Second-generation laser interferometry for gravitational wave detection: ACIGA progress

D. E. McClelland; S. M. Scott; M. B. Gray; D. A. Shaddock; B. J. Slagmolen; A. Searle; D. G. Blair; L. Ju; J. Winterflood; F. Benabid; M. Baker; J. Munch; P. J. Veitch; M. W. Hamilton; M. Ostermeyer; D. Mudge; D. Ottaway; C. Hollitt

doi:10.1088/0264-9381/18/19/321

Second-generation laser interferometry for gravitational wave detection: ACIGA progress

D. E. McClelland^*, S. M. Scott, M. B. Gray, D. A. Shaddock, B. J. Slagmolen, A. Searle, D. G. Blair, L. Ju, J. Winterflood, F. Benabid, M. Baker, J. Munch, P. J. Veitch, M. W. Hamilton, M. Ostermeyer, D. Mudge, D. Ottaway, C. Hollitt

^*Corresponding author for this work

Research output: Contribution to journal › Article › peer-review

6 Citations (Scopus)

Abstract

Reasonable event rate gravitational wave astronomy in the audio frequency detection band will require improving the sensitivity of long-baseline interferometer-based gravitational wave detectors currently under construction by at least a factor of 10. In this summary we report research being carried out by the Australian Consortium for Interferometric Gravitational Astronomy towards this end.

Original language	English
Pages (from-to)	4121-4126
Number of pages	6
Journal	Classical and Quantum Gravity
Volume	18
Issue number	19
DOIs	https://doi.org/10.1088/0264-9381/18/19/321
Publication status	Published - 7 Oct 2001

Access to Document

10.1088/0264-9381/18/19/321

Cite this

McClelland, D. E., Scott, S. M., Gray, M. B., Shaddock, D. A., Slagmolen, B. J., Searle, A., Blair, D. G., Ju, L., Winterflood, J., Benabid, F., Baker, M., Munch, J., Veitch, P. J., Hamilton, M. W., Ostermeyer, M., Mudge, D., Ottaway, D., & Hollitt, C. (2001). Second-generation laser interferometry for gravitational wave detection: ACIGA progress. Classical and Quantum Gravity, 18(19), 4121-4126. https://doi.org/10.1088/0264-9381/18/19/321

@article{2234494a98404046a59ed5aab2312bf6,

title = "Second-generation laser interferometry for gravitational wave detection: ACIGA progress",

abstract = "Reasonable event rate gravitational wave astronomy in the audio frequency detection band will require improving the sensitivity of long-baseline interferometer-based gravitational wave detectors currently under construction by at least a factor of 10. In this summary we report research being carried out by the Australian Consortium for Interferometric Gravitational Astronomy towards this end.",

author = "McClelland, {D. E.} and Scott, {S. M.} and Gray, {M. B.} and Shaddock, {D. A.} and Slagmolen, {B. J.} and A. Searle and Blair, {D. G.} and L. Ju and J. Winterflood and F. Benabid and M. Baker and J. Munch and Veitch, {P. J.} and Hamilton, {M. W.} and M. Ostermeyer and D. Mudge and D. Ottaway and C. Hollitt",

year = "2001",

month = oct,

day = "7",

doi = "10.1088/0264-9381/18/19/321",

language = "English",

volume = "18",

pages = "4121--4126",

journal = "Classical and Quantum Gravity",

issn = "0264-9381",

publisher = "IOP Publishing Ltd.",

number = "19",

}

McClelland, DE , Scott, SM , Gray, MB , Shaddock, DA , Slagmolen, BJ, Searle, A, Blair, DG, Ju, L, Winterflood, J, Benabid, F, Baker, M, Munch, J, Veitch, PJ, Hamilton, MW, Ostermeyer, M, Mudge, D, Ottaway, D & Hollitt, C 2001, 'Second-generation laser interferometry for gravitational wave detection: ACIGA progress', Classical and Quantum Gravity, vol. 18, no. 19, pp. 4121-4126. https://doi.org/10.1088/0264-9381/18/19/321

TY - JOUR

T1 - Second-generation laser interferometry for gravitational wave detection

T2 - ACIGA progress

AU - McClelland, D. E.

AU - Scott, S. M.

AU - Gray, M. B.

AU - Shaddock, D. A.

AU - Slagmolen, B. J.

AU - Searle, A.

AU - Blair, D. G.

AU - Ju, L.

AU - Winterflood, J.

AU - Benabid, F.

AU - Baker, M.

AU - Munch, J.

AU - Veitch, P. J.

AU - Hamilton, M. W.

AU - Ostermeyer, M.

AU - Mudge, D.

AU - Ottaway, D.

AU - Hollitt, C.

PY - 2001/10/7

Y1 - 2001/10/7

N2 - Reasonable event rate gravitational wave astronomy in the audio frequency detection band will require improving the sensitivity of long-baseline interferometer-based gravitational wave detectors currently under construction by at least a factor of 10. In this summary we report research being carried out by the Australian Consortium for Interferometric Gravitational Astronomy towards this end.

AB - Reasonable event rate gravitational wave astronomy in the audio frequency detection band will require improving the sensitivity of long-baseline interferometer-based gravitational wave detectors currently under construction by at least a factor of 10. In this summary we report research being carried out by the Australian Consortium for Interferometric Gravitational Astronomy towards this end.

UR - http://www.scopus.com/inward/record.url?scp=0035538536&partnerID=8YFLogxK

U2 - 10.1088/0264-9381/18/19/321

DO - 10.1088/0264-9381/18/19/321

M3 - Article

SN - 0264-9381

VL - 18

SP - 4121

EP - 4126

JO - Classical and Quantum Gravity

JF - Classical and Quantum Gravity

IS - 19

ER -

Second-generation laser interferometry for gravitational wave detection: ACIGA progress

Abstract

Access to Document

Other files and links

Fingerprint

Cite this