text:
-22 20:42:00 -0800},
	Journal = {Classical and Quantum Gravity},
	Number = {2},
	Pages = {405},
	Title = {Titania-doped tantala/silica coatings for gravitational-wave detection},
	Volume = {24},
	Year = {2007},
	Bdsk-Url-1 = {http://stacks.iop.org/0264-9381/24/i=2/a=008}}

@article{Harry:AO2006,
	Abstract = {Gravitational waves are a prediction of Einstein's general theory of relativity.These waves are created by massive objects, like neutron stars or black holes, oscillating at speeds appreciable to the speed of light. The detectable effect on the Earth of these waves is extremely small, however, creating strains of the order of10{\textminus}21. There are a number of basic physics experiments around the world designed to detect these waves by using interferometers with very long arms, up to4 km in length. The next-generation interferometers are currently being designed, and the thermal noise in the mirrors will set the sensitivity over much of the usable bandwidth. Thermal noise arising from mechanical loss in the optical coatings put on the mirrors will be a significant source of noise. Achieving higher sensitivity through lower mechanical loss coatings, while preserving the crucial optical and thermal properties, is an area of active research right now.},
	Author = {Gregory M. Harry and Helena Armandula and Eric Black and D. R. M. Crooks and Gianpietro Cagnoli and Jim Hough and Peter Murray and Stuart Reid and Sheila Rowan and Peter Sneddon and Martin M. Fejer and Roger Route and Steven D. Penn},
	Date-Added = {2011-12-17 04:50:14 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Appl. Opt.},
	Keywords = {Interference coatings ; Thin films, other properties; Astronomy and astrophysics},
	Month = {Mar},
	Number = {7},
	Pages = {1569--1574},
	Publisher = {OSA},
	Title = {Thermal noise from optical coatings in gravitational wave detectors},
	Volume = {45},
	Year = {2006},
	Bdsk-Url-1 = {http://ao.osa.org/abstract.cfm?URI=ao-45-7-1569},
	Bdsk-Url-2 = {http://dx.doi.org/10.1364/AO.45.001569}}

@article{Penn:CQG2003,
	Abstract = {Current interferometric gravitational wave detectors use test masses with mirror coatings formed from multiple layers of dielectric materials, most commonly alternating layers of SiO 2 (silica) and Ta 2 O 5 (tantala). However, mechanical loss in the Ta 2 O 5 /SiO 2 coatings may limit the design sensitivity for advanced detectors. We have investigated sources of mechanical loss in the Ta 2 O 5 /SiO 2 coatings, including loss associated with the coating--substrate interface, with the coating--layer interfaces and with the coating materials. Our results indicate that the loss is associated with the coating materials and that the loss of Ta 2 O 5 is substantially larger than that of SiO 2 .},
	Author = {Steven D Penn and Peter H Sneddon and Helena Armandula and Joseph C Betzwieser and Gianpietro Cagnoli and Jordan Camp and D R M Crooks and Martin M Fejer and Andri M Gretarsson and Gregory M Harry and Jim Hough and Scott E Kittelberger and Michael J Mortonson and Roger Route and Sheila Rowan and Christophoros C Vassiliou},
	Date-Added = {2011-12-17 04:45:40 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Classical and Quantum Gravity},
	Number = {13},
	Pages = {2917},
	Title = {Mechanical loss in tantala/silica dielectric mirror coatings},
	Volume = {20},
	Year = {2003},
	Bdsk-Url-1 = {http://stacks.iop.org/0264-9381/20/i=13/a=334}}

@article{Harry:CQG2002,
	Abstract = {We report on thermal noise from the internal friction of dielectric coatings made from alternating layers of Ta 2 O 5 and SiO 2 deposited on fused silica substrates. We present calculations of the thermal noise in gravitational wave interferometers due to optical coatings, when the material properties of the coating are different from those of the substrate and the mechanical loss angle in the coating is anisotropic. The loss angle in the coatings for strains parallel to the substrate surface was determined from ringdown experiments. We measured the mechanical quality factor of three fused silica samples with coatings deposited on them. The loss angle, ##IMG## [http://ej.iop.org/icons/Entities/phi.gif] {phi} || ( f ), of the coating material for strains parallel to the coated surface was found to be 4.2 $\pm$ 0.3 × 10 −4 for coatings deposited on commercially polished slides, and 1.0 $\pm$ 0.3 × 10 −4 for a coating deposited on a superpolished disc. Using these numbers, we estimate the effect of coatings on thermal noise in the initial LIGO and Advanced LIGO interferometers. We also find that the corresponding prediction for thermal noise in the 40 m LIGO prototype at Caltech is consistent with the noise data. These results are complemented by results for a different type of coating, presented in a companion paper.},
	Author = {Gregory M Harry and Andri M Gretarsson and Peter R Saulson and Scott E Kittelberger and Steven D Penn and William J Startin and Sheila Rowan and Martin M Fejer and D R M Crooks and Gianpietro Cagnoli and Jim Hough and Norio Nakagawa},
	Date-Added = {2011-12-17 04:45:04 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Classical and Quantum Gravity},
	Number = {5},
	Pages = {897},
	Title = {Thermal noise in interferometric gravitational wave detectors due to dielectric optical coatings},
	Volume = {19},
	Year = {2002},
	Bdsk-Url-1 = {http://stacks.iop.org/0264-9381/19/i=5/a=305}}

