text:
Journal of Physics: Conference Series},
	Number = {1},
	Pages = {012016},
	Title = {Design of the Advanced Virgo non-degenerate recycling cavities},
	Volume = {228},
	Year = {2010},
	Bdsk-Url-1 = {http://stacks.iop.org/1742-6596/228/i=1/a=012016}}

@article{Accadia:2011jh,
	Author = {Accadia, T and Acernese, F and Antonucci, F and Astone, P and Ballardin, G and Barone, F and Barsuglia, M and Bauer, Th S and Beker, M G and Belletoile, A and Birindelli, S and Bitossi, M and Bizouard, M A and Blom, M and Boccara, C and Bondu, F and Bonelli, L and Bonnand, R and Boschi, V and Bosi, L and Bouhou, B and Braccini, S and Bradaschia, C and Brillet, A and Brisson, V and Budzynski, R and Bulik, T and Bulten, H J and Buskulic, D and Buy, C and Cagnoli, G and Calloni, E and Campagna, E and Canuel, B and Carbognani, F and Cavalier, F and Cavalieri, R and Cella, G and Cesarini, E and Chassande-Mottin, E and Chincarini, A and Cleva, F and Coccia, E and Colacino, C N and Colas, J and Colla, A and Colombini, M and Corsi, A and Coulon, J P and Cuoco, E and D'Antonio, S and Dattilo, V and Davier, M and Day, R and De Rosa, R and Debreczeni, G and del Prete, M and Di Fiore, L and Di Lieto, A and Di Paolo Emilio, M and Di Virgilio, A and Dietz, A and Drago, M and Fafone, V and Ferrante, I and Fidecaro, F and Fiori, I and Flaminio, R and Fournier, J D and Franc, J and Frasca, S and Frasconi, F and Freise, A and Galimberti, M and Gammaitoni, L and Garufi, F and G{\'a}sp{\'a}r, M E and Gemme, G and Genin, E and Gennai, A and Giazotto, A and Gouaty, R and Granata, M and Greverie, C and Guidi, G M and Hayau, J F and Heitmann, H and Hello, P and Hild, S and Huet, D and Jaranowski, P and Kowalska, I and Krolak, A and Leroy, N and Letendre, N and Li, T G F and Lorenzini, M and Loriette, V and Losurdo, G and Majorana, E and Maksimovic, I and Man, N and Mantovani, M and Marchesoni, F and Marion, F and Marque, J and Martelli, F and Masserot, A and Michel, C and Milano, L and Minenkov, Y and Mohan, M and Moreau, J and Morgado, N and Morgia, A and Mosca, S and Moscatelli, V and Mours, B and Neri, I and Nocera, F and Pagliaroli, G and Palladino, L and Palomba, C and Paoletti, F and Pardi, S and Parisi, M and Pasqualetti, A and Passaquieti, R and Passuello, D and Persichetti, G and Pichot, M and Piergiovanni, F and Pietka, M and Pinard, L and Poggiani, R and Prato, M and Prodi, G A and Punturo, M and Puppo, P and Rabeling, D S and R{\'a}cz, I and Rapagnani, P and Re, V and Regimbau, T and Ricci, F and Robinet, F and Rocchi, A and Rolland, L and Romano, R and Rosinska, D and Ruggi, P and Sassolas, B and Sentenac, D and Sperandio, L and Sturani, R and Swinkels, B and Toncelli, A and Tonelli, M and Torre, O and Tournefier, E and Travasso, F and Vajente, G and J van den Brand, J F and van der Putten, S and Vasuth, M and Vavoulidis, M and Vedovato, G and Verkindt, D and Vetrano, F and Vicer{\'e}, A and Vinet, J Y and Vocca, H and Was, M and Yvert, M},
	Date-Added = {2012-01-16 21:44:15 -0800},
	Date-Modified = {2012-01-16 21:44:15 -0800},
	Journal = {Low Frequency Noise, Vibration and Active Control},
	Month = jun,
	Number = {1},
	Pages = {63--79},
	Title = {{The seismic Superattenuators of the Virgo gravitational waves interferometer}},
	Volume = {30},
	Year = {2011}}

@webpage{aVirgo:web,
	Author = {Virgo Collaboration},
	Date-Added = {2012-01-16 21:38:30 -0800},
	Date-Modified = {2014-01-23 08:50:11 +0000},
	Rating = {2},
	Url = {https://wwwcascina.virgo.infn.it/advirgo/},
	Year = {2011},
	Bdsk-Url-1 = {https://wwwcascina.virgo.infn.it/advirgo/}}

@article{Braginsky:2006ip,
	Author = {Braginsky, V B and Ryazhskaya, O G and Vyatchanin, S P},
	Date-Added = {2012-01-16 21:27:04 -0800},
	Date-Modified = {2012-01-16 21:27:04 -0800},
	Journal = {Physics Letters A},
	Month = nov,
	Number = {2},
	Pages = {86--89},
	Title = {{Limitations in quantum measurements resolution created by cosmic rays}},
	Volume = {359},
	Year = {2006}}

@article{Kazuhiro:Cosmic,
	Author = {Yamamoto, Kazuhiro and Hayakawa, Hideaki and Okada, Atsushi and Uchiyama, Takashi and Miyoki, Shinji and Ohashi, Masatake and Kuroda, Kazuaki and Kanda, Nobuyuki and Tatsumi, Daisuke and Tsunesada, Yoshiki},
	Date-Added = {2012-01-16 21:19:18 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issue = {2},
	Journal = {Phys. Rev. D},
	Month = {Jul},
	Numpages = {12},
	Pages = {022004},
	Publisher = {American Physical Society},
	Title = {Effect of energy deposited by cosmic-ray particles on interferometric gravitational wave detectors},
	Volume = {78},
	Year = {2008},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.78.022004},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.78.022004}}

@article{Penn:2004,
	Abstract = {We present the results of quality factor measurements for rod samples made of fused silica. To decrease the dissipation, we annealed our samples. The highest quality factor that we observed was Q = (2.03 $\pm$ 0.01) × 10 8 for a mode at 384 Hz. This is the highest published value of Q in fused silica measured to date.},
	Author = {Alexandr Ageev and Belkis Cabrera Palmer and Antonio De Felice and Steven D Penn and Peter R Saulson},
	Date-Added = {2012-01-16 16:53:47 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Classical and Quantum Gravity},
	Number = {16},
	Pages = {3887},
	Title = {Very high quality factor measured in annealed fused silica},
	Volume = {21},
	Year = {2004},
	Bdsk-Url-1 = {http://stacks.iop.org/0264-9381/21/i=16/a=004}}

@article{cole:261108,
	Author = {Garrett D. Cole and Simon Groblacher and Katharina Gugler and Sylvain Gigan and Markus Aspelmeyer},
	Date-Added = {2012-01-16 14:06:56 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Eid = {261108},
	Journal = {Applied Physics Letters},
	Keywords = {distributed Bragg reflectors; micromechanical resonators},
	Number = {26},
	Numpages = {3},
	Pages = {261108},
	Publisher = {AIP},
	Title = {Monocrystalline Al[sub x]Ga[sub 1 - x]As heterostructures for high-reflectivity high-Q micromechanical resonators in the megahertz regime},
	Volume = {92},
	Year = {2008},
	Bdsk-Url-1 = {http://link.aip.org/link/?APL/92/261108/1},
	Bdsk-Url-2 = {http://dx.doi.org/10.1063/1.2952512}}

@misc{Cheryl:Picture,
	Author = {Cheryl Vorvick},
	Date-Added = {2012-01-16 14:00:54 -0800},
	Date-Modified = {2013-06-08 08:57:38 +0000},
	Howpublished = {personal communication},
	Year = {2012}}

@article{JM:Mesa2008,
	Abstract = {Thermal effects are already important in currently operating interferometric gravitational wave detectors. Planned upgrades of these detectors involve increasing optical power to combat quantum shot noise. We consider the ramifications of this increased power for one particular class of laser beams---wide, flat-topped, mesa beams. In particular we model a single mesa beam Fabry--Perot cavity having thermoelastically deformed mirrors. We calculate the intensity profile of the fundamental cavity eigenmode in the presence of thermal perturbations, and the associated changes in thermal noise. We also outline an idealized method of correcting for such effects. At each stage we contrast our results with those of a comparable Gaussian beam cavity. Although we focus on mesa beams the techniques described are applicable to any azimuthally symmetric system.},
	Author = {J Miller and P Willems and H Yamamoto and J Agresti and R DeSalvo},
	Date-Added = {2012-01-16 13:55:56 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Classical and Quantum Gravity},
	Number = {23},
	Pages = {235016},
	Title = {Thermal distortions of non-Gaussian beams in Fabry--Perot cavities},
	Volume = {25},
	Year = {2008},
	Bdsk-Url-1 = {http://stacks.iop.org/0264-9381/25/i=23/a=235016}}

@article{JM:Mesa2007,
	Abstract = {We have tested a new kind of Fabry-Perot long-baseline optical resonator proposed to reduce the thermal noise sensitivity of gravitational wave interferometric detectors--the "mesa beam" cavity--whose flat top beam shape is achieved by means of an aspherical end mirror. We present the fundamental mode intensity pattern for this cavity and its distortion due to surface imperfections and tilt misalignments, and contrast the higher order mode patterns to the Gauss-Laguerre modes of a spherical mirror cavity. We discuss the effects of mirror tilts on cavity alignment and locking and present measurements of the mesa beam tilt sensitivity.},
	Author = {Marco G. Tarallo and John Miller and J. Agresti and E. D'Ambrosio and R. DeSalvo and D. Forest and B. Lagrange and J. M. Mackowsky and C. Michel and J. L. Montorio and N. Morgado and L. Pinard and A. Remilleux and B. Simoni and P. Willems},
	Date-Added = {2012-01-16 13:54:14 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Appl. Opt.},
	Keywords = {Fabry-Perot; Optical resonators; Detectors},
	Month = {Sep},
	Number = {26},
	Pages = {6648--6654},
	Publisher = {OSA},
	Title = {Generation of a flat-top laser beam for gravitational wave detectors by means of a nonspherical Fabry-Perot resonator},
	Volume = {46},
	Year = {2007},
	Bdsk-Url-1 = {http://ao.osa.org/abstract.cfm?URI=ao-46-26-6648},
	Bdsk-Url-2 = {http://dx.doi.org/10.1364/AO.46.006648}}

@article{Andreas:LG2009,
	Author = {Chelkowski, Simon and Hild, Stefan and Freise, Andreas},
	Date-Added = {2012-01-16 13:48:19 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issue = {12},
	Journal = {Phys. Rev. D},
	Month = {Jun},
	Numpages = {11},
	Pages = {122002},
	Publisher = {American Physical Society},
	Title = {Prospects of higher-order Laguerre-Gauss modes in future gravitational wave detectors},
	Volume = {79},
	Year = {2009},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.79.122002},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.79.122002}}

