{"id":648,"date":"2011-05-12T11:54:45","date_gmt":"2011-05-12T02:54:45","guid":{"rendered":"https:\/\/gwcenter.icrr.u-tokyo.ac.jp\/en"},"modified":"2017-10-05T10:09:29","modified_gmt":"2017-10-05T01:09:29","slug":"parameter","status":"publish","type":"page","link":"https:\/\/gwcenter.icrr.u-tokyo.ac.jp\/en\/researcher\/parameter","title":{"rendered":"KAGRA Parameters"},"content":{"rendered":"
\n

KAGRA Parameters<\/h2>\n<\/div>\n

KAGRA Sensitivity Curve<\/h3>\n

KAGRA official sensitivity limit<\/h4>\n

Estimated sensitivity limits of KAGRA are presented here. These curves are calculated from incoherent sum of the fundamental noise sources. Actual sensitivity to gravitational-wave signals may be degraded from these ideal calculation because of technical noise sources.<\/p>\n

Two types of curves are described. One is an official curve, which has been officially approved by the project manager. Another is a latest best estimation, which includes strategic or technical updates of detector design.<\/p>\n

Officially approved sensitivity limit curve is presented here.<\/p>\n

\n
  • Study report on KAGRA interferometer observation band, 8th Sep. 2009 (pdf, ~1.2MB)<\/a><\/li>\n
  • VRSE(D) data (deliminated text)<\/a><\/li>\n
  • VRSE(B) data (deliminated text)<\/a><\/li>\n
  • Detail spectra of noise budget (zip, ~800KB)<\/a><\/li>\n<\/div>\n
    \n\"\"<\/a><\/p>\n

    Officially approved sensitivity limit curve<\/p><\/div>\n

    last update : 8th Sep. 2009<\/p>\n

    bKAGRA Sensitivity Curve<\/h4>\n

    bKAGRA stands for baseline KAGRA, operated with the final detector configuration at cryogenic temperature.<\/p>\n

    \n
  • data and update history<\/a><\/li>\n<\/div>\n

    bKAGRA sensitivity limit curve <\/p>\n

    <\/p>\n<\/div>\n
    \nContact address (Email) : sensitivity-gwo_AT_gw.icrr.u-tokyo.ac.jp<\/p>\n

    (Please change ‘_AT_’ with ‘@’ for valid mail address.)<\/p>\n","protected":false},"excerpt":{"rendered":"

    KAGRA Parameters KAGRA Sensitivity Curve KAGRA official sensitivity limit Estimated sensitivity limits of KAGR […]<\/p>\n","protected":false},"author":1,"featured_media":0,"parent":67,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"researcher.php","meta":{"footnotes":""},"class_list":["post-648","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/gwcenter.icrr.u-tokyo.ac.jp\/en\/wp-json\/wp\/v2\/pages\/648","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/gwcenter.icrr.u-tokyo.ac.jp\/en\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/gwcenter.icrr.u-tokyo.ac.jp\/en\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/gwcenter.icrr.u-tokyo.ac.jp\/en\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/gwcenter.icrr.u-tokyo.ac.jp\/en\/wp-json\/wp\/v2\/comments?post=648"}],"version-history":[{"count":31,"href":"https:\/\/gwcenter.icrr.u-tokyo.ac.jp\/en\/wp-json\/wp\/v2\/pages\/648\/revisions"}],"predecessor-version":[{"id":1190,"href":"https:\/\/gwcenter.icrr.u-tokyo.ac.jp\/en\/wp-json\/wp\/v2\/pages\/648\/revisions\/1190"}],"up":[{"embeddable":true,"href":"https:\/\/gwcenter.icrr.u-tokyo.ac.jp\/en\/wp-json\/wp\/v2\/pages\/67"}],"wp:attachment":[{"href":"https:\/\/gwcenter.icrr.u-tokyo.ac.jp\/en\/wp-json\/wp\/v2\/media?parent=648"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}