@article{Pohl:RMP,
	Author = {Pohl, Robert O. and Liu, Xiao and Thompson, EunJoo},
	Date-Added = {2011-12-17 01:33:16 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issue = {4},
	Journal = {Rev. Mod. Phys.},
	Month = {Oct},
	Pages = {991--1013},
	Publisher = {American Physical Society},
	Title = {Low-temperature thermal conductivity and acoustic attenuation in amorphous solids},
	Volume = {74},
	Year = {2002},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/RevModPhys.74.991},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/RevModPhys.74.991}}

@article{Saulson:ThermalNoise,
	Author = {Saulson, Peter R.},
	Date-Added = {2011-12-15 10:00:56 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issue = {8},
	Journal = {Phys. Rev. D},
	Month = {Oct},
	Pages = {2437--2445},
	Publisher = {American Physical Society},
	Rating = {5},
	Title = {Thermal noise in mechanical experiments},
	Volume = {42},
	Year = {1990},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.42.2437},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.42.2437}}

@article{Drever:PR,
	Author = {R. W. P. Drever},
	Date-Added = {2011-12-15 08:11:46 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {AIP Conference Proceedings},
	Number = {1},
	Pages = {336-346},
	Publisher = {AIP},
	Title = {Laser interferometer gravitational radiation detectors},
	Volume = {96},
	Year = {1983},
	Bdsk-Url-1 = {http://link.aip.org/link/?APC/96/336/1},
	Bdsk-Url-2 = {http://dx.doi.org/10.1063/1.33953}}

@article{DHS:Garching,
	Author = {Shoemaker, D. and Schilling, R. and Schnupp, L. and Winkler, W. and Maischberger, K. and R\"udiger, A.},
	Date-Added = {2011-12-15 07:53:42 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issue = {2},
	Journal = {Phys. Rev. D},
	Month = {Jul},
	Pages = {423--432},
	Publisher = {American Physical Society},
	Title = {Noise behavior of the Garching 30-meter prototype gravitational-wave detector},
	Volume = {38},
	Year = {1988},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.38.423},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.38.423}}

@article{Byer:Sagnac,
	Author = {Peter T. Beyersdorf and R. L. Byer and M. M. Fejer},
	Date-Added = {2011-12-15 07:48:20 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Editor = {Sydney Meshkov},
	Journal = {AIP Conference Proceedings},
	Keywords = {gravitational wave detectors; light interferometers; light polarisation; optical delay lines; heterodyne detection; sensitivity},
	Number = {1},
	Pages = {200-203},
	Publisher = {AIP},
	Title = {The polarization Sagnac interferometer as a candidate configuration for an advanced detector},
	Volume = {523},
	Year = {2000},
	Bdsk-Url-1 = {http://link.aip.org/link/?APC/523/200/1},
	Bdsk-Url-2 = {http://dx.doi.org/10.1063/1.1291857}}

@article{Herriott:65,
	Abstract = {A long optical path has been folded between two 7.5-cm diam spherical or aspherical mirrors to provide an output beam which can be well separated from previous reflections with 1000 or more passes between the mirrors. The 3000-m path provides 10 {\textmu}sec of delay. This system can be used as a dispersionless optical delay line for use in filtering or storage of information modulated onto the light beam. The pattern of beams between the two mirrors is obtained in one of two ways. A small perturbing mirror may be inserted to give a series of offset ellipses, or one or both of the mirrors can be made astigmatic to give a Lissajous pattern of spots on each mirror. The output beam can be separated from others by discriminating in both angle and position. The diffraction losses of the system are much lower than those for an open beam because of the periodic focusing of the spherical mirrors. The extreme dependence of the loss of the delay line upon the absorption and scattering loss of the mirrors makes the system depeentupon very low loss mirrors and also makes the system a suitable method for measuring mirror loss.Block diagrams are shown for some possible filtering and storage applications.},
	Author = {Donald R. Herriott and Harry J. Schulte},
	Date-Added = {2011-12-15 07:45:56 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Appl. Opt.},
	Month = {Aug},
	Number = {8},
	Pages = {883--889},
	Publisher = {OSA},
	Title = {Folded Optical Delay Lines},
	Volume = {4},
	Year = {1965},
	Bdsk-Url-1 = {http://ao.osa.org/abstract.cfm?URI=ao-4-8-883},
	Bdsk-Url-2 = {http://dx.doi.org/10.1364/AO.4.000883}}

@article{lrr-2011-5,
	Author = {Matthew Pitkin and Stuart Reid and Sheila Rowan and James Hough},
	Date-Added = {2011-12-14 03:49:42 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Living Reviews in Relativity},
	Keywords = {Gravitational waves, Science runs, Gravitational wave detectors, Noise sources, Data analysis, Interferometric gravitational wave detectors, Laser interferometry},
	Number = {5},
	Title = {Gravitational Wave Detection by Interferometry (Ground and Space)},
	Volume = {14},
	Year = {2011},
	Bdsk-Url-1 = {http://www.livingreviews.org/lrr-2011-5}}

