gray, M. and Greenhalgh, R. J. S. and Gretarsson, A. M. and Grimaldi, F. and Grosso, R. and Grote, H. and Grunewald, S. and Guenther, M. and Gustafson, E. K. and Gustafson, R. and Hage, B. and Hallam, J. M. and Hanna, C. and Hanson, J. and Harms, J. and Harry, G. M. and Harstad, E. D. and Haughian, E. and Hayama, K. and Hayler, T. and Heefner, J. and Heng, I. S. and Heptonstall, A. and Hewitson, M. and Hild, S. and Hirose, E. and Hoak, D. and Holt, K. and Hosken, D. and Hough, J. and Huttner, S. H. and Ingram, D. and Ito, M. and Ivanov, A. and Johnson, B. and Johnson, W. W. and Jones, D. I. and Jones, G. and Jones, R. and Ju, L. and Kalmus, P. and Kalogera, V. and Kamat, S. and Kanner, J. and Kasprzyk, D. and Katsavounidis, E. and Kawabe, K. and Kawamura, S. and Kawazoe, F. and Kells, W. and Keppel, D. G. and Khalaidovski, A. and Khalili, F. Ya. and Khan, R. and Khazanov, E. and King, P. and Kissel, J. S. and Klimenko, S. and Kocsis, B. and Kokeyama, K. and Kondrashov, V. and Kopparapu, R. and Koranda, S. and Kozak, D. and Kozhevatov, I. and Krishnan, B. and Kwee, P. and Landry, M. and Lantz, B. and Lazzarini, A. and Lei, M. and Leonor, I. and Li, C. and Lin, H. and Lindquist, P. E. and Littenberg, T. B. and Lockerbie, N. A. and Lodhia, D. and Lormand, M. and Lu, P. and Lubinski, M. and Lucianetti, A. and L\"uck, H. and Machenschalk, B. and MacInnis, M. and Mageswaran, M. and Mailand, K. and Mandel, I. and Mandic, V. and M\'arka, S. and M\'arka, Z. and Markosyan, A. and Markowitz, J. and Maros, E. and Martin, I. W. and Martin, R. M. and Marx, J. N. and Mason, K. and Matichard, F. and Matone, L. and Matzner, R. and Mavalvala, N. and McCarthy, R. and McClelland, D. E. and McGuire, S. C. and McHugh, M. and McIntyre, G. and McKechan, D. and McKenzie, K. and Mehmet, M. and Melissinos, A. and Mendell, G. and Mercer, R. A. and Meshkov, S. and Messenger, C. J. and Meyers, D. and Miller, A. and Miller, J. and Minelli, J. and Mitra, S. and Mitrofanov, V. P. and Mitselmakher, G. and Mittleman, R. and Miyakawa, O. and Moe, B. and Mohanty, S. D. and Moreno, G. and Mors, K. and Mossavi, K. and MowLowry, C. and Mueller, G. and Muhammad, D. and Mukherjee, S. and Mukhopadhyay, H. and Mullavey, A. and M\"uller-Ebhardt, H. and Munch, J. and Murray, P. G. and Myers, E. and Myers, J. and Nash, T. and Nelson, J. and Newton, G. and Nishizawa, A. and Numata, K. and Ochsner, E. and O'Dell, J. and Ogin, G. and O'Reilly, B. and O'Shaughnessy, R. and Ottaway, D. J. and Ottens, R. S. and Overmier, H. and Owen, B. J. and Pan, Y. and Pankow, C. and Papa, M. A. and Parameshwaraiah, V. and Patel, P. and Pedraza, M. and Penn, S. and Perraca, A. and Petrie, T. and Pinto, I. M. and Pitkin, M. and Pletsch, H. J. and Plissi, M. V. and Postiglione, F. and Principe, M. and Prix, R. and Quetschke, V. and Raab, F. J. and Rabeling, D. S. and