@article{Ting:LG,
	Author = {Hong, T. and Miller, J. and Yamamoto, H. and Chen, Y. and Adhikari, R.},
	Date-Added = {2012-01-16 13:21:00 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issue = {10},
	Journal = {Phys. Rev. D},
	Month = {Nov},
	Numpages = {10},
	Pages = {102001},
	Publisher = {American Physical Society},
	Rating = {5},
	Read = {1},
	Title = {Effects of mirror aberrations on Laguerre-Gaussian beams in interferometric gravitational-wave detectors},
	Volume = {84},
	Year = {2011},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.84.102001},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.84.102001}}

@article{Vinet:LG,
	Author = {Vinet, Jean-Yves},
	Date-Added = {2012-01-16 13:20:16 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issue = {4},
	Journal = {Phys. Rev. D},
	Month = {Aug},
	Numpages = {9},
	Pages = {042003},
	Publisher = {American Physical Society},
	Title = {Thermal noise in advanced gravitational wave interferometric antennas: A comparison between arbitrary order Hermite and Laguerre Gaussian modes},
	Volume = {82},
	Year = {2010},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.82.042003},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.82.042003}}

@article{Rob:LG,
	Author = {Granata, M. and Buy, C. and Ward, R. and Barsuglia, M.},
	Date-Added = {2012-01-16 13:18:55 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issue = {23},
	Journal = {Phys. Rev. Lett.},
	Month = {Nov},
	Numpages = {4},
	Pages = {231102},
	Publisher = {American Physical Society},
	Title = {Higher-Order Laguerre-Gauss Mode Generation and Interferometry for Gravitational Wave Detectors},
	Volume = {105},
	Year = {2010},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevLett.105.231102},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevLett.105.231102}}

@article{Mesa:Erika,
	Abstract = {By using non-Gaussian, flat-topped beams in the advanced gravitational wave interferometers currently being designed, one can reduce the impact on the interferometer sensitivity of a variety of fundamental disturbances (thermoelastic noise, noise in mirror coatings, thermal lensing, etc). This may make beating the standard quantum limit an achievable goal.},
	Author = {Erika D'Ambrosio and Richard O'Shaugnessy and Kip Thorne and Phil Willems and Sergey Strigin and Sergey Vyatchanin},
	Date-Added = {2012-01-16 13:07:24 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Classical and Quantum Gravity},
	Number = {5},
	Pages = {S867},
	Rating = {2},
	Title = {Advanced LIGO: non-Gaussian beams},
	Volume = {21},
	Year = {2004},
	Bdsk-Url-1 = {http://stacks.iop.org/0264-9381/21/i=5/a=074}}

@webpage{aLIGO:web,
	Author = {LIGO},
	Date-Added = {2012-01-16 12:56:32 -0800},
	Date-Modified = {2012-02-17 22:14:39 -0800},
	Rating = {3},
	Read = {1},
	Url = {https://www.advancedligo.mit.edu/},
	Year = {2011},
	Bdsk-Url-1 = {https://www.advancedligo.mit.edu/}}

@techreport{Kip:Baffles1989,
	Address = {\url{http://www.ligo.caltech.edu/docs/T/T890017-00.pdf}},
	Author = {K.~S.~Thorne},
	Date-Added = {2012-01-16 10:46:05 -0800},
	Date-Modified = {2018-06-22 20:46:14 +0000},
	Institution = {Caltech},
	Rating = {4},
	Read = {1},
	Title = {Light Scattering and Proposed Baffle Configuration for the {LIGO}},
	Type = {{LIGO} Technical Report},
	Year = {1989}}

@article{Vinet:scatter,
	Author = {Vinet, Jean-Yves and Brisson, Violette and Braccini, Stefano and Ferrante, Isidoro and Pinard, Laurent and Bondu, Fran\ifmmode \mbox{\c{c}}\else \c{c}\fi{}ois and Tourni\'e, Eric},
	Date-Added = {2012-01-16 10:26:34 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issue = {10},
	Journal = {Phys. Rev. D},
	Month = {Nov},
	Pages = {6085--6095},
	Publisher = {American Physical Society},
	Title = {Scattered light noise in gravitational wave interferometric detectors: A statistical approach},
	Volume = {56},
	Year = {1997},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.56.6085},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.56.6085}}

@article{Armstrong:2005,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2005RaSc...40.2001A},
	Author = {{Asmar}, S.~W. and {Armstrong}, J.~W. and {Iess}, L. and {Tortora}, P.},
	Date-Added = {2012-01-15 16:58:27 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Eid = {RS2001},
	Journal = {Radio Science},
	Keywords = {Radio Science: Instruments and techniques (1241), Radio Science: Radio wave propagation, Radio Science: Signal processing (0674)},
	Month = mar,
	Pages = {2001},
	Title = {{Spacecraft Doppler tracking: Noise budget and accuracy achievable in precision radio science observations}},
	Volume = 40,
	Year = 2005,
	Bdsk-Url-1 = {http://dx.doi.org/10.1029/2004RS003101}}

@article{Deepto:2003,
	Annote = {10.1038/nature01732},
	Author = {Chakrabarty, Deepto and Morgan, Edward H. and Muno, Michael P. and Galloway, Duncan K. and Wijnands, Rudy and van der Klis, Michiel and Markwardt, Craig B.},
	Date = {2003/07/03/print},
	Date-Added = {2012-01-15 01:38:04 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Day = {03},
	Isbn = {0028-0836},
	Journal = {Nature},
	M3 = {10.1038/nature01732},
	Month = {07},
	Number = {6944},
	Pages = {42--44},
	Title = {Nuclear-powered millisecond pulsars and the maximum spin frequency of neutron stars},
	Ty = {JOUR},
	Volume = {424},
	Year = {2003},
	Bdsk-Url-1 = {http://dx.doi.org/10.1038/nature01732}}

@article{Owen:2006,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2006CQGra..23S...1O},
	Author = {{Owen}, B.~J.},
	Date-Added = {2012-01-15 01:32:11 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Classical and Quantum Gravity},
	Month = apr,
	Pages = {1},
	Title = {{Detectability of periodic gravitational waves by initial interferometers}},
	Volume = 23,
	Year = 2006,
	Bdsk-Url-1 = {http://dx.doi.org/10.1088/0264-9381/23/8/S01}}

@article{Bildsten:1998,
	Abstract = {Recent discoveries by the Rossi X-Ray Timing Explorer indicate that most of the rapidly accreting ( ##IMG## [http://ej.iop.org/icons/Entities/dotM.gif] {dot M} ##IMG## [http://ej.iop.org/icons/Entities/gtrsim.gif] {gtrsim} 10 −11 M ##IMG## [http://ej.iop.org/images/1538-4357/501/1/L89/img3.gif] {_{{\odot}}} yr −1 ) weakly magnetic ( B ##IMG## [http://ej.iop.org/icons/Entities/ll.gif] {ll} 10 11 G) neutron stars in the Galaxy are rotating at spin frequencies ν s ##IMG## [http://ej.iop.org/icons/Entities/gtrsim.gif] {gtrsim} 250 Hz. Remarkably, they all rotate in a narrow range of frequencies (no more than a factor of 2, with many within 20% of 300 Hz). I suggest that these stars rotate fast enough so that, on average, the angular momentum added by accretion is lost to gravitational radiation. The strong ν s -dependence of the angular momentum loss rate from gravitational radiation then provides a natural reason for similar spin frequencies. Provided that the interior temperature has a large-scale asymmetry misaligned from the spin axis, then the temperature-sensitive electron captures in the deep crust can provide the quadrupole needed ( ~10 −7 MR 2 ) to reach this limiting situation at ν s ≈ 300 Hz. This quadrupole is only present during accretion and makes it difficult to form radio pulsars with ν s > (600-800) Hz by accreting at ##IMG## [http://ej.iop.org/icons/Entities/dotM.gif] {dot M} ##IMG## [http://ej.iop.org/icons/Entities/gtrsim.gif] {gtrsim} 10 −10 M ##IMG## [http://ej.iop.org/images/1538-4357/501/1/L89/img3.gif] {_{{\odot}}} yr −1 . The gravity wave strength is h c ~(0.5-1) × 10 −26 from many of these neutron stars and greater than 2 × 10 −26 for Sco X-1. Prior knowledge of the position, spin frequency, and orbital periods will allow for deep searches for these periodic signals with gravitational wave interferometers (LIGO, VIRGO, and the "dual-recycled" GEO 600 detector), and experimenters need to take such sources into account. Sco X-1 will most likely be detected first.},
	Author = {Lars Bildsten},
	Date-Added = {2012-01-15 01:09:26 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {The Astrophysical Journal Letters},
	Number = {1},
	Pages = {L89},
	Title = {Gravitational Radiation and Rotation of Accreting Neutron Stars},
	Volume = {501},
	Year = {1998},
	Bdsk-Url-1 = {http://stacks.iop.org/1538-4357/501/i=1/a=L89}}

@article{Ipser:1971,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/1971ApJ...166..175I},
	Author = {{Ipser}, J.~R.},
	Date-Added = {2012-01-15 01:01:30 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {\apj},
	Month = may,
	Pages = {175},
	Title = {{Gravitational Radiation from Slowly Rotating, Fully Relativistic Stars}},
	Volume = 166,
	Year = 1971,
	Bdsk-Url-1 = {http://dx.doi.org/10.1086/150948}}

@article{Bell:1968,
	Annote = {10.1038/217709a0},
	Author = {Hewish, A. and Bell, S. J. and Pilkington, J. D. H. and Scott, P. F. and Collins, R. A.},
	Date = {1968/02/24/print},
	Date-Added = {2012-01-15 00:47:43 -0800},
	Date-Modified = {2012-02-28 06:41:27 -0800},
	Day = {24},
	Journal = {Nature},
	M3 = {10.1038/217709a0},
	Month = {02},
	Number = {5130},
	Pages = {709--713},
	Rating = {4},
	Title = {Observation of a Rapidly Pulsating Radio Source},
	Ty = {JOUR},
	Volume = {217},
	Year = {1968},
	Bdsk-Url-1 = {http://dx.doi.org/10.1038/217709a0}}

@article{Holger:GRG2011,
	Affiliation = {Department of Physics, University of California, 366 Le Conte Hall, Berkeley, CA 94720-7300, USA},
	Author = {Hohensee, Michael and Lan, Shau-Yu and Houtz, Rachel and Chan, Cheong and Estey, Brian and Kim, Geena and Kuan, Pei-Chen and M{\"u}ller, Holger},
	Date-Added = {2012-01-12 23:03:06 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issn = {0001-7701},
	Issue = {7},
	Journal = {General Relativity and Gravitation},
	Keyword = {Physics and Astronomy},
	Note = {10.1007/s10714-010-1118-x},
	Pages = {1905-1930},
	Publisher = {Springer Netherlands},
	Title = {Sources and technology for an atomic gravitational wave interferometric sensor},
	Volume = {43},
	Year = {2011},
	Bdsk-Url-1 = {http://dx.doi.org/10.1007/s10714-010-1118-x}}

@article{Dim:Atom2008,
	Author = {Dimopoulos, Savas and Graham, Peter W. and Hogan, Jason M. and Kasevich, Mark A. and Rajendran, Surjeet},
	Date-Added = {2012-01-12 23:01:19 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issue = {12},
	Journal = {Phys. Rev. D},
	Month = {Dec},
	Numpages = {35},
	Pages = {122002},
	Publisher = {American Physical Society},
	Title = {Atomic gravitational wave interferometric sensor},
	Volume = {78},
	Year = {2008},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.78.122002},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.78.122002}}