@article{BaWe:PhysToday,
	Author = {B.~Barish and R.~Weiss},
	Date-Added = {2011-12-14 03:34:07 -0800},
	Date-Modified = {2011-12-14 03:35:24 -0800},
	Journal = {Physics Today},
	Keywords = {ligo},
	Number = {10},
	Pages = {44},
	Rating = {4},
	Read = {1},
	Title = {LIGO and the Detection of Gravitational Waves},
	Volume = {52},
	Year = {1999}}

@article{Rai:RMP,
	Author = {Weiss, Rainer},
	Date-Added = {2011-12-14 03:31:52 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issue = {2},
	Journal = {Rev. Mod. Phys.},
	Month = {Mar},
	Pages = {S187--S196},
	Publisher = {American Physical Society},
	Rating = {5},
	Title = {Gravitational radiation},
	Volume = {71},
	Year = {1999},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/RevModPhys.71.S187},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/RevModPhys.71.S187}}

@techreport{Rai:QPR,
	Author = {R.~Weiss},
	Date-Added = {2011-12-14 03:22:27 -0800},
	Date-Modified = {2012-04-29 20:55:12 -0700},
	Institution = {Massachusetts Institute of Technology},
	Journal = {Quarterly Progress Report of the Research Laboratory of Electronics},
	Keywords = {interferometer},
	Rating = {5},
	Read = {1},
	Title = {Electromagnetically Coupled Broadband Gravitational Antenna},
	Url = {{https://dcc.ligo.org/cgi-bin/DocDB/ShowDocument?docid=38618}},
	Year = {1972},
	Bdsk-Url-1 = {%7Bhttps://dcc.ligo.org/cgi-bin/DocDB/ShowDocument?docid=38618%7D}}

@article{Detweiler:PTA,
	Author = {Steven Detweiler},
	Date-Added = {2011-11-28 01:03:23 -0800},
	Date-Modified = {2011-11-28 01:04:49 -0800},
	Journal = {The Astrophysical Journal},
	Keywords = {pulsar timing},
	Rating = {5},
	Read = {1},
	Title = {Pulsar Timing Measurements and the Search for Gravitational Waves},
	Volume = {234},
	Year = {1979}}

@article{Hobbs:IPTA,
	Abstract = {The International Pulsar Timing Array project combines observations of pulsars from both northern and southern hemisphere observatories with the main aim of detecting ultra-low frequency (~ 10 −9 --10 −8 Hz) gravitational waves. Here we introduce the project, review the methods used to search for gravitational waves emitted from coalescing supermassive binary black-hole systems in the centres of merging galaxies and discuss the status of the project.},
	Author = {G Hobbs and A Archibald and Z Arzoumanian and D Backer and M Bailes and N D R Bhat and M Burgay and S Burke-Spolaor and D Champion and I Cognard and W Coles and J Cordes and P Demorest and G Desvignes and R D Ferdman and L Finn and P Freire and M Gonzalez and J Hessels and A Hotan and G Janssen and F Jenet and A Jessner and C Jordan and V Kaspi and M Kramer and V Kondratiev and J Lazio and K Lazaridis and K J Lee and Y Levin and A Lommen and D Lorimer and R Lynch and A Lyne and R Manchester and M McLaughlin and D Nice and S Oslowski and M Pilia and A Possenti and M Purver and S Ransom and J Reynolds and S Sanidas and J Sarkissian and A Sesana and R Shannon and X Siemens and I Stairs and B Stappers and D Stinebring and G Theureau and R van Haasteren and W van Straten and J P W Verbiest and D R B Yardley and X P You},
	Date-Added = {2011-11-28 01:01:18 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Classical and Quantum Gravity},
	Number = {8},
	Pages = {084013},
	Title = {The International Pulsar Timing Array project: using pulsars as a gravitational wave detector},
	Volume = {27},
	Year = {2010},
	Bdsk-Url-1 = {http://stacks.iop.org/0264-9381/27/i=8/a=084013}}

@article{Lorimer:LRR,
	Author = {Duncan R. Lorimer},
	Date-Added = {2011-11-28 00:22:06 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Living Reviews in Relativity},
	Keywords = {pulsars},
	Number = {8},
	Title = {Binary and Millisecond Pulsars},
	Volume = {11},
	Year = {2008},
	Bdsk-Url-1 = {http://www.livingreviews.org/lrr-2008-8}}