Radkins, H. and Raffai, P. and Rainer, N. and Rakhmanov, M. and Ramsunder, M. and Reed, T. and Rehbein, H. and Reid, S. and Reitze, D. H. and Riesen, R. and Riles, K. and Rivera, B. and Robertson, N. A. and Robinson, C. and Robinson, E. L. and Roddy, S. and Rogan, A. M. and Rollins, J. and Romano, J. D. and Romie, J. H. and Rowan, S. and R\"udiger, A. and Ruet, L. and Russell, P. and Ryan, K. and Sakata, S. and Sancho de la Jordana, L. and Sandberg, V. and Sannibale, V. and Santamaria, L. and Saraf, S. and Sarin, P. and Sathyaprakash, B. S. and Sato, S. and Saulson, P. R. and Savage, R. and Savov, P. and Scanlan, M. and Schediwy, S. W. and Schilling, R. and Schnabel, R. and Schofield, R. and Schutz, B. F. and Schwinberg, P. and Scott, J. and Scott, S. M. and Searle, A. C. and Sears, B. and Seifert, F. and Sellers, D. and Sengupta, A. S. and Sergeev, A. and Shapiro, B. and Shawhan, P. and Shoemaker, D. H. and Sibley, A. and Siemens, X. and Sigg, D. and Sinha, S. and Sintes, A. M. and Slagmolen, B. J. J. and Slutsky, J. and Smith, J. R. and Smith, M. R. and Smith, N. D. and Somiya, K. and Sorazu, B. and Stein, L. C. and Strain, K. A. and Stuver, A. and Summerscales, T. Z. and Sun, K.-X. and Sung, M. and Sutton, P. J. and Takahashi, H. and Tanner, D. B. and Taylor, R. and Taylor, R. and Thacker, J. and Thorne, K. A. and Thorne, K. S. and Th\"uring, A. and Tokmakov, K. V. and Torres, C. and Torrie, C. and Traylor, G. and Trias, M. and Ugolini, D. and Urbanek, K. and Vahlbruch, H. and Van Den Broeck, C. and van der Sluys, M. V. and van Veggel, A. A. and Vass, S. and Vaulin, R. and Vecchio, A. and Veitch, J. D. and Veitch, P. and Villar, A. and Vorvick, C. and Vyachanin, S. P. and Waldman, S. J. and Wallace, L. and Ward, H. and Ward, R. L. and Weinert, M. and Weinstein, A. J. and Weiss, R. and Wen, L. and Wen, S. and Wette, K. and Whelan, J. T. and Whitcomb, S. E. and Whiting, B. F. and Wilkinson, C. and Willems, P. A. and Williams, H. R. and Williams, L. and Willke, B. and Wilmut, I. and Winkler, W. and Wipf, C. C. and Wiseman, A. G. and Woan, G. and Wooley, R. and Worden, J. and Wu, W. and Yakushin, I. and Yamamoto, H. and Yan, Z. and Yoshida, S. and Zanolin, M. and Zhang, J. and Zhang, L. and Zhao, C. and Zotov, N. and Zucker, M. E. and zur M\"uhlen, H. and Zweizig, J.},
	Date-Added = {2012-01-24 21:16:45 -0800},
	Date-Modified = {2012-02-17 22:04:45 -0800},
	Doi = {10.1103/PhysRevLett.102.111102},
	Issue = {11},
	Journal = {Phys. Rev. Lett.},
	Month = {Mar},
	Numpages = {6},
	Pages = {111102},
	Publisher = {American Physical Society},
	Title = {All-Sky LIGO Search for Periodic Gravitational Waves in the Early Fifth-Science-Run Data},
	Volume = {102},
	Year = {2009},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevLett.102.111102},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevLett.102.111102}}