@article{FaPh2003,
	Author = {Farmer, Alison J. and Phinney, E. S.},
	Date-Added = {2012-01-12 22:57:01 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issn = {1365-2966},
	Journal = {Monthly Notices of the Royal Astronomical Society},
	Keywords = {gravitational waves, binaries: close, diffuse radiation},
	Number = {4},
	Pages = {1197--1214},
	Publisher = {Blackwell Science Ltd},
	Title = {The gravitational wave background from cosmological compact binaries},
	Volume = {346},
	Year = {2003},
	Bdsk-Url-1 = {http://dx.doi.org/10.1111/j.1365-2966.2003.07176.x}}

@article{Nukes:1974,
	Author = {Chapline, G. F. and Nuckolls, J. and Wood, L. L.},
	Date-Added = {2012-01-08 15:02:47 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issue = {4},
	Journal = {Phys. Rev. D},
	Month = {Aug},
	Pages = {1064--1065},
	Publisher = {American Physical Society},
	Title = {Gravitational-radiation production using nuclear explosions},
	Volume = {10},
	Year = {1974},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.10.1064},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.10.1064}}

@inproceedings{All1996,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/1997rggr.conf..373A},
	Author = {{Allen}, B.},
	Booktitle = {Relativistic Gravitation and Gravitational Radiation},
	Date-Added = {2012-01-08 14:40:43 -0800},
	Date-Modified = {2012-01-08 14:41:39 -0800},
	Editor = {{J.-A.~Marck \& J.-P.~Lasota}},
	Eprint = {arXiv:gr-qc/9604033},
	Pages = {373},
	Rating = {5},
	Read = {1},
	Title = {{The Stochastic Gravity-Wave Background: Sources and Detection}},
	Year = 1997}

@article{Staro:1979,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/1979ZhPmR..30..719S},
	Author = {{Starobinskii}, A.~A.},
	Date-Added = {2012-01-08 14:20:58 -0800},
	Date-Modified = {2013-01-06 00:36:23 -0800},
	Journal = {JETP Letters},
	Keywords = {ASTRONOMICAL MODELS, ELECTROMAGNETIC SPECTRA, GRAVITATIONAL WAVES, RELIC RADIATION, UNIVERSE, GRAVITATION THEORY, PHENOMENOLOGY, QUANTUM THEORY, RADIATION MEASUREMENT, RELATIVITY},
	Month = dec,
	Pages = {719-723},
	Title = {{Spectrum of relict gravitational radiation and the early state of the universe}},
	Volume = 30,
	Year = 1979}

@article{Giffard:1978,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/1978ARA%26A..16..521T},
	Author = {{Tyson}, J.~A. and {Giffard}, R.~P.},
	Date-Added = {2012-01-08 13:43:10 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Annual Review of Astronomy and Astrophysics},
	Keywords = {ASTRONOMY, GRAVITATIONAL WAVES, STELLAR GRAVITATION, BINARY STARS, EINSTEIN EQUATIONS, FIELD THEORY (PHYSICS), GRAVITATION THEORY, GRAVITATIONAL WAVE ANTENNAS, LINEAR FILTERS, OPTIMIZATION, RADIATION DETECTORS, SIGNAL DETECTION, SPACE-TIME FUNCTIONS, SUPERNOVAE},
	Pages = {521-554},
	Rating = {3},
	Title = {{Gravitational-wave astronomy}},
	Volume = 16,
	Year = 1978,
	Bdsk-Url-1 = {http://dx.doi.org/10.1146/annurev.aa.16.090178.002513}}

@article{TOBA:2011,
	Author = {Ishidoshiro, Koji and Ando, Masaki and Takamori, Akiteru and Takahashi, Hirotaka and Okada, Kenshi and Matsumoto, Nobuyuki and Kokuyama, Wataru and Kanda, Nobuyuki and Aso, Yoichi and Tsubono, Kimio},
	Date-Added = {2012-01-08 04:02:07 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issue = {16},
	Journal = {Phys. Rev. Lett.},
	Month = {Apr},
	Numpages = {4},
	Pages = {161101},
	Publisher = {American Physical Society},
	Title = {Upper Limit on Gravitational Wave Backgrounds at 0.2 Hz with a Torsion-Bar Antenna},
	Volume = {106},
	Year = {2011},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevLett.106.161101},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevLett.106.161101}}

@article{Ando:TOBA,
	Author = {Ando, Masaki and Ishidoshiro, Koji and Yamamoto, Kazuhiro and Yagi, Kent and Kokuyama, Wataru and Tsubono, Kimio and Takamori, Akiteru},
	Date-Added = {2012-01-08 04:00:25 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issue = {16},
	Journal = {Phys. Rev. Lett.},
	Month = {Oct},
	Numpages = {4},
	Pages = {161101},
	Publisher = {American Physical Society},
	Rating = {5},
	Read = {1},
	Title = {Torsion-Bar Antenna for Low-Frequency Gravitational-Wave Observations},
	Volume = {105},
	Year = {2010},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevLett.105.161101},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevLett.105.161101}}

@article{Tyson:1982,
	Author = {Brown, B. L. and Mills, A. P. and Tyson, J. A.},
	Date-Added = {2012-01-08 03:52:20 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issue = {6},
	Journal = {Phys. Rev. D},
	Month = {Sep},
	Pages = {1209--1218},
	Publisher = {American Physical Society},
	Title = {Results of a 440-day search for gravitational radiation},
	Volume = {26},
	Year = {1982},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.26.1209},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.26.1209}}

@article{Jensen:1979,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/1979RvGSP..17.2057J},
	Author = {{Jensen}, O.~G.},
	Date-Added = {2012-01-08 03:45:43 -0800},
	Date-Modified = {2012-01-08 03:45:55 -0800},
	Journal = {Reviews of Geophysics and Space Physics},
	Keywords = {GRAVITATIONAL WAVES, SEISMIC WAVES, SEISMOGRAPHS, WAVE PROPAGATION, EARTH CRUST, EQUATIONS OF MOTION, RELATIVITY, SPACE-TIME FUNCTIONS, TENSOR ANALYSIS},
	Month = nov,
	Pages = {2057-2069},
	Title = {{Seismic detection of gravitational radiation}},
	Volume = 17,
	Year = 1979}

@article{Tyson:Nothing,
	Author = {Douglass, D. H. and Gram, R. Q. and Tyson, J. A. and Lee, R. W.},
	Date-Added = {2012-01-08 03:42:31 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issue = {8},
	Journal = {Phys. Rev. Lett.},
	Month = {Aug},
	Pages = {480--483},
	Publisher = {American Physical Society},
	Title = {Two-Detector-Coincidence Search for Bursts of Gravitational Radiation},
	Volume = {35},
	Year = {1975},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevLett.35.480},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevLett.35.480}}

@article{Weber:GW,
	Author = {Weber, J.},
	Date-Added = {2012-01-08 03:39:26 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issue = {1},
	Journal = {Phys. Rev.},
	Month = {Jan},
	Pages = {306--313},
	Publisher = {American Physical Society},
	Title = {Detection and Generation of Gravitational Waves},
	Volume = {117},
	Year = {1960},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRev.117.306},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRev.117.306}}

@article{Hawking:1971,
	Author = {Hawking, S. W.},
	Date-Added = {2012-01-08 03:38:23 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issue = {21},
	Journal = {Phys. Rev. Lett.},
	Month = {May},
	Pages = {1344--1346},
	Publisher = {American Physical Society},
	Title = {Gravitational Radiation from Colliding Black Holes},
	Volume = {26},
	Year = {1971},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevLett.26.1344},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevLett.26.1344}}

@article{Weber:Bars,
	Author = {Weber, J.},
	Date-Added = {2012-01-08 03:36:19 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issue = {6},
	Journal = {Phys. Rev. Lett.},
	Month = {Feb},
	Pages = {276--279},
	Publisher = {American Physical Society},
	Title = {Gravitational Radiation Experiments},
	Volume = {24},
	Year = {1970},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevLett.24.276},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevLett.24.276}}

@inproceedings{Deepto:2008,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2008AIPC.1068...67C},
	Archiveprefix = {arXiv},
	Author = {{Chakrabarty}, D.},
	Booktitle = {American Institute of Physics Conference Series},
	Date-Added = {2012-01-08 03:16:58 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Editor = {{R.~Wijnands, D.~Altamirano, P.~Soleri, N.~Degenaar, N.~Rea, P.~Casella, A.~Patruno, \& M.~Linares}},
	Eprint = {0809.4031},
	Keywords = {Pulsars, X-ray, Neutron stars},
	Month = oct,
	Pages = {67-74},
	Series = {American Institute of Physics Conference Series},
	Title = {{The spin distribution of millisecond X-ray pulsars}},
	Volume = 1068,
	Year = 2008,
	Bdsk-Url-1 = {http://dx.doi.org/10.1063/1.3031208}}

@article{Cornish:2007,
	Author = {Cornish, Neil J. and Porter, Edward K.},
	Date-Added = {2012-01-07 20:49:34 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issue = {2},
	Journal = {Phys. Rev. D},
	Month = {Jan},
	Numpages = {5},
	Pages = {021301},
	Publisher = {American Physical Society},
	Title = {Catching supermassive black hole binaries without a net},
	Volume = {75},
	Year = {2007},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.75.021301},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.75.021301}}

@article{Hu:AR2002,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2002ARA%26A..40..171H},
	Author = {{Hu}, W. and {Dodelson}, S.},
	Date-Added = {2012-01-07 19:39:58 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Eprint = {arXiv:astro-ph/0110414},
	Journal = {Annual Review of Astronomy and Astrophysics},
	Keywords = {background radiation, cosmology, theory, dark matter, early universe},
	Pages = {171-216},
	Rating = {5},
	Title = {{Cosmic Microwave Background Anisotropies}},
	Volume = 40,
	Year = 2002,
	Bdsk-Url-1 = {http://dx.doi.org/10.1146/annurev.astro.40.060401.093926}}

@webpage{LISA:2009,
	Author = {T.~Prince and the {LISA Science Team}},
	Date-Added = {2012-01-07 19:06:28 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Institution = {Caltech},
	Rating = {4},
	Read = {1},
	Title = {{LISA}: Probing the Universe with Gravitational Waves},
	Year = {2009},
	Bdsk-Url-1 = {http://list.caltech.edu/mission_documents}}

@article{Danzmann:2003,
	Abstract = {The existence of gravitational waves is the most prominent of Einstein's predictions that has not yet been directly verified. The space project LISA shares its goal and principle of operation with the ground-based interferometers currently under construction: the detection and measurement of gravitational waves by laser interferometry. Only in space, detection of signals below, say, 1 Hz is possible. LISA, a joint project of ESA and NASA, is a mission that will measure these low-frequency waves. LISA consists of three spacecraft in heliocentric orbits, forming a triangle with 5 million km sides. Launch for LISA is scheduled for 2011, following a technology demonstrator LTP in 2006.},
	Author = {Karsten Danzmann and Albrecht R{\"u}diger},
	Date-Added = {2012-01-07 18:46:13 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Classical and Quantum Gravity},
	Number = {10},
	Pages = {S1},
	Title = {LISA technology---concept, status, prospects},
	Volume = {20},
	Year = {2003},
	Bdsk-Url-1 = {http://stacks.iop.org/0264-9381/20/i=10/a=301}}