@article{Ando:DECIGO,
	Abstract = {A space gravitational-wave antenna, DECIGO (DECI-hertz interferometer Gravitational wave Observatory), will provide fruitful insights into the universe, particularly on the formation mechanism of supermassive black holes, dark energy and the inflation of the universe. In the current pre-conceptual design, DECIGO will be comprising four interferometer units; each interferometer unit will be formed by three drag-free spacecraft with 1000 km separation. Since DECIGO will be an extremely challenging mission with high-precision formation flight with long baseline, it is important to increase the technical feasibility before its planned launch in 2027. Thus, we are planning to launch two milestone missions. DECIGO pathfinder (DPF) is the first milestone mission, and key components for DPF are being tested on ground and in orbit. In this paper, we review the conceptual design and current status of DECIGO and DPF.},
	Author = {Masaki Ando and Seiji Kawamura and Naoki Seto and Shuichi Sato and Takashi Nakamura and Kimio Tsubono and Takeshi Takashima and Ikkoh Funaki and Kenji Numata and Nobuyuki Kanda and Takahiro Tanaka and Kunihito Ioka and Kazuhiro Agatsuma and Koh-suke Aoyanagi and Koji Arai and Akito Araya 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 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 Kiwamu Izumi and Isao Kawano 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 Hiroo Kunimori and Hitoshi Kuninaka and Kazuaki Kuroda and Kei-ichi Maeda and Hideo Matsuhara and Yasushi Mino and Osamu Miyakawa and Umpei Miyamoto and Shinji Miyoki and Mutsuko Y Morimoto and Toshiyuki Morisawa and Shigenori Moriwaki and Shinji Mukohyama and Mitsuru Musha and Shigeo Nagano and Isao Naito and Kouji Nakamura and Masahiro Nakamura and Hiroyuki Nakano and Kenichi Nakao and Shinichi Nakasuka and Yoshinori Nakayama and Kazuhiro Nakazawa 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 Kenshi Okada and Norio Okada and Kenichi Oohara and Norichika Sago and Motoyuki Saijo and Ryo Saito and Masaaki Sakagami and Shin-ichiro Sakai 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 Kent Yagi and Hiroshi Yamakawa and Kazuhiro Yamamoto and Toshitaka Yamazaki and Jun'ichi Yokoyama and Chul-Moon Yoo and Shijun Yoshida and Taizoh Yoshino and Ke-Xun Sun},
	Date-Added = {2011-11-26 17:29:36 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Journal = {Classical and Quantum Gravity},
	Number = {8},
	Pages = {084010},
	Title = {DECIGO and DECIGO pathfinder},
	Volume = {27},
	Year = {2010},
	Bdsk-Url-1 = {http://stacks.iop.org/0264-9381/27/i=8/a=084010}}

@webpage{DECIGO,
	Author = {{DECIGO}},
	Date-Added = {2011-11-26 17:23:25 -0800},
	Date-Modified = {2013-01-03 03:07:59 -0800},
	Title = {{DECIGO} Homepage},
	Url = {http://tamago.mtk.nao.ac.jp/decigo/},
	Year = {2011},
	Bdsk-Url-1 = {http://tamago.mtk.nao.ac.jp/decigo/}}

@webpage{ESA:LISA,
	Author = {{LISA Science Team}},
	Date-Added = {2011-11-26 17:06:38 -0800},
	Date-Modified = {2012-02-17 22:14:01 -0800},
	Keywords = {lisa esa},
	Rating = {2},
	Read = {1},
	Title = {{eLISA} Homepage},
	Url = {http://www.elisa-ngo.org},
	Year = {2012},
	Bdsk-Url-1 = {http://lisa.esa.int},
	Bdsk-Url-2 = {http://www.elisa-ngo.org}}

@article{Faller1989107,
	Author = {J.E. Faller and P.L. Bender and J.L. Hall and D. Hils and R.T. Stebbins and M.A. Vincent},
	Date-Added = {2011-11-26 16:52:08 -0800},
	Date-Modified = {2012-01-22 20:42:00 -0800},
	Issn = {0273-1177},
	Journal = {Advances in Space Research},
	Number = {9},
	Pages = {107 - 111},
	Title = {An antenna for laser gravitational-wave observations in space},
	Volume = {9},
	Year = {1989},
	Bdsk-Url-1 = {http://www.sciencedirect.com/science/article/pii/0273117789900148},
	Bdsk-Url-2 = {http://dx.doi.org/10.1016/0273-1177(89)90014-8}}

@article{Armstrong:SGW,
	Author = {J.~W.~Armstrong and L.~Iess and P.~Tortora and B.~Bertotti},
	Date-Added = {2011-11-21 00:10:44 -0800},
	Date-Modified = {2011-11-21 00:12:45 -0800},
	Journal = {Astrophysical Journal},
	Keywords = {satellite doppler cassini timing},
	Rating = {4},
	Title = {{Stochastic Gravitational Wave Background: Upper Limits in the 10^-6 to 10^-3 Hz Band}},
	Year = {2003}}

@proceedings{Zucker:Gas,
	Address = {Hackensack, N.J.},
	Author = {M.~E.~Zucker and S.~E.~Whitcomb},
	Date-Added = {2011-11-20 03:40:33 -0800},
	Date-Modified = {2014-01-23 08:46:13 +0000},
	Journal = {Proceedings of the Seventh Marcel Grossman Meeting on General Relativity},
	Publisher = {World Scientific},
	Rating = {3},
	Title = {Measurement of Optical Path Fluctuations due to Residual Gas in the LIGO 40 Meter Interferometer},
	Year = {1996}}

@article{TAMA:gas,
	Author = {R.~Takahashi and Y.~Saito and M.~Fukushima and M.~Ando and K.~Arai and D.~Tatsumi and G.~Heinzel and S.~Kawamura and T.~Yamazaki and S.~Moriwaki},
	Date-Added = {2011-11-20 03:39:40 -0800},
	Date-Modified = {2011-11-20 04:04:19 -0800},
	Journal = {Journal of Vacuum Science and Technology A: Vacuum, Surfaces, and Films},
	Keywords = {gas},
	Rating = {3},
	Title = {Direct measurement of residual gas effect on the sensitivity in TAMA300},
	Year = {2002}}

