Status of the GEO600 gravitational wave detector

B. Willke; P. Aufmuth; C. Aulbert; S. Babak; R. Balasubramanian; B. W. Barr; S. Berukoff; S. Bose; G. Cagnoli; M. M. Casey; D. Churches; C. N. Colacino; D. R.M. Crooks; C. Cutler; K. Danzmann; R. Davies; R. Dupuis; E. Elliffe; C. Fallnich; A. Freise; S. Goßler; A. Grant; H. Grote; J. Harms; G. Heinzel; S. Herden; A. Hepstonstall; M. Heurs; M. Hewitson; J. Hough; O. Jennrich; K. Kawabe; K. Kötter; V. Leonhardt; H. Lück; M. Malec; P. W. McNamara; K. Mossavi; S. Mohanty; S. Mukherjee; S. Nagano; G. P. Newton; B. J. Owen; M. A. Papa; M. V. Plissi; V. Quetschke; L. Ribichini; D. I. Robertson; N. A. Robertson; S. Rowan; A. Rüdiger; B. S. Sathyaprakash; R. Schilling; B. F. Schutz; F. Seifert; A. M. Sintes; K. D. Skeldon; P. Sneddon; K. A. Strain; I. Taylor; C. I. Torrie; A. Vecchio; H. Ward; U. Weiland; H. Welling; P. Williams; W. Winkler; G. Woan; I. Zawischa

doi:10.1117/12.459095

Status of the GEO600 gravitational wave detector

B. Willke
, P. Aufmuth
, C. Aulbert
, S. Babak
, R. Balasubramanian
, B. W. Barr
, S. Berukoff
, S. Bose
, G. Cagnoli
, M. M. Casey
, D. Churches
, C. N. Colacino
, D. R.M. Crooks
, C. Cutler
, K. Danzmann
, R. Davies
, R. Dupuis
, E. Elliffe
, C. Fallnich
, A. Freise

S. Goßler, A. Grant, H. Grote, J. Harms, G. Heinzel, S. Herden, A. Hepstonstall, M. Heurs, M. Hewitson, J. Hough, O. Jennrich, K. Kawabe, K. Kötter, V. Leonhardt, H. Lück, M. Malec, P. W. McNamara, K. Mossavi, S. Mohanty, S. Mukherjee, S. Nagano, G. P. Newton, B. J. Owen, M. A. Papa, M. V. Plissi, V. Quetschke, L. Ribichini, D. I. Robertson, N. A. Robertson, S. Rowan, A. Rüdiger, B. S. Sathyaprakash, R. Schilling, B. F. Schutz, F. Seifert, A. M. Sintes, K. D. Skeldon, P. Sneddon, K. A. Strain, I. Taylor, C. I. Torrie, A. Vecchio, H. Ward, U. Weiland, H. Welling, P. Williams, W. Winkler, G. Woan, I. Zawischa

Research output: Contribution to journal › Conference article › peer-review

Abstract

The GE0600 laser interferometric gravitational wave detector is approaching the end of its commissioning phase which started in 1995. During a test run in January 2002 the detector was operated for 15 days in a power-recycled michelson configuration. The detector and environmental data which were acquired during this test run were used to test the data analysis code. This paper describes the subsystems of GE0600: the status of the detector by August 2002 and the plans towards the first science run.

Original language	English (US)
Pages (from-to)	238-246
Number of pages	9
Journal	Proceedings of SPIE - The International Society for Optical Engineering
Volume	4856
DOIs	https://doi.org/10.1117/12.459095
State	Published - 2002
Event	Gravitational - Wave Detection - Waikoloa, HI, United States Duration: Aug 23 2002 → Aug 25 2002

All Science Journal Classification (ASJC) codes

Electronic, Optical and Magnetic Materials
Condensed Matter Physics
Computer Science Applications
Applied Mathematics
Electrical and Electronic Engineering