@article{Hirose:10,
	Abstract = {We observed the effect of radiation pressure on the angular sensing and control system of the Laser Interferometer Gravitational-Wave Observatory (LIGO) interferometer's core optics at LIGO Hanford Observatory. This is the first measurement of this effect in a complete gravitational-wave interferometer. Only one of the two angular modes survives with feedback control, because the other mode is suppressed when the control gain is sufficiently large. We developed a mathematical model to understand the physics of the system. This model matches well with the dynamics that we observe.},
	Author = {Eiichi Hirose and Keita Kawabe and Daniel Sigg and Rana Adhikari and Peter R. Saulson},
	Date-Added = {2012-01-07 18:33:10 -0800},
	Date-Modified = {2018-06-22 20:43:06 +0000},
	Journal = {Appl. Opt.},
	Keywords = {Gravity; Fabry-Perot; Interferometry; Alignment},
	Month = {Jun},
	Number = {18},
	Pages = {3474--3484},
	Publisher = {OSA},
	Title = {Angular instability due to radiation pressure in the {LIGO} gravitational-wave detector},
	Volume = {49},
	Year = {2010},
	Bdsk-Url-1 = {http://ao.osa.org/abstract.cfm?URI=ao-49-18-3474},
	Bdsk-Url-2 = {http://dx.doi.org/10.1364/AO.49.003474}}

@article{Leonhardt:06,
	Abstract = {A number of planned space interferometry missions, including the Laser Interferometer Space Antenna (LISA)gravitational wave detector, require a laser system with high-frequencystability over long time scales. A1064 nm wavelength nonplanar ring oscillator (NPRO) laser stabilizedto a resonant transition in molecular iodine is suitable for these missions,providing high-frequency stability at an absolute reference frequency. Theiodine stabilized laser also offers low sensitivity to temperature and alignmentfluctuations and allows frequency tuning. We have evaluated the noiseperformance of a NPRO laser stabilized to iodine using frequency modulationspectroscopy and have found an Allan standard deviation of10{\textminus}14 over 100 s.Simplified optical configurations and the radiation hardness of the frequency-doublingcrystals have also been investigated.},
	Author = {Volker Leonhardt and Jordan B. Camp},
	Date-Added = {2012-01-06 16:35:19 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Appl. Opt.},
	Keywords = {Spectroscopy, modulation; Space optics},
	Month = {Jun},
	Number = {17},
	Pages = {4142--4146},
	Publisher = {OSA},
	Title = {Space interferometry application of laser frequency stabilization with molecular iodine},
	Volume = {45},
	Year = {2006},
	Bdsk-Url-1 = {http://ao.osa.org/abstract.cfm?URI=ao-45-17-4142},
	Bdsk-Url-2 = {http://dx.doi.org/10.1364/AO.45.004142}}

@article{Ma:2004,
	Abstract = {A femtosecond laser--based optical frequency synthesizer is referenced to an optical standard, and we use it to demonstrate the generation and control of the frequency of electromagnetic fields over 100 terahertz of bandwidth with fractional uncertainties approaching 1 part in 1019. The reproducibility of this performance is verified by comparison of different types of femtosecond laser--based frequency synthesizers from three laboratories.},
	Author = {Ma, Long-Sheng and Bi, Zhiyi and Bartels, Albrecht and Robertsson, Lennart and Zucco, Massimo and Windeler, Robert S. and Wilpers, Guido and Oates, Chris and Hollberg, Leo and Diddams, Scott A.},
	Date-Added = {2012-01-06 16:33:41 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Eprint = {http://www.sciencemag.org/content/303/5665/1843.full.pdf},
	Journal = {Science},
	Number = {5665},
	Pages = {1843-1845},
	Rating = {4},
	Title = {Optical Frequency Synthesis and Comparison with Uncertainty at the 10-19 Level},
	Volume = {303},
	Year = {2004},
	Bdsk-Url-1 = {http://www.sciencemag.org/content/303/5665/1843.abstract},
	Bdsk-Url-2 = {http://dx.doi.org/10.1126/science.1095092}}

@article{Cella:2011,
	Author = {G. Cella and A. Giazotto},
	Date-Added = {2012-01-04 20:13:34 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Eid = {101101},
	Journal = {Review of Scientific Instruments},
	Keywords = {gravitational wave detectors; gravitational waves; light interferometers},
	Number = {10},
	Numpages = {44},
	Pages = {101101},
	Publisher = {AIP},
	Rating = {5},
	Title = {Interferometric gravity wave detectors},
	Volume = {82},
	Year = {2011},
	Bdsk-Url-1 = {http://link.aip.org/link/?RSI/82/101101/1},
	Bdsk-Url-2 = {http://dx.doi.org/10.1063/1.3652857}}

@book{Haykin:Adaptive,
	Author = {Haykin, S.S.},
	Date-Added = {2012-01-03 14:03:25 -0800},
	Date-Modified = {2012-02-28 06:43:11 -0800},
	Isbn = {9780130901262},
	Lccn = {20021604},
	Publisher = {Prentice Hall},
	Rating = {4},
	Series = {Prentice-Hall information and system sciences series},
	Title = {Adaptive Filter Theory},
	Year = {2002},
	Bdsk-Url-1 = {http://books.google.com/books?id=eMcZAQAAIAAJ}}

@book{Huang:MIMO,
	Author = {Huang, Y. and Benesty, J. and Chen, J.},
	Date-Added = {2012-01-03 14:02:04 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Isbn = {9783540376309},
	Lccn = {2006920463},
	Publisher = {Springer},
	Series = {Signals and communication technology},
	Title = {Acoustic MIMO signal processing},
	Year = {2006},
	Bdsk-Url-1 = {http://books.google.com/books?id=OSlGAQAAIAAJ}}

@article{NIST:Wiener,
	Abstract = {We demonstrate a method to measure and actively reduce the coupling of vibrations            to the phase noise of a cavity-stabilized laser. This method uses the vibration noise of            the laboratory environment rather than active drive to perturb the optical cavity. The            laser phase noise is measured via a beat note with a second unperturbed ultra-stable            laser while the vibrations are measured by accelerometers positioned around the cavity.            A Wiener filter algorithm extracts the frequency and direction dependence of the cavity            response function. Once the cavity response function is known, real-time noise            cancellation can be implemented by use of the accelerometer measurements to predict and            then cancel the laser phase fluctuations. We present real-time noise cancellation that            results in a 25 dB reduction of the laser phase noise power spectral density.},
	Author = {Michael J. Thorpe and David R. Leibrandt and Tara M. Fortier and Till Rosenband},
	Date-Added = {2012-01-03 02:41:56 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Opt. Express},
	Keywords = {Vibration analysis; Optical resonators; Laser stabilization},
	Month = {Aug},
	Number = {18},
	Pages = {18744--18751},
	Publisher = {OSA},
	Rating = {4},
	Read = {1},
	Title = {Measurement and real-time cancellation of vibration-induced phase noise in a cavity-stabilized laser},
	Volume = {18},
	Year = {2010},
	Bdsk-Url-1 = {http://www.opticsexpress.org/abstract.cfm?URI=oe-18-18-18744},
	Bdsk-Url-2 = {http://dx.doi.org/10.1364/OE.18.018744}}

@article{3G:Science,
	Abstract = {Large gravitational wave interferometric detectors, like Virgo and LIGO, demonstrated the capability to reach their design sensitivity, but to transform these machines into an effective observational instrument for gravitational wave astronomy a large improvement in sensitivity is required. Advanced detectors in the near future and third-generation observatories in more than one decade will open the possibility to perform gravitational wave astronomical observations from the Earth. An overview of the possible science reaches and the technological progress needed to realize a third-generation observatory are discussed in this paper. The status of the project Einstein Telescope (ET), a design study of a third-generation gravitational wave observatory, will be reported.},
	Author = {M Punturo and M Abernathy and F Acernese and B Allen and N Andersson and K Arun and F Barone and B Barr and M Barsuglia and M Beker and N Beveridge and S Birindelli and S Bose and L Bosi and S Braccini and C Bradaschia and T Bulik and E Calloni and G Cella and E Chassande Mottin and S Chelkowski and A Chincarini and J Clark and E Coccia and C Colacino and J Colas and A Cumming and L Cunningham and E Cuoco and S Danilishin and K Danzmann and G De Luca and R De Salvo and T Dent and R Derosa and L Di Fiore and A Di Virgilio and M Doets and V Fafone and P Falferi and R Flaminio and J Franc and F Frasconi and A Freise and P Fulda and J Gair and G Gemme and A Gennai and A Giazotto and K Glampedakis and M Granata and H Grote and G Guidi and G Hammond and M Hannam and J Harms and D Heinert and M Hendry and I Heng and E Hennes and S Hild and J Hough and S Husa and S Huttner and G Jones and F Khalili and K Kokeyama and K Kokkotas and B Krishnan and M Lorenzini and H L{\"u}ck and E Majorana and I Mandel and V Mandic and I Martin and C Michel and Y Minenkov and N Morgado and S Mosca and B Mours and H M{\"u}ller-Ebhardt and P Murray and R Nawrodt and J Nelson and R Oshaughnessy and C D Ott and C Palomba and A Paoli and G Parguez and A Pasqualetti and R Passaquieti and D Passuello and L Pinard and R Poggiani and P Popolizio and M Prato and P Puppo and D Rabeling and P Rapagnani and J Read and T Regimbau and H Rehbein and S Reid and L Rezzolla and F Ricci and F Richard and A Rocchi and S Rowan and A R{\"u}diger and B Sassolas and B Sathyaprakash and R Schnabel and C Schwarz and P Seidel and A Sintes and K Somiya and F Speirits and K Strain and S Strigin and P Sutton and S Tarabrin and J van den Brand and C van Leewen and M van Veggel and C van den Broeck and A Vecchio and J Veitch and F Vetrano and A Vicere and S Vyatchanin and B Willke and G Woan and P Wolfango and K Yamamoto},
	Date-Added = {2012-01-03 01:47:09 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Classical and Quantum Gravity},
	Number = {8},
	Pages = {084007},
	Rating = {3},
	Title = {The third generation of gravitational wave observatories and their science reach},
	Volume = {27},
	Year = {2010},
	Bdsk-Url-1 = {http://stacks.iop.org/0264-9381/27/i=8/a=084007}}

@inproceedings{Drever:FP1991,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/1991dgw..conf..306D},
	Author = {{Drever}, R.~W.~P.},
	Booktitle = {The Detection of Gravitational Waves},
	Date-Added = {2012-01-03 01:03:22 -0800},
	Date-Modified = {2012-12-31 01:44:48 -0800},
	Editor = {{D.~G.~Blair}},
	Pages = {306},
	Rating = {4},
	Title = {{Fabry-Perot Cavity Gravity-Wave Detectors}},
	Year = 1991}