@article{Miller:ESD,
	Author = {John Miller and Matthew Evans and Lisa Barsotti and Peter Fritschel and Myron MacInnis and Richard Mittleman and Brett Shapiro and Jonathan Soto and Calum Torrie},
	Date-Added = {2012-01-24 14:20:17 -0800},
	Date-Modified = {2012-01-24 14:20:32 -0800},
	Doi = {10.1016/j.physleta.2010.12.032},
	Issn = {0375-9601},
	Journal = {Physics Letters A},
	Keywords = {Electrostatic drive},
	Number = {3},
	Pages = {788 - 794},
	Title = {Damping parametric instabilities in future gravitational wave detectors by means of electrostatic actuators},
	Url = {http://www.sciencedirect.com/science/article/pii/S0375960110015719},
	Volume = {375},
	Year = {2011},
	Bdsk-Url-1 = {http://www.sciencedirect.com/science/article/pii/S0375960110015719},
	Bdsk-Url-2 = {http://dx.doi.org/10.1016/j.physleta.2010.12.032}}

@article{Blair:PIStrategy,
	Abstract = {Parametric instabilities have been predicted to occur in all advanced high optical power gravitational wave detectors. In this paper we review the problem of parametric instabilities, summarize the latest findings and assess various schemes proposed for their control. We show that non-resonant passive damping of test masses reduces parametric instability but has a noise penalty, and fails to suppress the Q -factor of many modes. Resonant passive damping is shown to have significant advantages but requires detailed modeling. An optical feedback mode suppression interferometer is proposed which is capable of suppressing all instabilities but requires experimental development.},
	Author = {L Ju and D G Blair and C Zhao and S Gras and Z Zhang and P Barriga and H Miao and Y Fan and L Merrill},
	Date-Added = {2012-01-24 14:18:07 -0800},
	Date-Modified = {2012-01-24 14:18:25 -0800},
	Journal = {Classical and Quantum Gravity},
	Number = {1},
	Pages = {015002},
	Title = {Strategies for the control of parametric instability in advanced gravitational wave detectors},
	Url = {http://stacks.iop.org/0264-9381/26/i=1/a=015002},
	Volume = {26},
	Year = {2009},
	Bdsk-Url-1 = {http://stacks.iop.org/0264-9381/26/i=1/a=015002}}

@article{Gras:PI2009,
	Abstract = {The next generation of laser interferometer gravitational wave detectors requires optical cavities with stored power approaching 1 MW. However, such proposed cavities are subject to parametric instability where carrier power resonantly downconverts to drive a large number of test mass acoustic resonances. Damping rings on the test mass circumference have been proposed as a means of suppressing such instabilities, and in previous work, the affect of such a ring on test mass acoustic modes and thermal noise was analysed. The purpose of this paper is to investigate the general issue of parametric instability suppression with damping rings. We determine the optimal position and geometry of damping rings, so as to obtain sufficient instability suppression with the least thermal noise penalty. It is shown that unilateral stability can be attained with a ring damper alone at the expense of a 20% increase in thermal noise, while if just one optical mode is suppressed, there is only a 5% noise penalty.},
	Author = {S Gras and D G Blair and C Zhao},
	Date-Added = {2012-01-24 14:16:16 -0800},
	Date-Modified = {2012-01-24 14:16:30 -0800},
	Journal = {Classical and Quantum Gravity},
	Number = {13},
	Pages = {135012},
	Title = {Suppression of parametric instabilities in future gravitational wave detectors using damping rings},
	Url = {http://stacks.iop.org/0264-9381/26/i=13/a=135012},
	Volume = {26},
	Year = {2009},
	Bdsk-Url-1 = {http://stacks.iop.org/0264-9381/26/i=13/a=135012}}

@article{Matt:PI,
	Author = {M. Evans and L. Barsotti and P. Fritschel},
	Date-Added = {2012-01-24 14:12:47 -0800},
	Date-Modified = {2012-02-17 22:03:38 -0800},
	Doi = {10.1016/j.physleta.2009.11.023},
	Issn = {0375-9601},
	Journal = {Physics Letters A},
	Number = {4},
	Pages = {665 - 671},
	Title = {A general approach to optomechanical parametric instabilities},
	Volume = {374},
	Year = {2010},
	Bdsk-Url-1 = {http://www.sciencedirect.com/science/article/pii/S0375960109014558},
	Bdsk-Url-2 = {http://dx.doi.org/10.1016/j.physleta.2009.11.023}}

@article{Nergis:PI2005,
	Author = {Corbitt, Thomas and Ottaway, David and Innerhofer, Edith and Pelc, Jason and Mavalvala, Nergis},
	Date-Added = {2012-01-24 14:11:08 -0800},
	Date-Modified = {2012-01-24 14:11:23 -0800},
	Doi = {10.1103/PhysRevA.74.021802},
	Issue = {2},
	Journal = {Phys. Rev. A},
	Month = {Aug},
	Numpages = {4},
	Pages = {021802},
	Publisher = {American Physical Society},
	Title = {Measurement of radiation-pressure-induced optomechanical dynamics in a suspended Fabry-Perot cavity},
	Url = {http://link.aps.org/doi/10.1103/PhysRevA.74.021802},
	Volume = {74},
	Year = {2006},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevA.74.021802},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevA.74.021802}}