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10.1117/12.459095

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Willke, B., Aufmuth, P., Aulbert, C., Babak, S., Balasubramanian, R., Barr, B. W., Berukoff, S., Bose, S., Cagnoli, G., Casey, M. M., Churches, D., Colacino, C. N., Crooks, D. R. M., Cutler, C., Danzmann, K., Davies, R., Dupuis, R., Elliffe, E., Fallnich, C., ... Zawischa, I. (2002). Status of the GEO600 gravitational wave detector. Proceedings of SPIE - The International Society for Optical Engineering, 4856, 238-246. https://doi.org/10.1117/12.459095

@article{5a0b812d05984479b04227cf1ce0ef68,

title = "Status of the GEO600 gravitational wave detector",

abstract = "The GE0600 laser interferometric gravitational wave detector is approaching the end of its commissioning phase which started in 1995. During a test run in January 2002 the detector was operated for 15 days in a power-recycled michelson configuration. The detector and environmental data which were acquired during this test run were used to test the data analysis code. This paper describes the subsystems of GE0600: the status of the detector by August 2002 and the plans towards the first science run.",

author = "B. Willke and P. Aufmuth and C. Aulbert and S. Babak and R. Balasubramanian and Barr, \{B. W.\} and S. Berukoff and S. Bose and G. Cagnoli and Casey, \{M. M.\} and D. Churches and Colacino, \{C. N.\} and Crooks, \{D. R.M.\} and C. Cutler and K. Danzmann and R. Davies and R. Dupuis and E. Elliffe and C. Fallnich and A. Freise and S. Go{\ss}ler and A. Grant and H. Grote and J. Harms and G. Heinzel and S. Herden and A. Hepstonstall and M. Heurs and M. Hewitson and J. Hough and O. Jennrich and K. Kawabe and K. K{\"o}tter and V. Leonhardt and H. L{\"u}ck and M. Malec and McNamara, \{P. W.\} and K. Mossavi and S. Mohanty and S. Mukherjee and S. Nagano and Newton, \{G. P.\} and Owen, \{B. J.\} and Papa, \{M. A.\} and Plissi, \{M. V.\} and V. Quetschke and L. Ribichini and Robertson, \{D. I.\} and Robertson, \{N. A.\} and S. Rowan and A. R{\"u}diger and Sathyaprakash, \{B. S.\} and R. Schilling and Schutz, \{B. F.\} and F. Seifert and Sintes, \{A. M.\} and Skeldon, \{K. D.\} and P. Sneddon and Strain, \{K. A.\} and I. Taylor and Torrie, \{C. I.\} and A. Vecchio and H. Ward and U. Weiland and H. Welling and P. Williams and W. Winkler and G. Woan and I. Zawischa",

year = "2002",

doi = "10.1117/12.459095",

language = "English (US)",

volume = "4856",

pages = "238--246",

journal = "Proceedings of SPIE - The International Society for Optical Engineering",

issn = "0277-786X",

publisher = "SPIE",

note = "Gravitational - Wave Detection ; Conference date: 23-08-2002 Through 25-08-2002",

}

Willke, B, Aufmuth, P, Aulbert, C, Babak, S, Balasubramanian, R, Barr, BW, Berukoff, S, Bose, S, Cagnoli, G, Casey, MM, Churches, D, Colacino, CN, Crooks, DRM, Cutler, C, Danzmann, K, Davies, R, Dupuis, R, Elliffe, E, Fallnich, C, Freise, A, Goßler, S, Grant, A, Grote, H, Harms, J, Heinzel, G, Herden, S, Hepstonstall, A, Heurs, M, Hewitson, M, Hough, J, Jennrich, O, Kawabe, K, Kötter, K, Leonhardt, V, Lück, H, Malec, M, McNamara, PW, Mossavi, K, Mohanty, S, Mukherjee, S, Nagano, S, Newton, GP, Owen, BJ, Papa, MA, Plissi, MV, Quetschke, V, Ribichini, L, Robertson, DI, Robertson, NA, Rowan, S, Rüdiger, A, Sathyaprakash, BS, Schilling, R, Schutz, BF, Seifert, F, Sintes, AM, Skeldon, KD, Sneddon, P, Strain, KA, Taylor, I, Torrie, CI, Vecchio, A, Ward, H, Weiland, U, Welling, H, Williams, P, Winkler, W, Woan, G & Zawischa, I 2002, 'Status of the GEO600 gravitational wave detector', Proceedings of SPIE - The International Society for Optical Engineering, vol. 4856, pp. 238-246. https://doi.org/10.1117/12.459095

TY - JOUR

T1 - Status of the GEO600 gravitational wave detector

AU - Willke, B.

