Abstract
This paper gives an update on the status of the LISA technology package (LTP) which is to be launched in 2009 by ESA as a technology demonstration mission for the spaceborne gravitational wave observatory LISA. The dominant noise source in the interferometer prototype has been investigated and improved such that it is now comfortably below its budget at all frequencies.
Original language | English (US) |
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Pages (from-to) | 132-136 |
Number of pages | 5 |
Journal | Journal of Physics: Conference Series |
Volume | 32 |
Issue number | 1 |
DOIs | |
State | Published - Mar 2 2006 |
Externally published | Yes |
ASJC Scopus subject areas
- Physics and Astronomy(all)