@article{Schnupp:1985,
	Abstract = {In long-light-path laser interferometry, as used for gravitational wave detection, scattered light is a major noise source. Interferometers that employ optical delay lines are particularly susceptible to noise from scattered light. The authors present a method of suppressing such noise signals by using fast phase modulation of the laser light. It is shown that all scattered all contributions from the delay line may be cancelled, up to arbitrarily long path differences. This can be achieved with an appropriately structured square-wave modulation function which switches the phase of the light by pi .},
	Author = {L Schnupp and W Winkler and K Maischberger and A Rudiger and R Schilling},
	Date-Added = {2012-01-03 00:41:32 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Journal of Physics E: Scientific Instruments},
	Number = {6},
	Pages = {482},
	Rating = {4},
	Read = {1},
	Title = {Reduction of noise due to scattered light in gravitational wave antennae by modulating the phase of the laser light},
	Volume = {18},
	Year = {1985},
	Bdsk-Url-1 = {http://stacks.iop.org/0022-3735/18/i=6/a=005}}

@article{Vinet:1988,
	Author = {Vinet, Jean-Yves and Meers, Brian and Man, Catherine Nary and Brillet, Alain},
	Date-Added = {2012-01-03 00:28:57 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issue = {2},
	Journal = {Phys. Rev. D},
	Month = {Jul},
	Pages = {433--447},
	Publisher = {American Physical Society},
	Rating = {2},
	Title = {Optimization of long-baseline optical interferometers for gravitational-wave detection},
	Volume = {38},
	Year = {1988},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.38.433},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.38.433}}

@article{Stanford:Sagnac1996,
	Author = {Sun, Ke-Xun and Fejer, M. M. and Gustafson, Eric and Byer, Robert L.},
	Date-Added = {2012-01-03 00:19:46 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issue = {17},
	Journal = {Phys. Rev. Lett.},
	Month = {Apr},
	Pages = {3053--3056},
	Publisher = {American Physical Society},
	Title = {Sagnac Interferometer for Gravitational-Wave Detection},
	Volume = {76},
	Year = {1996},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevLett.76.3053},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevLett.76.3053}}

@article{HaOr:2011,
	Abstract = {In April of 2009 a seismic survey utilizing explosive charges took place in Livingston parish, Louisiana. The area of the survey encompassed the location of the Laser Interferometer Gravitational-Wave Observatory (LIGO) Livingston interferometer. In this paper, we present an analysis of seismic data recorded with three of the LIGO seismometers and a geophone array that was deployed during the time of the survey. In particular, the geophone-array data are used to study the propagation of surface waves, whereas first-arrival measurements with the LIGO seismometers provide estimates of the speed of compressional seismic waves as a function of depth. We find that fundamental Rayleigh waves have a speed close to 205 m/s consistent with results from previous borehole tests and that speed of compressional waves is 1650 m/s at 25 m depth, increasing to 2300 m/s at 1 km depth. Blast spectra are further investigated to determine the Q value of the ground medium experienced by Rayleigh waves (f>1 Hz) and body waves deeper underground. The estimated Q value is approximately 50 for the surface waves and exceeds a value of 190 for body waves propagating at depths below 100 m.},
	Author = {Harms, Jan and O'Reilly, Brian},
	Date-Added = {2012-01-02 22:42:55 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Eprint = {http://www.bssaonline.org/content/101/4/1478.full.pdf+html},
	Journal = {Bulletin of the Seismological Society of America},
	Number = {4},
	Pages = {1478-1487},
	Rating = {3},
	Title = {Velocity and Attenuation Characterization of the LIGO Site near Livingston, Louisiana},
	Volume = {101},
	Year = {2011},
	Bdsk-Url-1 = {http://www.bssaonline.org/content/101/4/1478.abstract},
	Bdsk-Url-2 = {http://dx.doi.org/10.1785/0120100095}}

@article{aLIGO:Seismic2002,
	Abstract = {The baseline design concept for a seismic isolation component of the proposed 'Advanced LIGO' detector upgrade has been developed with proof-of-principle experiments and computer models. It consists of a two-stage in-vacuum active isolation platform that is supported by an external hydraulic actuation stage. Construction is underway for prototype testing of a full-scale preliminary design.},
	Author = {R Abbott and R Adhikari and G Allen and S Cowley and E Daw and D DeBra and J Giaime and G Hammond and M Hammond and C Hardham and J How and W Hua and W Johnson and B Lantz and K Mason and R Mittleman and J Nichol and S Richman and J Rollins and D Shoemaker and G Stapfer and R Stebbins},
	Date-Added = {2012-01-02 20:23:27 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Classical and Quantum Gravity},
	Number = {7},
	Pages = {1591},
	Rating = {2},
	Title = {Seismic isolation for Advanced LIGO},
	Volume = {19},
	Year = {2002},
	Bdsk-Url-1 = {http://stacks.iop.org/0264-9381/19/i=7/a=349}}

@article{Virgo:SA2010,
	Author = {F. Acernese and F. Antonucci and S. Aoudia and K.G. Arun and P. Astone and G. Ballardin and F. Barone and M. Barsuglia and Th.S. Bauer and M.G. Beker and S. Bigotta and S. Birindelli and M. Bitossi and M.A. Bizouard and M. Blom and C. Boccara and F. Bondu and L. Bonelli and L. Bosi and S. Braccini and C. Bradaschia and A. Brillet and V. Brisson and R. Budzy{\'n}ski and T. Bulik and H.J. Bulten and D. Buskulic and G. Cagnoli and E. Calloni and E. Campagna and B. Canuel and F. Carbognani and F. Cavalier and R. Cavalieri and G. Cella and E. Cesarini and E. Chassande-Mottin and A. Chincarini and F. Cleva and E. Coccia and C.N. Colacino and J. Colas and A. Colla and M. Colombini and C. Corda and A. Corsi and J.-P. Coulon and E. Cuoco and S. D'Antonio and A. Dari and V. Dattilo and M. Davier and R. Day and R. De Rosa and M. Del Prete and L. Di Fiore and A. Di Lieto and M. Di Paolo Emilio and A. Di Virgilio and A. Dietz and M. Drago and V. Fafone and I. Ferrante and F. Fidecaro and I. Fiori and R. Flaminio and J.-D. Fournier and J. Franc and S. Frasca and F. Frasconi and A. Freise and L. Gammaitoni and F. Garufi and G. Gemme and E. Genin and A. Gennai and A. Giazotto and M. Granata and C. Greverie and G. Guidi and H. Heitmann and P. Hello and S. Hild and D. Huet and P. Jaranowski and I. Kowalska and A. Kr{\'o}lak and P. La Penna and N. Leroy and N. Letendre and T.G.F. Li and M. Lorenzini and V. Loriette and G. Losurdo and J.-M. Mackowski and E. Majorana and N. Man and M. Mantovani and F. Marchesoni and F. Marion and J. Marque and F. Martelli and A. Masserot and F. Menzinger and C. Michel and L. Milano and Y. Minenkov and M. Mohan and J. Moreau and N. Morgado and A. Morgia and S. Mosca and V. Moscatelli and B. Mours and I. Neri and F. Nocera and G. Pagliaroli and C. Palomba and F. Paoletti and S. Pardi and M. Parisi and A. Pasqualetti and R. Passaquieti and D. Passuello and G. Persichetti and M. Pichot and F. Piergiovanni and M. Pietka and L. Pinard and R. Poggiani and M. Prato and G.A. Prodi and M. Punturo and P. Puppo and O. Rabaste and D.S. Rabeling and P. Rapagnani and V. Re and T. Regimbau and F. Ricci and F. Robinet and A. Rocchi and L. Rolland and R. Romano and D. Rosi{\'n}ska and P. Ruggi and F. Salemi and B. Sassolas and D. Sentenac and R. Sturani and B. Swinkels and A. Toncelli and M. Tonelli and E. Tournefier and F. Travasso and J. Trummer and G. Vajente and J.F.J. van den Brand and S. van der Putten and M. Vavoulidis and G. Vedovato and D. Verkindt and F. Vetrano and A. Vicer{\'e} and J.-Y. Vinet and H. Vocca and M. Was and M. Yvert},
	Date-Added = {2012-01-02 20:19:14 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issn = {0927-6505},
	Journal = {Astroparticle Physics},
	Keywords = {Seismic isolation},
	Number = {3},
	Pages = {182 - 189},
	Rating = {2},
	Title = {Measurements of Superattenuator seismic isolation by Virgo interferometer},
	Volume = {33},
	Year = {2010},
	Bdsk-Url-1 = {http://www.sciencedirect.com/science/article/pii/S0927650510000253},
	Bdsk-Url-2 = {http://dx.doi.org/10.1016/j.astropartphys.2010.01.006}}

@article{Szabi:TAMASAS,
	Abstract = {The TAMA SAS seismic attenuation system was developed to provide the extremely high level of seismic isolation required by the next generation of interferometric gravitational wave detectors to achieve the desired sensitivity at low frequencies. Our aim was to provide good performance at frequencies above ~10 Hz, while utilizing only passive subsystems in the sensitive frequency band of the TAMA interferometric gravitational wave detectors. The only active feedback is relegated below 6 Hz and it is used to damp the rigid body resonances of the attenuation chain. Simulations, based on subsystem performance characterizations, indicate that the system can achieve rms mirror residual motion measured in a few tens of nanometres. We will give a brief overview of the subsystems and point out some of the characterization results, supporting our claims of achieved performance. SAS is a passive, UHV compatible and low cost system. It is likely that extremely sensitive experiments in other fields will also profit from our study.},
	Author = {Szabolcs M{\'a}rka and Akiteru Takamori and Masaki Ando and Alessandro Bertolini and Giancarlo Cella and Riccardo DeSalvo and Mitsuhiro Fukushima and Yukiyoshi Iida and Florian Jacquier and Seiji Kawamura and Yuhiko Nishi and Kenji Numata and Virginio Sannibale and Kentaro Somiya and Ryutaro Takahashi and Hareem Tariq and Kimio Tsubono and Jose Ugas and Nicolas Viboud and Chenyang Wang and Hiroaki Yamamoto and Tatsuo Yoda},
	Date-Added = {2012-01-02 20:15:24 -0800},
	Date-Modified = {2018-06-22 20:42:41 +0000},
	Journal = {Classical and Quantum Gravity},
	Number = {7},
	Pages = {1605},
	Rating = {3},
	Title = {Anatomy of the {TAMA SAS} seismic attenuation system},
	Volume = {19},
	Year = {2002},
	Bdsk-Url-1 = {http://stacks.iop.org/0264-9381/19/i=7/a=351}}

@article{Giaime:1996,
	Author = {Joseph Giaime and Partha Saha and David Shoemaker and Lisa Sievers},
	Date-Added = {2012-01-02 20:07:40 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Review of Scientific Instruments},
	Keywords = {ELASTOMERS; INTERFEROMETRY; MECHANICAL VIBRATIONS; SEISMIC NOISE; STAINLESS STEELS; GRAVITATIONAL WAVE DETECTORS; LASER BEAMS; VISCOELASTICITY},
	Number = {1},
	Pages = {208-214},
	Publisher = {AIP},
	Title = {A passive vibration isolation stack for LIGO: Design, modeling, and testing},
	Volume = {67},
	Year = {1996},
	Bdsk-Url-1 = {http://link.aip.org/link/?RSI/67/208/1},
	Bdsk-Url-2 = {http://dx.doi.org/10.1063/1.1146573}}