AU - Aufmuth, P.

AU - Aulbert, C.

AU - Babak, S.

AU - Balasubramanian, R.

AU - Barr, B. W.

AU - Berukoff, S.

AU - Bose, S.

AU - Cagnoli, G.

AU - Casey, M. M.

AU - Churches, D.

AU - Colacino, C. N.

AU - Crooks, D. R.M.

AU - Cutler, C.

AU - Danzmann, K.

AU - Davies, R.

AU - Dupuis, R.

AU - Elliffe, E.

AU - Fallnich, C.

AU - Freise, A.

AU - Goßler, S.

AU - Grant, A.

AU - Grote, H.

AU - Harms, J.

AU - Heinzel, G.

AU - Herden, S.

AU - Hepstonstall, A.

AU - Heurs, M.

AU - Hewitson, M.

AU - Hough, J.

AU - Jennrich, O.

AU - Kawabe, K.

AU - Kötter, K.

AU - Leonhardt, V.

AU - Lück, H.

AU - Malec, M.

AU - McNamara, P. W.

AU - Mossavi, K.

AU - Mohanty, S.

AU - Mukherjee, S.

AU - Nagano, S.

AU - Newton, G. P.

AU - Owen, B. J.

AU - Papa, M. A.

AU - Plissi, M. V.

AU - Quetschke, V.

AU - Ribichini, L.

AU - Robertson, D. I.

AU - Robertson, N. A.

AU - Rowan, S.

AU - Rüdiger, A.

AU - Sathyaprakash, B. S.

AU - Schilling, R.

AU - Schutz, B. F.

AU - Seifert, F.

AU - Sintes, A. M.

AU - Skeldon, K. D.

AU - Sneddon, P.

AU - Strain, K. A.

AU - Taylor, I.

AU - Torrie, C. I.

AU - Vecchio, A.

AU - Ward, H.

AU - Weiland, U.

AU - Welling, H.

AU - Williams, P.

AU - Winkler, W.

AU - Woan, G.

AU - Zawischa, I.

PY - 2002

Y1 - 2002

N2 - The GE0600 laser interferometric gravitational wave detector is approaching the end of its commissioning phase which started in 1995. During a test run in January 2002 the detector was operated for 15 days in a power-recycled michelson configuration. The detector and environmental data which were acquired during this test run were used to test the data analysis code. This paper describes the subsystems of GE0600: the status of the detector by August 2002 and the plans towards the first science run.

AB - The GE0600 laser interferometric gravitational wave detector is approaching the end of its commissioning phase which started in 1995. During a test run in January 2002 the detector was operated for 15 days in a power-recycled michelson configuration. The detector and environmental data which were acquired during this test run were used to test the data analysis code. This paper describes the subsystems of GE0600: the status of the detector by August 2002 and the plans towards the first science run.

UR - https://www.scopus.com/pages/publications/0038530851

UR - https://www.scopus.com/pages/publications/0038530851#tab=citedBy

U2 - 10.1117/12.459095

DO - 10.1117/12.459095

M3 - Conference article

AN - SCOPUS:0038530851

SN - 0277-786X

VL - 4856

SP - 238

EP - 246

JO - Proceedings of SPIE - The International Society for Optical Engineering

JF - Proceedings of SPIE - The International Society for Optical Engineering

T2 - Gravitational - Wave Detection

Y2 - 23 August 2002 through 25 August 2002

ER -

Status of the GEO600 gravitational wave detector

Abstract

All Science Journal Classification (ASJC) codes

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