Status of LIGO at the start of the fifth science run
2006
Abbott, B. | Abbott, R. | Adhikari, R. | Agresti, J. | Ajith, P. | Allen, B. | Amin, R. | Anderson, S. | Anderson, W. | Arain, M. | Araya, M. | Armandula, H. | Ashley, M. | Aston, S. | Aufmuth, P. | Aulbert, C. | Babak, S. | Ballmer, S. | Bantilan, H. | Barish, B. | et al. | Veitch, Peter John | Hosken, David John | Munch, Jesper
Copyright © Institute of Physics and IOP Publishing Limited 2006. Peter Veitch, David Hosken and Jesper Munch are members of the LIGO Scientific Collaboration
اظهر المزيد [+] اقل [-]<jats:p>In November 2005, the LIGO interferometer network began data taking for its latest data run (S5). All three interferometers are working at design sensitivities with duty cycles expected to reach 80%. The Hanford 4 km detector regularly achieves a<jats:inline-graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="cqg227189ieqn1.gif"/>neutron star inspiral range of 12 Mpc. The S5 data run will record one year of coincident science data at unprecedented sensitivity ending in mid 2007.</jats:p>
اظهر المزيد [+] اقل [-]Samuel J Waldman (for the LIGO Science Collaboration)
اظهر المزيد [+] اقل [-]المعلومات البيبليوغرافية
تم تزويد هذا السجل من قبل University of Adelaide
