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Niobe was a ground-based, cryogenic resonant bar gravitational-wave detector. The detector used a microwave parametric transducer readout to improve noise performance and detector bandwidth.^[1] The detector was run by David Blair at University of Western Australia in Perth. The detector ran in joint science runs from 1993-1998 with the gravitational-wave detectors Auriga, Allegro, Explorer and Nautillus.^[1]

References

^ ^a ^b Aguiar, Odylio Denys (December 2010). "Past, present and future of the Resonant-Mass gravitational wave detectors". Research in Astronomy and Astrophysics. 11 (1): 1–42. arXiv:1009.1138. doi:10.1088/1674-4527/11/1/001. ISSN 1674-4527. S2CID 250693208.

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[:0-1] Aguiar, Odylio Denys (December 2010). "Past, present and future of the Resonant-Mass gravitational wave detectors". Research in Astronomy and Astrophysics. 11 (1): 1–42. arXiv:1009.1138. doi:10.1088/1674-4527/11/1/001. ISSN 1674-4527. S2CID 250693208.

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+{{Short description|Gravitational-wave detector}}
+{{Use dmy dates|date=April 2022}}
+[[File:Gravitational-wave detector NIOBE on display at the Gravity Discovery Centre, September 2021 01.jpg|thumb|240px|NIOBE on display at the [[Gravity Discovery Centre]]]]
+'''Niobe''' was a ground-based, cryogenic resonant bar [[gravitational-wave detector]].  The detector used a microwave parametric transducer readout to improve noise performance and detector bandwidth.<ref name=":0">{{cite journal |last1=Aguiar |first1=Odylio Denys |title=Past, present and future of the Resonant-Mass gravitational wave detectors |journal=Research in Astronomy and Astrophysics |date=December 2010 |volume=11 |issue=1 |pages=1–42 |doi=10.1088/1674-4527/11/1/001 |language=en |issn=1674-4527|arxiv=1009.1138 |s2cid=250693208 }}</ref> The detector was run by [[David Blair (physicist)|David Blair]] at [[University of Western Australia]] in [[Perth]]. The detector ran in joint science runs from 1993-1998 with the gravitational-wave detectors [[AURIGA|Auriga]], [[Allegro gravitational-wave detector|Allegro]], [[Explorer]] and [[Nautillus]].<ref name=":0" />
+== See also ==
-'''Niobe''' was a ground-based, cryogenic resonant bar [[gravitational-wave detector]].  The detector used a microwave parametric transducer readout to improve noise performance and detector bandwidth.<ref name=":0">{{cite journal |last1=Aguiar |first1=Odylio Denys |title=Past, present and future of the Resonant-Mass gravitational wave detectors |journal=Research in Astronomy and Astrophysics |date=December 2010 |volume=11 |issue=1 |pages=1–42 |doi=10.1088/1674-4527/11/1/001 |url=https://iopscience.iop.org/article/10.1088/1674-4527/11/1/001 |accessdate=29 July 2019 |language=en |issn=1674-4527|arxiv=1009.1138 }}</ref> The detector was run by [[David Blair (physicist)|David Blair]] at [[University of Western Australia]] in [[Perth]]. The detector ran in joint science runs from 1993-1998 with the gravitational-wave detectors [[AURIGA|Auriga]], [[Allegro gravitational-wave detector|Allegro]], [[Explorer]] and [[Nautillus]].<ref name=":0" />
+* [[Gravitational-wave astronomy]]
 == References ==
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 {{Gravitational waves|state=collapsed}}
+{{Portal bar|Australia|Physics|Astronomy|Stars|Spaceflight|Outer space|Solar System|Education|Science}}
 {{coord missing|Western Australia}}
 [[Category:Gravitational-wave telescopes]]
-[[Category:Astronomical observatories in Australia]]
+[[Category:Astronomical observatories in Western Australia]]
+{{Observatory-stub}}
+{{PerthAU-stub}}