@article{Einstein:1916a,
	Author = {A.~Einstein},
	Date-Added = {2011-11-19 23:26:35 -0800},
	Date-Modified = {2013-03-01 00:20:17 +0000},
	Journal = {Annalen der Physik},
	Rating = {5},
	Read = {1},
	Title = {Grundlage der allgemeinen Relativit{\"a}tstheorie},
	Year = {1916}}

@article{Abu1962,
	Author = {I.~Abubakar},
	Journal = {Math.~Proc.~Cambridge Phil.~Soc.},
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	Volume = {58},
	Year = {1962}}

@article{Abu1963,
	Author = {I.~Abubakar},
	Journal = {Math.~Proc.~Cambridge Phil.~Soc.},
	Pages = {231},
	Title = {{Scattering of plane elastic waves at rough surfaces. II}},
	Volume = {59},
	Year = {1963}}

@article{AcEA2008,
	Author = {F.~Acernese and R.~DeSalvo and J.~Harms and A.~Sajeva and L.~Shaffner and T.~Trancynger},
	Journal = {LIGO DCC},
	Title = {{Seismic stations implementation and improvements at Homestake}},
	Volume = {T080344},
	Year = {2008}}

@article{AcEA2007,
	Author = {{F.~Acernese et al.}},
	Journal = {Class.~Quantum Grav.},
	Pages = {S381},
	Title = {{Status of Virgo detector}},
	Volume = {24},
	Year = {2007}}

@book{AkRi2009,
	Author = {K.~Aki and P.~G.~Richards},
	Publisher = {University Science Books},
	Title = {{Quantitative Seismology, 2nd edition}},
	Year = {2009}}

@article{AlRo1999,
	Author = {B.~Allen and J.~D.~Romano},
	Journal = {Phys.~Rev.~D},
	Pages = {102001},
	Title = {Detecting a stochastic background of gravitational radiation: {S}ignal processing strategies and sensitivities},
	Volume = {59},
	Year = {1999}}

@article{Ama1982,
	Author = {S.-I.~Amari},
	Journal = {Ann.~Stat.},
	Pages = {357},
	Title = {{Differential Geometry of Curved Exponential Families-Curvatures and Information Loss}},
	Volume = {10},
	Year = {1982}}

@article{An1998,
	Author = {N.~Andersson},
	Journal = {ApJ},
	Pages = {708},
	Title = {A new class of unstable modes of rotating relativistic stars},
	Volume = {502},
	Year = {1998}}

@article{AnEA2001,
	Author = {{M.~Ando et al.}},
	Journal = {Phys.~Rev.~Lett.},
	Pages = {3950},
	Title = {{Stable Operation of a 300-m Laser Interferometer with Sufficient Sensitivity to Detect Gravitational-Wave Events within Our Galaxy}},
	Volume = {86},
	Year = {2001}}

@article{ACST1994,
	Author = {T.~A.~Apostolatos and C.~Cutler and G.~J.~Sussman and K.~S.~Thorne},
	Journal = {Phys.~Rev.~D},
	Pages = {6274},
	Title = {Spin-induced orbital precession and its modulation of the gravitational waveforms from merging binaries},
	Volume = {49},
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	Author = {M.~Vallisneri and J.~Crowder and M.~Tinto},
	Date-Modified = {2012-01-22 20:42:01 -0800},
	Title = {Sensitivity and parameter-estimation precision for alternate LISA configurations},
	Year = {2007},
	Bdsk-Url-1 = {arXiv:0710.4369}}

@article{Vec2004,
	Author = {A.~Vecchio},
	Journal = {Phys.~Rev.~D},
	Pages = {042001},
	Title = {{LISA} observations of rapidly spinning massive black hole binary systems},
	Volume = {70},
	Year = {2004}}

@article{VeWi2004,
	Author = {A.~Vecchio and E.~D.~L.~Wickham},
	Journal = {CLASS.~QUANTUM GRAV.},
	Pages = {S661},
	Title = {{LISA} response function and parameter estimation},
	Volume = {21},
	Year = {2004}}

@techreport{aVir2009,
	Author = {{The Virgo Collaboration}},
	Date-Modified = {2014-01-23 08:49:29 +0000},
	Institution = {Virgo},
	Number = {{VIR 027A 09}},
	Title = {{Advanced Virgo Baseline Design}},
	Url = {https://wwwcascina.virgo.infn.it/advirgo/},
	Year = {2009},
	Bdsk-Url-1 = {https://wwwcascina.virgo.infn.it/advirgo/}}

@article{VoTa2003,
	Author = {R.~Voss and T.~M.~Tauris},
	Date-Modified = {2012-04-29 21:20:03 -0700},
	Journal = {Monthly Notices of the Royal Astronomical Society},
	Pages = {1169},
	Title = {Galactic distribution of merging neutron stars and black holes - prospects for short gamma-ray burst progenitors and {LIGO/VIRGO}},
	Volume = {342},
	Year = {2003}}

@article{Vya1998,
	Author = {S.~P.~Vyatchanin},
	Journal = {Phys.~Lett.~A},
	Pages = {201},
	Title = {The estimation of signal force parameters in quantum variation measurement},
	Volume = {239},
	Year = {1998}}

@article{VyMa1993,
	Author = {S.~P.~Vyatchanin and A.~B.~Matsko},
	Journal = {JETP},
	Pages = {218},
	Title = {Quantum limit on force measurements},
	Volume = {77},
	Year = {1993}}

