Details
Original language | English |
---|---|
Pages (from-to) | 132-136 |
Number of pages | 5 |
Journal | Journal of Physics: Conference Series |
Volume | 32 |
Early online date | 29 Mar 2006 |
Publication status | Published - 2011 |
Event | Sixth Edoardo Amaldi Conference on gravitational waves - Okinawa, Japan Duration: 20 Jun 2005 → 24 Jun 2005 |
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.
ASJC Scopus subject areas
- Physics and Astronomy(all)
- General Physics and Astronomy
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In: Journal of Physics: Conference Series, Vol. 32, 2011, p. 132-136.
Research output: Contribution to journal › Conference article › Research › peer review
}
TY - JOUR
T1 - Interferometry for the LISA technology package LTP
T2 - Sixth Edoardo Amaldi Conference on gravitational waves
AU - Heinzel, G.
AU - Bogenstahl, J.
AU - Braxmaier, C.
AU - Danzmann, K.
AU - Garcia, A.
AU - Guzman, F.
AU - Hough, J.
AU - Hoyland, D.
AU - Jennrich, O.
AU - Killow, C.
AU - Robertson, D.
AU - Sodnik, Z.
AU - Steier, F.
AU - Ward, H.
AU - Wand, V.
PY - 2011
Y1 - 2011
N2 - 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.
AB - 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.
UR - http://www.scopus.com/inward/record.url?scp=33645499330&partnerID=8YFLogxK
U2 - 10.1088/1742-6596/32/1/021
DO - 10.1088/1742-6596/32/1/021
M3 - Conference article
AN - SCOPUS:33645499330
VL - 32
SP - 132
EP - 136
JO - Journal of Physics: Conference Series
JF - Journal of Physics: Conference Series
SN - 1742-6588
Y2 - 20 June 2005 through 24 June 2005
ER -