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Detector description and performance for the first coincidence observations between LIGO and GEO

✍ Scribed by B. Abbott; R. Abbott; R. Adhikari; A. Ageev; B. Allen; R. Amin; S.B. Anderson; W.G. Anderson; M. Araya; H. Armandula; F. Asiri; P. Aufmuth; C. Aulbert; S. Babak; R. Balasubramanian; S. Ballmer; B.C. Barish; D. Barker; C. Barker-Patton; M. Barnes; B. Barr; M.A. Barton; K. Bayer; R. Beausoleil; K. Belczynski; R. Bennett; S.J. Berukoff; J. Betzwieser; B. Bhawal; I.A. Bilenko; G. Billingsley; E. Black; K. Blackburn; B. Bland-Weaver; B. Bochner; L. Bogue; R. Bork; S. Bose; P.R. Brady; V.B. Braginsky; J.E. Brau; D.A. Brown; S. Brozek; A. Bullington; A. Buonanno; R. Burgess; D. Busby; W.E. Butler; R.L. Byer; L. Cadonati; G. Cagnoli; J.B. Camp; C.A. Cantley; L. Cardenas; K. Carter; M.M. Casey; J. Castiglione; A. Chandler; J. Chapsky; P. Charlton; S. Chatterji; Y. Chen; V. Chickarmane; D. Chin; N. Christensen; D. Churches; C. Colacino; R. Coldwell; M. Coles; D. Cook; T. Corbitt; D. Coyne; J.D.E. Creighton; T.D. Creighton; D.R.M. Crooks; P. Csatorday; B.J. Cusack; C. Cutler; E. D'Ambrosio; K. Danzmann; R. Davies; E. Daw; D. DeBra; T. Delker; R. DeSalvo; S. Dhurandar; M. Dı́az; H. Ding; R.W.P. Drever; R.J. Dupuis; C. Ebeling; J. Edlund; P. Ehrens; E.J. Elliffe; T. Etzel; M. Evans; T. Evans; C. Fallnich; D. Farnham; M.M. Fejer; M. Fine; L.S. Finn; É. Flanagan; A. Freise; R. Frey; P. Fritschel; V. Frolov; M. Fyffe; K.S. Ganezer; J.A. Giaime; A. Gillespie; K. Goda; G. González; S. Goßler; P. Grandclément; A. Grant; C. Gray; A.M. Gretarsson; D. Grimmett; H. Grote; S. Grunewald; M. Guenther; E. Gustafson; R. Gustafson; W.O. Hamilton; M. Hammond; J. Hanson; C. Hardham; G. Harry; A. Hartunian; J. Heefner; Y. Hefetz; G. Heinzel; I.S. Heng; M. Hennessy; N. Hepler; A. Heptonstall; M. Heurs; M. Hewitson; N. Hindman; P. Hoang; J. Hough; M. Hrynevych; W. Hua; R. Ingley; M. Ito; Y. Itoh; A. Ivanov; O. Jennrich; W.W. Johnson; W. Johnston; L. Jones; D. Jungwirth; V. Kalogera; E. Katsavounidis; K. Kawabe; S. Kawamura; W. Kells; J. Kern; A. Khan; S. Killbourn; C.J. Killow; C. Kim; C. King; P. K


Book ID
104067835
Publisher
Elsevier Science
Year
2004
Tongue
English
Weight
904 KB
Volume
517
Category
Article
ISSN
0168-9002

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✦ Synopsis


For 17 days in August and September 2002, the LIGO and GEO interferometer gravitational wave detectors were operated in coincidence to produce their first data for scientific analysis. Although the detectors were still far from their design sensitivity levels, the data can be used to place better upper limits on the flux of gravitational waves incident on the earth than previous direct measurements. This paper describes the instruments and the data in some detail, as a companion to analysis papers based on the first data.


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Description of an observational method f
✍ J. Houtgast 📂 Article 📅 1970 🏛 Springer 🌐 English ⚖ 731 KB

The results of measurements of absolute intensities in the spectrum of the centre of the sun's disk in the wavelength region 2977-4087/~ have already been published (Houtgast 1965(Houtgast , 1968) and use has been made of them on different occasions. The intensities at 206 spectral points have been