@article{VyMa1996a,
	Author = {S.~P.~Vyatchanin and A.~B.~Matsko},
	Journal = {JETP},
	Pages = {1007},
	Title = {Quantum variational force measurement and the cancellation of nonlinear feedback},
	Volume = {82},
	Year = {1996}}

@article{VyMa1996b,
	Author = {S.~P.~Vyatchanin and A.~B.~Matsko},
	Journal = {JETP},
	Pages = {690},
	Title = {Quantum variational measurements of force and compensation of the nonlinear backaction in an interferometric displacement transducer},
	Volume = {83},
	Year = {1996}}

@article{VyZu1995,
	Author = {S.~P.~Vyatchanin and E.~A.~Zubova},
	Journal = {Phys.~Lett.~A},
	Pages = {269},
	Title = {Quantum variation measurement of a force},
	Volume = {201},
	Year = {1995}}

@article{Wah1987,
	Author = {H.~Wahlquist},
	Journal = {Gen.~Rel.~Gravitation},
	Pages = {1101},
	Title = {The {D}oppler response to gravitational waves from a binary star source},
	Volume = {19},
	Year = {1987}}

@book{WaZu1962,
	Author = {L.~A.~Wainstein and V.~D.~Zubakov},
	Publisher = {Dover},
	Title = {{Extraction of Signals from Noise}},
	Year = {1962}}

@book{WaMi1995,
	Author = {D.~F.~Walls and G.~J.~Milburn},
	Publisher = {Springer},
	Title = {{Quantum Optics}},
	Year = {1995}}

@article{WaSa1996,
	Author = {T.~Watanabe and K.~Sassa},
	Journal = {Int J Rock Mech Min Sci Geomech Abstr},
	Pages = {467},
	Title = {Seismic attenuation tomography and its application to rock mass evaluation},
	Volume = {33},
	Year = {1996}}

@phdthesis{Wat2005,
	Author = {M.~Wathelet},
	School = {{Universit\'e de Li\`ege}},
	Title = {Array recordings of ambient vibrations: surface-wave inversion},
	Year = {2005}}

@article{Wei2002,
	Author = {A.~Weinstein},
	Journal = {CLASS.~QUANTUM GRAV.},
	Pages = {1575},
	Title = {{Advanced LIGO optical configuration and prototyping effort}},
	Volume = {19},
	Year = {2002}}

@article{Wel1967,
	Author = {P.~D.~Welch},
	Journal = {IEEE Transactions on Audio and Electroacoustics},
	Pages = {70},
	Title = {{The Use of Fast Fourier Transform for the Estimation of Power Spectra: A Method Based on Time Averaging Over Short, Modified Periodograms}},
	Volume = {15},
	Year = {1967}}

@article{Wen2003,
	Author = {L.~Wen},
	Journal = {ApJ},
	Pages = {419},
	Title = {On the eccentricity distribution of coalescing black hole binaries driven by the {K}ozai mechanism in globular clusters},
	Volume = {598},
	Year = {2003}}

@article{Whi1962,
	Author = {J.~E.~White},
	Journal = {Geophysics},
	Pages = {327},
	Title = {{ELASTIC WAVES ALONG A CYLINDRICAL BORE}},
	Volume = {27},
	Year = {1962}}

@article{WiEA2002,
	Author = {{Willke et al.}},
	Journal = {CLASS.~QUANTUM GRAV.},
	Pages = {1377},
	Title = {The {GEO} 600 gravitational wave detector},
	Volume = {19},
	Year = {2002}}

@article{WiEA1996,
	Author = {M.~M.~Withers and R.~C.~Aster and C.~J.~Young and E.~P.~Chael},
	Journal = {BSSA},
	Pages = {1507},
	Title = {{High-Frequency Analysis of Seismic Background Noise as a Function of Wind Speed and Shallow Depth}},
	Volume = {86},
	Year = {1996}}

@book{WCC1995,
	Author = {{Woodward-Clyde Consultants}},
	Publisher = {Livingston, Louisiana},
	Title = {{Geotechnical Investigation of the LIGO site}},
	Year = {1995}}

@phdthesis{Wu1962,
	Author = {R.-S.~Wu},
	School = {{Massachusetts Institute of Technology}},
	Title = {Seismic wave scattering and the small scale inhomogeneities in the lithosphere},
	Year = {1962}}

@book{Yo1999,
	Author = {I.~R.~Young},
	Publisher = {Elsevier},
	Title = {Wind generated ocean waves},
	Year = {1999}}

@article{Yue1976,
	Author = {H.~P.~Yuen},
	Journal = {Phys.~Rev.~A},
	Pages = {2226},
	Title = {Two-photon coherent states of the radiation field},
	Volume = {13},
	Year = {1976}}

@article{ZFG1990,
	Author = {W.-M.~Zhang and D.~H.~Feng and R.~Gilmore},
	Journal = {Rev.~Mod.~Phys.},
	Pages = {867},
	Title = {Coherent states: Theory and some application},
	Volume = {62},
	Year = {1990}}

@article{Zha2006,
	Author = {W.~Zhao},
	Date-Modified = {2012-01-22 20:42:01 -0800},
	Title = {Improved calculation of relic gravitational waves},
	Year = {2006},
	Bdsk-Url-1 = {arXiv:gr-qc/0612041}}

@article{Aso2004,
	Author = {Y.~Aso},
	Date-Modified = {2011-12-31 13:09:26 -0800},
	Journal = {Phys.~Lett.~A},
	Rating = {4},
	Title = {Stabilization of a {F}abry-{P}\'erot interferometer using a {S}uspension-{P}oint {I}nterferometer},
	Volume = {327},
	Year = {2004}}

@article{Num2008,
	Author = {K.~Numata and J.~Camp},
	Journal = {Applied Optics},
	Title = {Interferometric testbed for nanometer level stabilization of environmental motion over long time scales},
	Year = {2008}}

@article{Mik2006,
	Author = {Mikhailov, Eugeniy E. and Goda, Keisuke and Corbitt, Thomas and Mavalvala, Nergis},
	Date-Modified = {2012-01-22 20:42:01 -0800},
	Issue = {5},
	Journal = {Phys. Rev. A},
	Month = {May},
	Numpages = {5},
	Pages = {053810},
	Publisher = {American Physical Society},
	Title = {Frequency-dependent squeeze-amplitude attenuation and squeeze-angle rotation by electromagnetically induced transparency for gravitational-wave interferometers},
	Volume = {73},
	Year = {2006},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevA.73.053810},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevA.73.053810}}

@article{Gro2013,
	Adsnote = {Provided by the SAO/NASA Astrophysics Data System},
	Adsurl = {http://adsabs.harvard.edu/abs/2013PhRvL.110r1101G},
	Archiveprefix = {arXiv},
	Author = {{Grote}, H. and {Danzmann}, K. and {Dooley}, K.~L. and {Schnabel}, R. and {Slutsky}, J. and {Vahlbruch}, H.},
	Doi = {10.1103/PhysRevLett.110.181101},
	Eid = {181101},
	Eprint = {1302.2188},
	Journal = {Physical Review Letters},
	Keywords = {Gravitational wave detectors and experiments, Quantum fluctuations quantum noise and quantum jumps, Gravitational radiation detectors, mass spectrometers, and other instrumentation and techniques, Interferometry},
	Month = may,
	Number = 18,
	Pages = {181101},
	Primaryclass = {physics.ins-det},
	Title = {{First Long-Term Application of Squeezed States of Light in a Gravitational-Wave Observatory}},
	Volume = 110,
	Year = 2013,
	Bdsk-Url-1 = {http://dx.doi.org/10.1103/PhysRevLett.110.181101}}

@article{Vah2008,
	Author = {Vahlbruch, Henning and Mehmet, Moritz and Chelkowski, Simon and Hage, Boris and Franzen, Alexander and Lastzka, Nico and Go\ss{}ler, Stefan and Danzmann, Karsten and Schnabel, Roman},
	Doi = {10.1103/PhysRevLett.100.033602},
	Issue = {3},
	Journal = {Phys. Rev. Lett.},
	Month = {Jan},
	Numpages = {4},
	Pages = {033602},
	Publisher = {American Physical Society},
	Title = {Observation of Squeezed Light with 10-dB Quantum-Noise Reduction},
	Url = {http://link.aps.org/doi/10.1103/PhysRevLett.100.033602},
	Volume = {100},
	Year = {2008},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevLett.100.033602},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevLett.100.033602}}

@article{Mehmet:2011je,
	Archiveprefix = {arXiv},
	Author = {Mehmet, Moritz and Ast, Stefan and Eberle, Tobias and Steinlechner, Sebastian and Vahlbruch, Henning and others},
	Eprint = {1110.3737},
	Primaryclass = {quant-ph},
	Slaccitation = {%%CITATION = ARXIV:1110.3737;%%},
	Title = {{Squeezed light at 1550 nm with a quantum noise reduction of 12.3 dB}},
	Year = {2011}}

@article{PhysRevA.71.013806,
	Author = {Chelkowski, Simon and Vahlbruch, Henning and Hage, Boris and Franzen, Alexander and Lastzka, Nico and Danzmann, Karsten and Schnabel, Roman},
	Doi = {10.1103/PhysRevA.71.013806},
	Issue = {1},
	Journal = {Phys. Rev. A},
	Month = {Jan},
	Numpages = {8},
	Pages = {013806},
	Publisher = {American Physical Society},
	Title = {Experimental characterization of frequency-dependent squeezed light},
	Url = {http://link.aps.org/doi/10.1103/PhysRevA.71.013806},
	Volume = {71},
	Year = {2005},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevA.71.013806},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevA.71.013806}}

