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CLIO

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is an optical interferometer with two perpendicular arms each of 100 m length. The mirrors are cooled to 20 K (−253 °C); this reduces various thermal noise sources which trouble other gravity observatories, but cooling the mirrors (which are heated by the powerful laser used in the
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CLIO is one of the science facilities for physics of the Institute for Cosmic Ray Research of the
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interferometer) while keeping them isolated from vibrations is difficult.
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K. Yamamoto; et al. (2008). "Current status of the CLIO project".
1038: 586: 397: 269:"Cryogenic systems of the Cryogenic Laser Interferometer Observatory" 812: 601: 570: 448: 228: 162: 642: 591: 566: 308: 1052: 999: 968: 908: 834: 827: 800: 767: 733: 717: 708: 688: 667: 651: 620: 559: 548: 503: 487: 421: 380: 369: 360: 92: 55: 44: 31: 180:CLIO is situated 1000 m underground in the 889:(first-ever possible light from bh-bh merger) 320: 8: 26: 1176:Buildings and structures in Gifu Prefecture 163:Kamioka Gravitational Wave Detector (KAGRA) 35:Cryogenic Laser Interferometer Observatory 831: 714: 556: 377: 366: 327: 313: 305: 159:Cryogenic Laser Interferometer Observatory 101: 36: 25: 292: 227: 16:Detector for gravitational waves in Japan 901:(first black hole - neutron star merger) 204: 273:Journal of Physics: Conference Series 215:Journal of Physics: Conference Series 7: 459:Stanford gravitational wave detector 1171:Astronomical observatories in Japan 611:European Gravitational Observatory 14: 895:(first-ever "mass gap" collision) 267:T. Uchiyama; et al. (2006). 122: 115: 352:Gravitational-wave observatory 246:10.1088/1742-6596/122/1/012002 97:gravitational-wave observatory 1: 1161:Gravitational-wave telescopes 1044:Gravitational wave background 596:LIGO Scientific Collaboration 847:First observation (GW150914) 633:TAMA 20, later known as LISM 336:Gravitational-wave astronomy 123: 981:Tests of general relativity 1197: 643:Caltech 40m interferometer 294:10.1088/1742-6596/32/1/038 165:. It is located in Japan. 18: 342: 141: 110: 1084:Supermassive black holes 923:Resonant mass detectors 77:36.42694°N 137.31194°E 32:Alternative names 1108:Rotating neutron star 919:Laser interferometers 1000:Effects / properties 929:Atom interferometers 842:List of observations 769:Pulsar timing arrays 93:Telescope style 19:For other uses, see 1089:Stellar black holes 1069:quantum fluctuation 949:Pulsar timing array 936:Indirect detection 876:neutron star merger 659:INDIGO (LIGO-India) 285:2006JPhCS..32..259U 238:2008JPhCS.122a2002Y 193:University of Tokyo 182:Kamioka Observatory 82:36.42694; 137.31194 73: /  28: 976:General relativity 680:Einstein Telescope 582:Fermilab holometer 347:Gravitational wave 1166:Research in Japan 1148: 1147: 964: 963: 915:Direct detection 763: 762: 759: 758: 741:Big Bang Observer 704: 703: 544: 543: 152: 151: 1188: 1080:Binary inspiral 1074:Phase transition 1065:Cosmic inflation 832: 715: 557: 378: 367: 329: 322: 315: 306: 299: 298: 296: 264: 258: 257: 231: 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808:Einstein@Home 806: 805: 803: 801:Data analysis 799: 793: 790: 788: 785: 783: 780: 778: 775: 774: 772: 770: 766: 752: 749: 747: 744: 742: 739: 738: 736: 732: 726: 723: 722: 720: 716: 713: 707: 697: 694: 693: 691: 687: 681: 678: 676: 673: 672: 670: 666: 660: 657: 656: 654: 650: 644: 641: 639: 636: 634: 631: 629: 626: 625: 623: 619: 612: 608: 605: 603: 600: 597: 593: 592:Advanced LIGO 590: 588: 585: 583: 580: 578: 575: 572: 568: 565: 564: 562: 558: 555: 553: 547: 536: 532: 529: 527: 524: 522: 519: 516: 512: 509: 508: 506: 502: 496: 493: 492: 490: 486: 480: 477: 475: 472: 470: 467: 465: 462: 460: 457: 454: 450: 447: 444: 440: 437: 434: 430: 427: 426: 424: 420: 414: 411: 409: 406: 403: 399: 396: 393: 389: 386: 385: 383: 379: 376: 374: 371:Resonant mass 368: 365: 363: 359: 353: 350: 348: 345: 344: 341: 337: 330: 325: 323: 318: 316: 311: 310: 307: 295: 290: 286: 282: 278: 274: 270: 263: 260: 255: 251: 247: 243: 239: 235: 230: 225: 222:(1): 012002. 221: 217: 216: 208: 205: 198: 196: 194: 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940:B-modes 909:Methods 874:(first 751:TianQin 718:Planned 652:Planned 469:GEOGRAV 439:ALLEGRO 281:Bibcode 234:Bibcode 157:is the 51:, Japan 1113:Burst 1039:energy 969:Theory 835:Events 746:DECIGO 587:GEO600 560:Active 464:ALTAIR 398:AURIGA 381:Active 252:  99:  813:PyCBC 602:KAGRA 571:ACIGA 526:SFERA 511:GRAIL 474:AGATA 449:NIOBE 250:S2CID 224:arXiv 143:[ 1135:and 1099:EMRI 792:PPTA 782:IPTA 777:EPTA 725:LISA 621:Past 577:CLIO 567:AIGO 521:TIGA 495:TOBA 453:IGEC 443:IGEC 433:IGEC 422:Past 402:IGEC 392:IGEC 174:CLIO 155:CLIO 27:CLIO 944:CMB 942:of 289:doi 242:doi 220:122 1157:: 287:. 277:32 275:. 271:. 248:. 240:. 232:. 218:. 195:. 188:. 184:, 1067:- 1034:) 878:) 613:) 609:( 598:) 594:( 573:) 569:( 537:) 517:) 455:) 451:( 445:) 441:( 435:) 431:( 404:) 400:( 394:) 390:( 328:e 321:t 314:v 297:. 291:: 283:: 256:. 244:: 236:: 226:: 147:] 23:.

Index

Clio Awards
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Gifu Prefecture
36°25′37″N 137°18′43″E / 36.42694°N 137.31194°E / 36.42694; 137.31194
gravitational-wave observatory
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CLIO is located in Earth
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Kamioka Gravitational Wave Detector (KAGRA)
Kamioka Observatory
Gifu Prefecture
University of Tokyo
Journal of Physics: Conference Series
arXiv
0805.2384
Bibcode
2008JPhCS.122a2002Y
doi
10.1088/1742-6596/122/1/012002
S2CID
14580628
"Cryogenic systems of the Cryogenic Laser Interferometer Observatory"
Bibcode
2006JPhCS..32..259U
doi
10.1088/1742-6596/32/1/038
v
t
e
Gravitational-wave astronomy

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