@article{Vahala:PRL2005,
	Author = {Kippenberg, T. J. and Rokhsari, H. and Carmon, T. and Scherer, A. and Vahala, K. J.},
	Date-Added = {2012-01-24 14:09:31 -0800},
	Date-Modified = {2012-01-24 14:09:47 -0800},
	Doi = {10.1103/PhysRevLett.95.033901},
	Issue = {3},
	Journal = {Phys. Rev. Lett.},
	Month = {Jul},
	Numpages = {4},
	Pages = {033901},
	Publisher = {American Physical Society},
	Title = {Analysis of Radiation-Pressure Induced Mechanical Oscillation of an Optical Microcavity},
	Url = {http://link.aps.org/doi/10.1103/PhysRevLett.95.033901},
	Volume = {95},
	Year = {2005},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevLett.95.033901},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevLett.95.033901}}

@article{Braginsky:2008ea,
	Author = {Braginsky, V B},
	Date-Added = {2012-01-24 14:06:47 -0800},
	Date-Modified = {2012-01-24 14:06:47 -0800},
	Journal = {Astronomy Letters},
	Month = aug,
	Number = {8},
	Pages = {558--562},
	Title = {{Detection of gravitational waves from astrophysical sources}},
	Volume = {34},
	Year = {2008}}

@article{Sato:DECIGO2009,
	Abstract = {DECi-hertz Interferometer Gravitational wave Observatory (DECIGO) is the planned Japanese space gravitational wave antenna, aiming to detect gravitational waves from astrophysically and cosmologically significant sources mainly between 0.1 Hz and 10 Hz and thus to open a new window for gravitational wave astronomy and for the universe. DECIGO will consist of three drag-free spacecraft, 1000 km apart from each other, whose relative displacements are measured by a differential Fabry-Perot interferometer. We plan to launch DECIGO in middle of 2020s, after sequence of two precursor satellite missions, DECIGO pathfinder and Pre-DECIGO, for technology demonstration required to realize DECIGO and hopefully for detection of gravitational waves from our galaxy or nearby galaxies.},
	Author = {Shuichi Sato and Seiji Kawamura and Masaki Ando and Takashi Nakamura and Kimio Tsubono and Akito Araya and Ikkoh Funaki and Kunihito Ioka and Nobuyuki Kanda and Shigenori Moriwaki and Mitsuru Musha and Kazuhiro Nakazawa and Kenji Numata and Shin-ichiro Sakai and Naoki Seto and Takeshi Takashima and Takahiro Tanaka and Kazuhiro Agatsuma and Koh-suke Aoyanagi and Koji Arai and Hideki Asada and Yoichi Aso and Takeshi Chiba and Toshikazu Ebisuzaki and Yumiko Ejiri and Motohiro Enoki and Yoshiharu Eriguchi and Masa-Katsu Fujimoto and Ryuichi Fujita and Mitsuhiro Fukushima and Toshifumi Futamase and Katsuhiko Ganzu and Tomohiro Harada and Tatsuaki Hashimoto and Kazuhiro Hayama and Wataru Hikida and Yoshiaki Himemoto and Hisashi Hirabayashi and Takashi Hiramatsu and Feng-Lei Hong and Hideyuki Horisawa and Mizuhiko Hosokawa and Kiyotomo Ichiki and Takeshi Ikegami and Kaiki T Inoue and Koji Ishidoshiro and Hideki Ishihara and Takehiko Ishikawa and Hideharu Ishizaki and Hiroyuki Ito and Yousuke Itoh and Nobuki Kawashima and Fumiko Kawazoe and Naoko Kishimoto and Kenta Kiuchi and Shiho Kobayashi and Kazunori Kohri and Hiroyuki Koizumi and Yasufumi Kojima and Keiko Kokeyama and Wataru Kokuyama and Kei Kotake and Yoshihide Kozai and Hideaki Kudoh and Hiroo Kunimori and Hitoshi Kuninaka and Kazuaki Kuroda and Kei-ichi Maeda and Hideo Matsuhara and Yasushi Mino and Osamu Miyakawa and Shinji Miyoki and Mutsuko Y Morimoto and Tomoko Morioka and Toshiyuki Morisawa and Shinji Mukohyama and Shigeo Nagano and Isao Naito and Kouji Nakamura and Hiroyuki Nakano and Kenichi Nakao and Shinichi Nakasuka and Yoshinori Nakayama and Erina Nishida and Kazutaka Nishiyama and Atsushi Nishizawa and Yoshito Niwa and Taiga Noumi and Yoshiyuki Obuchi and Masatake Ohashi and Naoko Ohishi and Masashi Ohkawa and Norio Okada and Kouji Onozato and Kenichi Oohara and Norichika Sago and Motoyuki Saijo and Masaaki Sakagami and Shihori Sakata and Misao Sasaki and Takashi Sato and Masaru Shibata and Hisaaki Shinkai and Kentaro Somiya and Hajime Sotani and Naoshi Sugiyama and Yudai Suwa and Rieko Suzuki and Hideyuki Tagoshi and Fuminobu Takahashi and Kakeru Takahashi and Keitaro Takahashi and Ryutaro Takahashi and Ryuichi Takahashi and Tadayuki Takahashi and Hirotaka Takahashi and Takamori Akiteru and Tadashi Takano and Keisuke Taniguchi and Atsushi Taruya and Hiroyuki Tashiro and Yasuo Torii and Morio Toyoshima and Shinji Tsujikawa and Yoshiki Tsunesada and Akitoshi Ueda and Ken-ichi Ueda and Masayoshi Utashima and Yaka Wakabayashi and Hiroshi Yamakawa and Kazuhiro Yamamoto and Toshitaka Yamazaki and Jun'ichi Yokoyama and Chul-Moon Yoo and Shijun Yoshida and Taizoh Yoshino},
	Date-Added = {2012-01-22 20:43:06 -0800},
	Date-Modified = {2012-01-22 20:43:22 -0800},
	Journal = {Journal of Physics: Conference Series},
	Number = {1},
	Pages = {012040},
	Title = {DECIGO: The Japanese space gravitational wave antenna},
	Url = {http://stacks.iop.org/1742-6596/154/i=1/a=012040},
	Volume = {154},
	Year = {2009},
	Bdsk-Url-1 = {http://stacks.iop.org/1742-6596/154/i=1/a=012040}}

