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Construction of the Japanese second-generation gravitational-wave detector KAGRA has been started.
P. Saulson, Phys. Rev. D 42
1990
Earlier work this paper cites.
J. Mizuno et al
1993
Earlier work this paper cites.
Y. Levin, Phys. Rev. D 57
1998
Earlier work this paper cites.
M. Cerdonio, L. Conti, A. Heidmann, and M. Pinard, Phys. Rev. D 63
2001
Earlier work this paper cites.
A. Buonanno and Y. Chen, Phys. Rev. D 64
2001
Earlier work this paper cites.
D. Morelli et al
2002
Earlier work this paper cites.
G. Harry et al
2002
Earlier work this paper cites.
S. Sato et al
2004
Earlier work this paper cites.
T. Tomaru et al
2004
Earlier work this paper cites.
B. Willke et al
2006
Cited alongside, same era.
K. Yamamoto et al
2006
Cited alongside, same era.
K. Somiya, Y. Chen, S. Kawamura, and N. Mio, Phys. Rev. D 73
2006
Cited alongside, same era.
C. Kim, AIP Conf. Proc., 983, 576-583 (2007)
2007
Cited alongside, same era.
D. Lorimer, Living Rev. Relativity, 11
2008
Cited alongside, same era.
I. Martin et al
2008
Cited alongside, same era.
”Advanced Virgo Baseline Design,” The Virgo Collaboration, VIR-0027A-09 (2009); available from https://pub3.ego-gw.it/itf/tds/
2009
Cited alongside, same era.
G. Harry for the LIGO Scientific Collaboration, Class. Quantum Grav., 27
2010
Later among the works it cites.
S. Hild, et al
2010
Later among the works it cites.
J. Abadie et al
2010
Later among the works it cites.
R. Flaminio et al
2010
Later among the works it cites.
I. Martin et al
2010
Later among the works it cites.
K. Somiya, K. Kokeyama, and R. Nawrodt, Phys. Rev. D 82
2010
Later among the works it cites.
”Sapphire for the KAGRA project,” E.Hirose, K.Watanabe, and N.Mio, JGW-G1100626-v1 (2011); available from http://gwdoc.icrr.u-tokyo.ac.jp/cgi-bin/DocDB/DocumentDatabase
2011
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”Discussion about losses in the perpendicular and parallel directions,” K. Somiya, LIGO-DCC T0900033-v1 (2009); available from https://dcc.ligo.org/
2009
Cited alongside, same era.
”The thermal noise of the Virgo+ and Virgo Advanced Last Stage Suspension (The PPP effect),” F. Piergiovanni, M. Punturo, and P. Puppo, VIR-015E-09 (2009)
2009
Cited alongside, same era.
This estimated noise spectrum is slightly different from the official sensitivity curve of KAGRA provided in the web page (http://gwcenter.icrr.u-tokyo.ac.jp/en/researcher/parameter), which is calculated with the most optimistic parameter set
Cited in the paper.
http://www.nikhef.nl/en/for-nikhef-users/departments/scientific-departments/gw
Cited in the paper.
Temperature dependence of each thermal parameter is given as follows, fitted to measurement results: κ s = ( 0.272 × T m − 2.2 + 6.22 × 10 − 9 × T m 3.04 ) − 1.25 \kappa_{\mathrm{s}}=(0.272\times T_{\mathrm{m}}^{-2.2}+6.22\times 10^{-9}\times T_{\mathrm{m}}^{3.04})^{-1.25} [W/m/K], C s = 0.227 × T m 3.14 C_{\mathrm{s}}=0.227\times T_{\mathrm{m}}^{3.14} [J/ m 3 \mathrm{m}^{3} /K], α = 7.21 × 10 − 13 × T m 2.99 \alpha=7.21\times 10^{-13}\times T_{\mathrm{m}}^{2.99} [1/K], where T m T_{\mathrm{m}} is in Kelvin
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”Development of cryogenic system for Large-scale Cryogenic Gravitational wave Telescope (4) - Reduction of initial cooling time of KAGRA mirrors -,” Y. Sakakibara, et al
2011
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