@article{Stefano:2001,
	Author = {G. Ballardin and L. Bracci and S. Braccini and C. Bradaschia and C. Casciano and G. Calamai and R. Cavalieri and R. Cecchi and G. Cella and E. Cuoco and E. D'Ambrosio and V. Dattilo and A. Di Virgilio and L. Fabbroni and F. Fidecaro and F. Frasconi and A. Gaddi and A. Gennai and G. Gennaro and A. Giazotto and G. Losurdo and L. Holloway and P. La Penna and F. Lelli and E. Majorana and M. Mazzoni and F. Paoletti and M. Pasotti and A. Pasqualetti and R. Passaquieti and D. Passuello and R. Poggiani and P. Puppo and F. Raffaelli and P. Rapagnani and F. Ricci and P. Ruggi and R. Stanga and R. Taddei and F. Vetrano and A. Vicere and Z. Zhang},
	Date-Added = {2012-01-02 19:31:19 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Review of Scientific Instruments},
	Keywords = {gravitational wave detectors; astronomical instruments; light interferometers; vibration isolation; physical instrumentation control; measurement by laser beam; pendulums; mechanical stability; transfer functions; optical control},
	Number = {9},
	Pages = {3643-3652},
	Publisher = {AIP},
	Rating = {3},
	Read = {1},
	Title = {Measurement of the VIRGO superattenuator performance for seismic noise suppression},
	Volume = {72},
	Year = {2001},
	Bdsk-Url-1 = {http://link.aip.org/link/?RSI/72/3643/1},
	Bdsk-Url-2 = {http://dx.doi.org/10.1063/1.1392338}}

@article{BeEA1998,
	Abstract = {In this paper we analyse the noise level induced by changes in the mass density distribution around the Virgo interferometric antenna. These stochastic mass density fluctuations generate a gravitational field which couples directly to the mirrors of the optical apparatus, and it could be relevant if the planned final sensitivity of the Virgo interferometer is to be reached.},
	Author = {M Beccaria and M Bernardini and S Braccini and C Bradaschia and A Bozzi and C Casciano and G Cella and A Ciampa and E Cuoco and G Curci and E D'Ambrosio and V Dattilo and G De Carolis and R De Salvo and A Di Virgilio and A Delapierre and D Enard and A Errico and G Feng and I Ferrante and F Fidecaro and F Frasconi and A Gaddi and A Gennai and G Gennaro and A Giazotto and P La Penna and G Losurdo and M Maggiore and S Mancini and F Palla and H B Pan and F Paoletti and A Pasqualetti and R Passaquieti and D Passuello and R Poggiani and P Popolizio and F Raffaelli and S Rapisarda and A Vicer{\'e} and Z Zhang},
	Date-Added = {2012-01-02 03:44:39 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Classical and Quantum Gravity},
	Number = {11},
	Pages = {3339},
	Title = {Relevance of Newtonian seismic noise for the VIRGO interferometer sensitivity},
	Volume = {15},
	Year = {1998},
	Bdsk-Url-1 = {http://stacks.iop.org/0264-9381/15/i=11/a=004}}

@article{Kip:Dancing,
	Author = {Thorne, Kip S. and Winstein, Carolee J.},
	Date-Added = {2012-01-02 03:28:15 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issue = {8},
	Journal = {Phys. Rev. D},
	Month = {Sep},
	Numpages = {11},
	Pages = {082001},
	Publisher = {American Physical Society},
	Rating = {3},
	Title = {Human gravity-gradient noise in interferometric gravitational-wave detectors},
	Volume = {60},
	Year = {1999},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.60.082001},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.60.082001}}

@article{Cre2008,
	Abstract = {The relative positions of the test masses in gravitational-wave detectors will be influenced not only by astrophysical gravitational waves, but also by the fluctuating Newtonian gravitational forces of moving masses in the ground and air around the detector. These effects are often referred to as gravity gradient noise. This paper considers the effects of gravity gradients from density perturbations in the atmosphere, and from massive airborne objects near the detector. These have been discussed previously by Saulson (1984 Phys. Rev. D 30 732), who considered the effects of background acoustic pressure waves and of massive objects moving smoothly past the interferometer; the gravity gradients he predicted would be too small to be of serious concern even for advanced interferometric gravitational-wave detectors. In this paper, I revisit these phenomena, considering transient atmospheric shocks, and estimating the effects of sound waves or objects colliding with the ground or buildings around the test masses. I also consider another source of atmospheric density fluctuations: temperature perturbations that are advected past the detector by the wind. I find that background acoustic noise and temperature fluctuations still produce gravity gradient noise that is below the noise floor even of advanced interferometric detectors, although temperature perturbations carried along non-laminar streamlines could produce noise that is within an order of magnitude of the projected noise floor at 10 Hz. A definitive study of this effect may require better models of the wind flow past a given instrument. I also find that transient shockwaves in the atmosphere could potentially produce large spurious signals, with signal-to-noise ratios in the hundreds in an advanced interferometric detector. These signals could be vetoed by means of acoustic sensors outside of the buildings. Massive wind-borne objects such as tumbleweeds could also produce gravity gradient signals with signal-to-noise ratios in the hundreds if they collide with the interferometer buildings, so it may be necessary to build fences preventing such objects from approaching within about 30 m of the test masses.},
	Author = {Teviet Creighton},
	Date-Added = {2012-01-02 03:01:56 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Classical and Quantum Gravity},
	Number = {12},
	Pages = {125011},
	Rating = {2},
	Title = {Tumbleweeds and airborne gravitational noise sources for LIGO},
	Volume = {25},
	Year = {2008},
	Bdsk-Url-1 = {http://stacks.iop.org/0264-9381/25/i=12/a=125011}}

@article{HuTh1998,
	Author = {Hughes, Scott A. and Thorne, Kip S.},
	Date-Added = {2012-01-02 02:53:13 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issue = {12},
	Journal = {Phys. Rev. D},
	Month = {Nov},
	Numpages = {27},
	Pages = {122002},
	Publisher = {American Physical Society},
	Rating = {5},
	Read = {1},
	Title = {Seismic gravity-gradient noise in interferometric gravitational-wave detectors},
	Volume = {58},
	Year = {1998},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.58.122002},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.58.122002}}

@article{Saulson:NN,
	Author = {Saulson, Peter R.},
	Date-Added = {2012-01-02 02:25:51 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issue = {4},
	Journal = {Phys. Rev. D},
	Month = {Aug},
	Pages = {732--736},
	Publisher = {American Physical Society},
	Title = {Terrestrial gravitational noise on a gravitational wave antenna},
	Volume = {30},
	Year = {1984},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.30.732},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.30.732}}

@article{LIGO:Science,
	Abstract = {The goal of the Laser Interferometer Gravitational-Wave Observatory (LIGO) Project is to detect and study astrophysical gravitational waves and use data from them for research in physics and astronomy. LIGO will support studies concerning the nature and nonlinear dynamics of gravity, the structures of black holes, and the equation of state of nuclear matter. It will also measure the masses, birth rates, collisions, and distributions of black holes and neutron stars in the universe and probe the cores of supernovae and the very early universe. The technology for LIGO has been developed during the past 20 years. Construction will begin in 1992, and under the present schedule, LIGO's gravitational-wave searches will begin in 1998.},
	Author = {Abramovici, Alex and Althouse, William E. and Drever, Ronald W. P. and G{\"u}rsel, Yekta and Kawamura, Seiji and Raab, Frederick J. and Shoemaker, David and Sievers, Lisa and Spero, Robert E. and Thorne, Kip S. and Vogt, Rochus E. and Weiss, Rainer and Whitcomb, Stanley E. and Zucker, Michael E.},
	Date-Added = {2012-01-01 17:16:46 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Eprint = {http://www.sciencemag.org/content/256/5055/325.full.pdf},
	Journal = {Science},
	Number = {5055},
	Pages = {325-333},
	Rating = {4},
	Read = {1},
	Title = {LIGO: The Laser Interferometer Gravitational-Wave Observatory},
	Volume = {256},
	Year = {1992},
	Bdsk-Url-1 = {http://www.sciencemag.org/content/256/5055/325.abstract},
	Bdsk-Url-2 = {http://dx.doi.org/10.1126/science.256.5055.325}}

@article{DHS:Detector2004,
	Author = {Abbott, B. and Abbott, R. and Adhikari, R. and Ageev, A. and Allen, B. and Amin, R. and Anderson, SB and Anderson, WG and Araya, M. and Armandula, H. and others},
	Date-Added = {2012-01-01 17:02:10 -0800},
	Date-Modified = {2012-01-01 17:02:35 -0800},
	Journal = {Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment},
	Number = {1},
	Pages = {154--179},
	Publisher = {Elsevier},
	Title = {Detector description and performance for the first coincidence observations between LIGO and GEO},
	Volume = {517},
	Year = {2004}}

@phdthesis{NSmith:Thesis,
	Author = {Nicolas Smith},
	Date-Added = {2011-12-30 19:54:15 -0500},
	Date-Modified = {2012-05-03 09:04:10 +0000},
	Keywords = {interferometer LIGO},
	Rating = {3},
	Read = {0},
	School = {{Massachusetts Institute of Technology}},
	Year = {2012}}

@phdthesis{Hartmut:PhD,
	Author = {Hartmut Grote},
	Date-Added = {2011-12-30 19:51:55 -0500},
	Date-Modified = {2011-12-30 19:52:47 -0500},
	Keywords = {geo interferometer},
	Rating = {5},
	School = {{Universit\"at Hannover}},
	Title = {Making it Work: Second Generation Interferometry in GEO 600!},
	Year = {2003}}

@phdthesis{Lisa:PhD,
	Author = {Lisa Barsotti},
	Date-Added = {2011-12-30 19:43:51 -0500},
	Date-Modified = {2011-12-30 19:44:50 -0500},
	Keywords = {virgo interferometer control},
	Rating = {3},
	School = {University of Pisa},
	Title = {The control of the Virgo interferometer for gravitational wave detection},
	Year = {2006}}

@article{Sigg:2008,
	Abstract = {All three LIGO gravitational wave detectors have reached their design sensitivities. A sky-averaged detection range (SNR > 8) of more than 15 Mpc for gravitational waves emitted from inspiral binary neutron stars with masses of 1.4 M ##IMG## [http://ej.iop.org/icons/Entities/odot.gif] {odot} has been achieved with the two 4 km instruments. The fifth LIGO science run started in November 2005 and ended in September 2007. A full year of triple coincidence data has been acquired. The duty cycle of a single instrument was between 66% and 79%. Results from previous science runs are presented.},
	Author = {Daniel Sigg and the LIGO Scientific Collaboration},
	Date-Added = {2011-12-30 02:42:34 -0500},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Classical and Quantum Gravity},
	Number = {11},
	Pages = {114041},
	Title = {Status of the LIGO detectors},
	Volume = {25},
	Year = {2008},
	Bdsk-Url-1 = {http://stacks.iop.org/0264-9381/25/i=11/a=114041}}