@electronic{LCGT:web,
	Author = {KAGRA},
	Date-Added = {2012-01-17 01:50:27 -0800},
	Date-Modified = {2013-01-21 10:11:48 +0000},
	Title = {{KAGRA} Home Page},
	Url = {http://gwcenter.icrr.u-tokyo.ac.jp/en/},
	Year = {2011},
	Bdsk-Url-1 = {http://www.icrr.u-tokyo.ac.jp/gr/LCGT.html},
	Bdsk-Url-2 = {http://gwcenter.icrr.u-tokyo.ac.jp/en/}}

@article{Gregg:aLIGO2010,
	Abstract = {The Advanced LIGO gravitational wave detectors are next generation instruments which will replace the existing initial LIGO detectors. They are currently being constructed and installed. Advanced LIGO strain sensitivity is designed to be about a factor 10 better than initial LIGO over a broad band and usable to 10 Hz, in contrast to 40 Hz for initial LIGO. This is expected to allow for detections and significant astrophysics in most categories of gravitational waves. To achieve this sensitivity, all hardware subsystems are being replaced with improvements. Designs and expected performance are presented for the seismic isolation, suspensions, optics and laser subsystems. Possible enhancements to Advanced LIGO, either to resolve problems that may arise and/or to allow for improved performance, are now being researched. Some of these enhancements are discussed along with some potential technology being considered for detectors beyond Advanced LIGO.},
	Author = {Gregory M Harry},
	Date-Added = {2012-01-17 01:00:41 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Classical and Quantum Gravity},
	Number = {8},
	Pages = {084006},
	Rating = {1},
	Read = {1},
	Title = {Advanced LIGO: the next generation of gravitational wave detectors},
	Volume = {27},
	Year = {2010},
	Bdsk-Url-1 = {http://stacks.iop.org/0264-9381/27/i=8/a=084006}}

@article{Granata:2010,
	Abstract = {Advanced Virgo is the project to upgrade the interferometric gravitational wave detector Virgo, and it foresees the implementation of power and signal non-degenerate recycling cavities. Such cavities suppress the build-up of high order modes of the resonating sidebands, with some advantage for the commissioning of the detector and the build-up of the gravitational signal. Here we present the baseline design of the Advanced Virgo non-degenerate recycling cavities, giving some preliminay results of simulations about the tolerances of this design to astigmatism, mirror figure errors and thermal lensing.},
	Author = {M Granata and M Barsuglia and R Flaminio and A Freise and S Hild and J Marque},
	Date-Added = {2012-01-16 21:58:16 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {