Details
Originalsprache | Englisch |
---|---|
Seiten (von - bis) | 132-136 |
Seitenumfang | 5 |
Fachzeitschrift | Journal of Physics: Conference Series |
Jahrgang | 32 |
Frühes Online-Datum | 29 März 2006 |
Publikationsstatus | Veröffentlicht - 2011 |
Veranstaltung | Sixth Edoardo Amaldi Conference on gravitational waves - Okinawa, Japan Dauer: 20 Juni 2005 → 24 Juni 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 Sachgebiete
- Physik und Astronomie (insg.)
- Allgemeine Physik und Astronomie
Zitieren
- Standard
- Harvard
- Apa
- Vancouver
- BibTex
- RIS
in: Journal of Physics: Conference Series, Jahrgang 32, 2011, S. 132-136.
Publikation: Beitrag in Fachzeitschrift › Konferenzaufsatz in Fachzeitschrift › Forschung › 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 -