@article{Virgo:2011,
	Abstract = {We describe the present state and future evolution of the Virgo gravitational wave detector, realized by the Virgo Collaboration at the European Gravitational Observatory, in Cascina near Pisa in Italy. We summarize basic principles of the operation and the design features of the Virgo detector. We present the sensitivity evolution due to a series of intermediate upgrades called Virgo+ which is being completed this year and includes new monolithic suspensions. We describe the present scientific potential of the detector. Finally we discuss the plans for the second generation of the detector, called Advanced Virgo, introducing its new features, the expected sensitivity evolution and the scientific potential.},
	Author = {T Accadia and F Acernese and F Antonucci and P Astone and G Ballardin and F Barone and M Barsuglia and A Basti and Th S Bauer and M Bebronne and M G Beker and A Belletoile and S Birindelli and M Bitossi and M A Bizouard and M Blom and F Bondu and L Bonelli and R Bonnand and V Boschi and L Bosi and B Bouhou and S Braccini and C Bradaschia and M Branchesi and T Briant and A Brillet and V Brisson and R Budzy{\'n}ski and T Bulik and H J Bulten and D Buskulic and C Buy and G Cagnoli and E Calloni and B Canuel and F Carbognani and F Cavalier and R Cavalieri and G Cella and E Cesarini and O Chaibi and E Chassande Mottin and A Chincarini and F Cleva and E Coccia and P-F Cohadon and C N Colacino and J Colas and A Colla and M Colombini and A Corsi and J-P Coulon and E Cuoco and S D'Antonio and V Dattilo and M Davier and R Day and R De Rosa and G Debreczeni and W Del Pozzo and M del Prete and L Di Fiore and A Di Lieto and M Di Paolo Emilio and A Di Virgilio and A Dietz and M Drago and V Fafone and I Ferrante and F Fidecaro and I Fiori and R Flaminio and L A Forte and J-D Fournier and J Franc and S Frasca and F Frasconi and M Galimberti and L Gammaitoni and F Garufi and M E G{\'a}sp{\'a}r and G Gemme and E Genin and A Gennai and A Giazotto and R Gouaty and M Granata and C Greverie and G M Guidi and J-F Hayau and A Heidmann and H Heitmann and P Hello and D Huet and P Jaranowski and I Kowalska and A Kr{\'o}lak and N Leroy and N Letendre and T G F Li and N Liguori and M Lorenzini and V Loriette and G Losurdo and E Majorana and I Maksimovic and N Man and M Mantovani and F Marchesoni and F Marion and J Marque and F Martelli and A Masserot and C Michel and L Milano and Y Minenkov and M Mohan and N Morgado and A Morgia and S Mosca and V Moscatelli and B Mours and F Nocera and G Pagliaroli and L Palladino and C Palomba and F Paoletti and M Parisi and A Pasqualetti and R Passaquieti and D Passuello and G Persichetti and M Pichot and F Piergiovanni and M Pietka and L Pinard and R Poggiani and M Prato and G A Prodi and M Punturo and P Puppo and D S Rabeling and I R{\'a}cz and P Rapagnani and V Re and T Regimbau and F Ricci and F Robinet and A Rocchi and L Rolland and R Romano and D Rosi{\'n}ska and P Ruggi and B Sassolas and D Sentenac and L Sperandio and R Sturani and B Swinkels and M Tacca and L Taffarello and A Toncelli and M Tonelli and O Torre and E Tournefier and F Travasso and G Vajente and J F J van den Brand and C Van Den Broeck and S van der Putten and M Vasuth and M Vavoulidis and G Vedovato and D Verkindt and F Vetrano and A Vicer{\'e} and J-Y Vinet and S Vitale and H Vocca and R L Ward and M Was and M Yvert and J-P Zendri},
	Date-Added = {2011-12-30 02:37:45 -0500},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Classical and Quantum Gravity},
	Number = {11},
	Pages = {114002},
	Title = {Status of the Virgo project},
	Volume = {28},
	Year = {2011},
	Bdsk-Url-1 = {http://stacks.iop.org/0264-9381/28/i=11/a=114002}}

@article{Hartmut:2010,
	Abstract = {The British--German gravitational wave detector GEO 600 has concluded a long observational period called Astrowatch , which lasted from November 2007 to July 2009. Together with the LIGO-H2 detector, GEO 600 was kept observing, while other detectors of the world-wide network of laser-interferometers like LIGO(L1 and H1) and Virgo were upgraded. A fraction of the time during the astrowatch period was set apart for noise investigations and experiments preparing future upgrades. Even with these investigations GEO 600 reached an observation time of 86.0% of the overall time, such that a total of 522 days worth of data were collected. The average sensitivity was roughly a factor of 2 lower than that of the LIGO-H2 detector for frequencies above 500 Hz. In July 2009 GEO 600 has started an upgrade program called GEO-HF . Within this program we aim at improving the sensitivity by a number of sequential upgrades, like tuned signal recycling, DC readout, output mode-cleaning, injection of squeezed vacuum states and the increase of circulating light power. Tuned signal recycling and DC readout have already been implemented and can be operated robustly, due to a new technique associated with the automatic alignment system.},
	Author = {Hartmut Grote},
	Date-Added = {2011-12-30 02:13:30 -0500},
	Date-Modified = {2012-02-15 21:22:47 -0800},
	Journal = {Classical and Quantum Gravity},
	Number = {8},
	Pages = {084003},
	Title = {The GEO 600 status},
	Volume = {27},
	Year = {2010},
	Bdsk-Url-1 = {http://stacks.iop.org/0264-9381/27/i=8/a=084003}}

@article{TAMA:2009,
	Abstract = {The Large-scale Cryogenic Gravitational wave Telescope (LCGT) is planned as a future Japanese project for gravitational wave detection. A 3 km interferometer will be built in an underground mine at Kamioka. Cryogenic sapphire mirrors are going to be employed for the test masses. For the demonstration of LCGT technologies, two prototype interferometers, TAMA300 and CLIO, are being developed. This paper describes the current status of the LCGT project and the two prototype interferometers.},
	Author = {K Arai and R Takahashi and D Tatsumi and K Izumi and Y Wakabayashi and H Ishizaki and M Fukushima and T Yamazaki and M-K Fujimoto and A Takamori and K Tsubono and R DeSalvo and A Bertolini and S M{\'a}rka and V Sannibale and the TAMA Collaboration and T Uchiyama and O Miyakawa and S Miyoki and K Agatsuma and T Saito and M Ohashi and K Kuroda and I Nakatani and S Telada and K Yamamoto and T Tomaru and T Suzuki and T Haruyama and N Sato and A Yamamoto and T Shintomi and the CLIO Collaboration and The LCGT Collaboration},
	Date-Added = {2011-12-30 02:05:41 -0500},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Classical and Quantum Gravity},
	Number = {20},
	Pages = {204020},
	Rating = {3},
	Title = {Status of Japanese gravitational wave detectors},
	Volume = {26},
	Year = {2009},
	Bdsk-Url-1 = {http://stacks.iop.org/0264-9381/26/i=20/a=204020}}

@article{TAMA:2008,
	Abstract = {TAMA300 has been upgraded to improve the sensitivity at low frequencies after the last observation run in 2004. To avoid the noise caused by seismic activities, we installed a new seismic isolation system---the TAMA seismic attenuation system (SAS). Four SAS towers for the test-mass mirrors were sequentially installed from 2005 to 2006. The recycled Fabry--Perot Michelson interferometer was successfully locked with the SAS. We confirmed the reduction of both length and angular fluctuations at frequencies higher than 1 Hz owing to the SAS.},
	Author = {R Takahashi and K Arai and D Tatsumi and M Fukushima and T Yamazaki and M-K Fujimoto and K Agatsuma and Y Arase and N Nakagawa and A Takamori and K Tsubono and R DeSalvo and A Bertolini and S M{\'a}rka and V Sannibale and the TAMA Collaboration},
	Date-Added = {2011-12-30 01:58:00 -0500},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Classical and Quantum Gravity},
	Number = {11},
	Pages = {114036},
	Title = {Operational status of TAMA300 with the seismic attenuation system (SAS)},
	Volume = {25},
	Year = {2008},
	Bdsk-Url-1 = {http://stacks.iop.org/0264-9381/25/i=11/a=114036}}

@article{Corbitt:Review2004,
	Abstract = {We present an overview of quantum noise in gravitational-wave interferometers. Current gravitational-wave detectors are modified variants of a Michelson interferometer and the quantum noise limits are strongly influenced by the optical configuration of the interferometer. We describe recent developments in the treatment of quantum noise in the complex interferometers of present-day and future gravitational-wave detectors and explore prospects for beating the standard quantum limit by use of both injected and ponderomotive squeezing in future interferometers.},
	Author = {Thomas Corbitt and Nergis Mavalvala},
	Date-Added = {2011-12-29 20:07:15 -0500},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Journal of Optics B: Quantum and Semiclassical Optics},
	Number = {8},
	Pages = {S675},
	Title = {Review: Quantum noise in gravitational-wave interferometers},
	Volume = {6},
	Year = {2004},
	Bdsk-Url-1 = {http://stacks.iop.org/1464-4266/6/i=8/a=008}}

@article{Richman:1997,
	Author = {D. B. Newell and S. J. Richman and P. G. Nelson and R. T. Stebbins and P. L. Bender and J. E. Faller and J. Mason},
	Date-Added = {2011-12-29 17:45:58 -0500},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Review of Scientific Instruments},
	Keywords = {gravitational wave detectors; light interferometers; astronomical instruments; vibration control; physical instrumentation control; pendulums; servomechanisms; feedback; adaptive control},
	Number = {8},
	Pages = {3211-3219},
	Publisher = {AIP},
	Title = {An ultra-low-noise, low-frequency, six degrees of freedom active vibration isolator},
	Volume = {68},
	Year = {1997},
	Bdsk-Url-1 = {http://link.aip.org/link/?RSI/68/3211/1},
	Bdsk-Url-2 = {http://dx.doi.org/10.1063/1.1148269}}

@article{Chu:1999,
	Author = {Joel M. Hensley and Achim Peters and Steven Chu},
	Date-Added = {2011-12-29 17:17:13 -0500},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Review of Scientific Instruments},
	Keywords = {vibration isolation; particle interferometry; acceleration measurement; measurement errors; feedback},
	Number = {6},
	Pages = {2735-2741},
	Publisher = {AIP},
	Title = {Active low frequency vertical vibration isolation},
	Volume = {70},
	Year = {1999},
	Bdsk-Url-1 = {http://link.aip.org/link/?RSI/70/2735/1},
	Bdsk-Url-2 = {http://dx.doi.org/10.1063/1.1149838}}

@article{Logan:1993,
	Abstract = {... 10] PM Morse, Vibration and sound (McGraw-Hill, New York, 1948) p. 170. 11 ] J. Kovalik and PR Saulson , submitted to Rev. Sci. Instrum. ... PM Morse, Vibration and sound, McGraw-Hill, New York (1948), p. 170. J. Kovalik and PR Saulson , submitted to Rev. Sci. Instrum. ...},
	Author = {J.~E.~Logan and J.~Hough and N.~A.~Robertson},
	Date-Added = {2011-12-29 00:35:03 -0500},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Physics Letters A},
	Rating = {0},
	Read = {Yes},
	Title = {Aspects of the thermal motion of a mass suspended as a pendulum by wires},
	Year = {1993},
	Bdsk-File-1 = {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},
	Bdsk-Url-1 = {http://www.sciencedirect.com/science/article/pii/037596019391161W}}