@article{Isogai2013,
	Abstract = {Long-storage-time Fabry-Perot cavities are a core component of many precision measurementexperiments. Optical loss in such cavities is a critical parameter in determining their performance;however, it is very difficult to determine a priori from independent characterisation of theindividual cavity mirrors. Here, we summarise three techniques for directly measuring this loss insitu and apply them to a high-finesse, near-concentric, 2 m system. Through small modifications ofthe cavity\&\#x02019;s length, we explore optical loss as a function of beam spot size over the1\&\#x02013;3 mm range. In this regime we find that optical loss is relatively constant at around 5ppm per mirror and shows greater dependence on the positions of the beam spots on the cavity opticsthan on their size. These results have immediate consequences for the application of squeezed lightto advanced gravitational-wave interferometers.},
	Author = {T. Isogai and J. Miller and P. Kwee and L. Barsotti and M. Evans},
	Date-Modified = {2015-09-28 00:00:00 +0000},
	Doi = {10.1364/OE.21.030114},
	Journal = {Opt. Express},
	Keywords = {Fabry-Perot; Interferometry; Scattering},
	Month = {Dec},
	Number = {24},
	Pages = {30114--30125},
	Publisher = {OSA},
	Title = {Loss in long-storage-time optical cavities},
	Url = {http://www.opticsexpress.org/abstract.cfm?URI=oe-21-24-30114},
	Volume = {21},
	Year = {2013},
	Bdsk-Url-1 = {http://www.opticsexpress.org/abstract.cfm?URI=oe-21-24-30114},
	Bdsk-Url-2 = {http://dx.doi.org/10.1364/OE.21.030114}}

@article{Dwyer:13,
	Abstract = {Squeezed states of light are an important tool for optical measurements below the shot noise limit and for optical realizations of quantum information systems. Recently, squeezed vacuum states were deployed to enhance the shot noise limited performance of gravitational wave detectors. In most practical implementations of squeezing enhancement, relative fluctuations between the squeezed quadrature angle and the measured quadrature (sometimes called squeezing angle jitter or phase noise) are one limit to the noise reduction that can be achieved. We present calculations of several effects that lead to quadrature fluctuations, and use these estimates to account for the observed quadrature fluctuations in a LIGO gravitational wave detector. We discuss the implications of this work for quantum enhanced advanced detectors and even more sensitive third generation detectors.},
	Author = {S. Dwyer and L. Barsotti and S. S. Y. Chua and M. Evans and M. Factourovich and D. Gustafson and T. Isogai and K. Kawabe and A. Khalaidovski and P. K. Lam and M. Landry and N. Mavalvala and D. E. McClelland and G. D. Meadors and C. M. Mow-Lowry and R. Schnabel and R. M. S. Schofield and N. Smith-Lefebvre and M. Stefszky and C. Vorvick and D. Sigg},
	Doi = {10.1364/OE.21.019047},
	Journal = {Opt. Express},
	Keywords = {Interferometry; Parametric oscillators and amplifiers; Fluctuations, relaxations, and noise; Squeezed states; Astronomy and astrophysics},
	Month = {Aug},
	Number = {16},
	Pages = {19047--19060},
	Publisher = {OSA},
	Title = {Squeezed quadrature fluctuations in a gravitational wave detector using squeezed light},
	Url = {http://www.opticsexpress.org/abstract.cfm?URI=oe-21-16-19047},
	Volume = {21},
	Year = {2013},
	Bdsk-Url-1 = {http://www.opticsexpress.org/abstract.cfm?URI=oe-21-16-19047},
	Bdsk-Url-2 = {http://dx.doi.org/10.1364/OE.21.019047}}

@article{Eva2013,
	Author = {Evans, M. and Barsotti, L. and Kwee, P. and Harms, J. and Miao, H.},
	Doi = {10.1103/PhysRevD.88.022002},
	Issue = {2},
	Journal = {Phys. Rev. D},
	Month = {Jul},
	Numpages = {7},
	Pages = {022002},
	Publisher = {American Physical Society},
	Title = {Realistic filter cavities for advanced gravitational wave detectors},
	Url = {http://link.aps.org/doi/10.1103/PhysRevD.88.022002},
	Volume = {88},
	Year = {2013},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.88.022002},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.88.022002}}

@article{Kha2010,
	Author = {Khalili, F. Ya.},
	Doi = {10.1103/PhysRevD.81.122002},
	Issue = {12},
	Journal = {Phys. Rev. D},
	Month = {Jun},
	Numpages = {11},
	Pages = {122002},
	Publisher = {American Physical Society},
	Title = {Optimal configurations of filter cavity in future gravitational-wave detectors},
	Url = {http://link.aps.org/doi/10.1103/PhysRevD.81.122002},
	Volume = {81},
	Year = {2010},
	Bdsk-Url-1 = {http://link.aps.org/doi/10.1103/PhysRevD.81.122002},
	Bdsk-Url-2 = {http://dx.doi.org/10.1103/PhysRevD.81.122002}}

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@article{Harris2021:Perspective,
	Author = {Jesse A. Harris},
	Date-Modified = {2021-01-08 22:58:47 -0800},
	Journal = {Frontiers in Psychology},
	Keywords = {perspective, free indirect discourse, discourse	},
	Number = {},
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	Title = {Extended perspective shift and discourse economy in language processing},
	Volume = {},
	Year = {2021}}


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inherit autotools opendreambox-git lib_package pkgconfig

repository: opendreambox/opendreambox

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text:
@inproceedings{bowyer2019human,
 author = {Bowyer, Alex and Wilson, Rob and Wheater, Stuart and Snape, Matthew and Montague, Kyle},
 booktitle = {Extended Abstracts of the 2019 CHI Conference on Human Factors in Computing Systems},
 organization = {ACM},
 pages = {LBW2320},
 title = {Human-Data Interaction in the Context of Care: Co-designing Family Civic Data Interfaces and Practices},
 year = {2019}
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