@article{gonzalez:207,
	Author = {Gabriela I. Gonz{\'a}lez and Peter R. Saulson},
	Date-Added = {2011-12-29 00:30:46 -0500},
	Date-Modified = {2013-01-17 07:40:13 +0000},
	Journal = {The Journal of the Acoustical Society of America},
	Keywords = {PENDULUMS; EQUATIONS OF MOTION; WIRES; FIBERS; MECHANICAL VIBRATIONS; TEMPERATURE NOISE; POWER SPECTRA; GRAVITATIONAL WAVE DETECTORS; ANELASTICITY; BROWNIAN MOVEMENT},
	Number = {1},
	Pages = {207-212},
	Publisher = {ASA},
	Title = {Brownian motion of a mass suspended by an anelastic wire},
	Volume = {96},
	Year = {1994},
	Bdsk-Url-1 = {http://link.aip.org/link/?JAS/96/207/1},
	Bdsk-Url-2 = {http://dx.doi.org/10.1121/1.410467}}

@book{Zener:1948,
	Author = {C.~M.~Zener},
	Date-Added = {2011-12-28 21:33:42 -0500},
	Date-Modified = {2011-12-28 21:34:57 -0500},
	Publisher = {University of Chicago Press},
	Rating = {5},
	Title = {Elasticity and Anelasticity of Metals},
	Year = {1948}}

@article{Rob:2008,
	Abstract = {The Laser Interferometer Gravitational Wave Observatory (LIGO) operates a 40m prototype interferometer on the Caltech campus. The primary mission of the prototype is to serve as an experimental testbed for upgrades to the LIGO interferometers and for gaining experience with advanced interferometric techniques, including detuned resonant sideband extraction (i.e. signal recycling) and dc readout (optical homodyne detection). The former technique will be employed in Advanced LIGO, and the latter in both Enhanced and Advanced LIGO. Using dc readout for gravitational wave signal extraction has several technical advantages, including reduced laser and oscillator noise couplings as well as reduced shot noise, when compared to the traditional rf readout technique (optical heterodyne detection) currently in use in large-scale ground-based interferometric gravitational wave detectors. The Caltech 40m laboratory is currently prototyping a dc readout system for a fully suspended interferometric gravitational wave detector. The system includes an optical filter cavity at the interferometer's output port, and the associated controls and optics to ensure that the filter cavity is optimally coupled to the interferometer. We present the results of measurements to characterize noise couplings in rf and dc readout using this system.},
	Author = {R L Ward and R Adhikari and B Abbott and R Abbott and D Barron and R Bork and T Fricke and V Frolov and J Heefner and A Ivanov and O Miyakawa and K McKenzie and B Slagmolen and M Smith and R Taylor and S Vass and S Waldman and A Weinstein},
	Date-Added = {2011-12-26 19:39:57 -0600},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Classical and Quantum Gravity},
	Number = {11},
	Pages = {114030},
	Title = {{DC} readout experiment at the Caltech 40m prototype interferometer},
	Volume = {25},
	Year = {2008},
	Bdsk-Url-1 = {http://stacks.iop.org/0264-9381/25/i=11/a=114030}}

@article{Geppo:2000,
	Author = {G. Cagnoli and J. Hough and D. DeBra and M.M. Fejer and E. Gustafson and S. Rowan and V. Mitrofanov},
	Date-Added = {2011-12-26 19:25:48 -0600},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issn = {0375-9601},
	Journal = {Physics Letters A},
	Number = {1-2},
	Pages = {39 - 45},
	Title = {Damping dilution factor for a pendulum in an interferometric gravitational waves detector},
	Volume = {272},
	Year = {2000},
	Bdsk-Url-1 = {http://www.sciencedirect.com/science/article/pii/S0375960100004114},
	Bdsk-Url-2 = {http://dx.doi.org/10.1016/S0375-9601(00)00411-4}}

@article{Gerhard:1998,
	Author = {Heinzel, G. and Strain, K. A. and Mizuno, J. and Skeldon, K. D. and Willke, B. and Winkler, W. and Schilling, R. and R\"udiger, A. and Danzmann, K.},
	Date-Added = {2011-12-23 10:38:51 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issue = {25},
	Journal = {Phys. Rev. Lett.},
	Month = {Dec},
	Pages = {5493--5496},
	Publisher = {American Physical Society},
	Title = {Experimental Demonstration of a Suspended Dual Recycling Interferometer for Gravitational Wave Detection},
	Volume = {81},
	Year = {1998},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevLett.81.5493},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevLett.81.5493}}

@article{Brett:2003,
	Author = {Bochner, Brett},
	Date-Added = {2011-12-23 10:20:55 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issn = {0001-7701},
	Issue = {6},
	Journal = {General Relativity and Gravitation},
	Keyword = {Physics and Astronomy},
	Note = {10.1023/A:1024016917669},
	Pages = {1029-1057},
	Publisher = {Springer Netherlands},
	Title = {Simulating a Dual-Recycled Gravitational Wave Interferometer with Realistically Imperfect Optics},
	Volume = {35},
	Year = {2003},
	Bdsk-Url-1 = {http://dx.doi.org/10.1023/A:1024016917669}}

@techreport{Kip:Scatter95,
	Author = {E.~E.~Flanagan and K.~S.~Thorne},
	Date-Added = {2011-12-18 00:31:38 -0800},
	Date-Modified = {2018-06-22 20:41:55 +0000},
	Institution = {LIGO},
	Number = {T950102},
	Title = {Scattered-Light Noise for {LIGO}},
	Url = {https://dcc.ligo.org/LIGO-T950102/public},
	Year = {1995},
	Bdsk-Url-1 = {https://dcc.ligo.org/LIGO-T950102/public}}

@techreport{Weiss:Scatter97,
	Address = {https://dcc.ligo.org/public/T970083},
	Author = {Rainer Weiss},
	Date-Added = {2011-12-18 00:29:13 -0800},
	Date-Modified = {2015-10-20 00:22:55 +0000},
	Institution = {LIGO},
	Title = {Concerning: Scattering in the Interferometer},
	Year = {1997}}

@article{Stefano:Scatter,
	Author = {Vinet, Jean-Yves and Brisson, Violette and Braccini, Stefano},
	Date-Added = {2011-12-18 00:24:24 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issue = {2},
	Journal = {Phys. Rev. D},
	Month = {Jul},
	Pages = {1276--1286},
	Publisher = {American Physical Society},
	Title = {Scattered light noise in gravitational wave interferometric detectors: Coherent effects},
	Volume = {54},
	Year = {1996},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.54.1276},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.54.1276}}

@article{Gillespie:1995,
	Author = {Gillespie, A. and Raab, F.},
	Date-Added = {2011-12-17 09:39:26 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issue = {2},
	Journal = {Phys. Rev. D},
	Month = {Jul},
	Pages = {577--585},
	Publisher = {American Physical Society},
	Title = {Thermally excited vibrations of the mirrors of laser interferometer gravitational-wave detectors},
	Volume = {52},
	Year = {1995},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.52.577},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.52.577}}

@article{Blair:RPP2000,
	Abstract = {Gravitational wave detectors have been under development since the pioneering work of Weber in the 1960s. The long and painstaking research effort has yielded enormous improvements in detector sensitivity. Astronomical observations of binary pulsar systems have confirmed the existence of gravitational radiation. Direct detection is inevitable once planned detectors reach sensitivity goals. This review begins by introducing the concept of gravitational waves, and discusses their significance. Section 2 discusses sources of gravitational waves, giving estimates of signal characteristics and signal strengths. Section 3 presents an overview of gravitational wave detection and the critical issues of data processing. In the fourth section the physics of resonant-mass gravitational wave detectors is discussed in some detail, covering all areas from antenna materials to transducers and the quantum limits to measurement. This section reviews the major operating antennas in the existing worldwide array but also discusses the prospects for achieving substantial increases in sensitivity in the future. The fifth section presents the concepts and designs for laser interferometer gravitational wave detectors. Large-scale devices will be in operation in the first decade of the twenty-first century and should eventually be certain of detecting a known class of gravitational wave source. At their predicted sensitivity, space interferometers will be able to detect numerous known galactic sources of gravitational waves and also will be able to detect black hole mergers that are thought to have occurred as primordial galaxies merged and grew in the early universe.},
	Author = {L Ju and D G Blair and C Zhao},
	Date-Added = {2011-12-17 08:34:11 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Reports on Progress in Physics},
	Number = {9},
	Pages = {1317},
	Title = {Detection of gravitational waves},
	Volume = {63},
	Year = {2000},
	Bdsk-Url-1 = {http://stacks.iop.org/0034-4885/63/i=9/a=201}}

@article{Matt:TOnoise,
	Author = {Evans, M. and Ballmer, S. and Fejer, M. and Fritschel, P. and Harry, G. and Ogin, G.},
	Date-Added = {2011-12-17 05:29:48 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issue = {10},
	Journal = {Phys. Rev. D},
	Month = {Nov},
	Numpages = {10},
	Pages = {102003},
	Publisher = {American Physical Society},
	Title = {Thermo-optic noise in coated mirrors for high-precision optical measurements},
	Volume = {78},
	Year = {2008},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.78.102003},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.78.102003}}

@article{Goro:2011,
	Author = {Kondratiev, N. M. and Gurkovsky, A. G. and Gorodetsky, M. L.},
	Date-Added = {2011-12-17 05:11:18 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issue = {2},
	Journal = {Phys. Rev. D},
	Month = {Jul},
	Numpages = {9},
	Pages = {022001},
	Publisher = {American Physical Society},
	Title = {Thermal noise and coating optimization in multilayer dielectric mirrors},
	Volume = {84},
	Year = {2011},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.84.022001},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.84.022001}}

@article{Harry:CQG2007,
	Abstract = {Reducing thermal noise from optical coatings is crucial to reaching the required sensitivity in next generation interferometric gravitational-wave detectors. Here we show that adding TiO 2 to Ta 2 O 5 in Ta 2 O 5 /SiO 2 coatings reduces the internal friction and in addition present data confirming it reduces thermal noise. We also show that TiO 2 -doped Ta 2 O 5 /SiO 2 coatings are close to satisfying the optical absorption requirements of second generation gravitational-wave detectors.},
	Author = {Gregory M Harry and Matthew R Abernathy and Andres E Becerra-Toledo and Helena Armandula and Eric Black and Kate Dooley and Matt Eichenfield and Chinyere Nwabugwu and Akira Villar and D R M Crooks and Gianpietro Cagnoli and Jim Hough and Colin R How and Ian MacLaren and Peter Murray and Stuart Reid and Sheila Rowan and Peter H Sneddon and Martin M Fejer and Roger Route and Steven D Penn and Patrick Ganau and Jean-Marie Mackowski and Christophe Michel and Laurent Pinard and Alban Remillieux},
	Date-Added = {2011-12-17 05:09:10 -0800},
	Date-Modified = {2012-01

license: MIT

license_type: permissive

branch_name: refs/heads/master

extension: bib