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  5. Sensor noise in LISA Pathfinder: An extensive in-flight review of the angular and longitudinal interferometric measurement system
 

Sensor noise in LISA Pathfinder: An extensive in-flight review of the angular and longitudinal interferometric measurement system

Journal
PHYSICAL REVIEW D  
Date Issued
2022
Author(s)
Armano, M.
•
Audley, H.
•
Baird, J.
•
Binetruy, P.
•
Born, M.
•
Bortoluzzi, D.
•
Brandt, N.
•
Castelli, E.
•
Cavalleri, A.
•
Cesarini, A.
•
Cruise, A. M.
•
Danzmann, K.
•
de Deus Silva, M.
•
Diepholz, I.
•
Dixon, G.
•
Dolesi, R.
•
Ferraioli, L.
•
Ferroni, V.
•
Fitzsimons, E. D.
•
Flatscher, R.
•
Freschi, M.
•
García, A.
•
Gerndt, R.
•
Gesa, L.
•
Giardini, D.
•
Gibert, F.
•
Giusteri, R.
•
Grimani, C.
•
Grzymisch, J.
•
Guzman, F.
•
Harrison, I.
•
Hartig, M. -S.
•
Hechenblaikner, G.
•
Heinzel, G.
•
Hewitson, M.
•
Hollington, D.
•
Hoyland, D.
•
Hueller, M.
•
Inchauspé, H.
•
Jennrich, O.
•
Jetzer, P.
•
Johann, U.
•
Johlander, B.
•
Karnesis, N.
•
Kaune, B.
•
Killow, C. J.
•
Korsakova, N.
•
Lobo, J. A.
•
López-Zaragoza, J. P.
•
Maarschalkerweerd, R.
•
Mance, D.
•
Martín, V.
•
Martin-Polo, L.
•
Martin-Porqueras, F.
•
Martino, J.
•
McNamara, P. W.
•
Mendes, J.
•
Mendes, L.
•
Meshksar, N.
•
Monsky, A.
•
Nofrarias, M.
•
Paczkowski, S.
•
Perreur-Lloyd, M.
•
Petiteau, A.
•
Plagnol, E.
•
Ramos-Castro, J.
•
Reiche, J.
•
Rivas, F.
•
Robertson, D. I.
•
RUSSANO, Giuliana  
•
Sanjuan, J.
•
Slutsky, J.
•
Sopuerta, C. F.
•
Steier, F.
•
Sumner, T.
•
Texier, D.
•
Thorpe, J. I.
•
Vetrugno, D.
•
Vitale, S.
•
Wand, V.
•
Wanner, G.
•
Ward, H.
•
Wass, P. J.
•
Weber, W. J.
•
Wissel, L.
•
Wittchen, A.
•
Zweifel, P.
DOI
10.1103/PhysRevD.106.082001
Abstract
In a previous article [1], we have reported on the first subpicometer interferometer flown in space as part of ESA's LISA Pathfinder mission, and have shown the residual sensor noise to be on the level of 32.0-1.7+2.4 fm /√{Hz } . This review provides a deeper and more complete overview of the full system and its interferometric mission performance under varying operational conditions, allowing a much more detailed view on the noise model. We also include the optical measurements of rotations through differential wave front sensing (DWS), which reached a sensitivity of as good as 100 prad /√{Hz } . We present more evidence for the long-term stability of the interferometric performance and components. This proves a solid foundation for future interferometry in space such as the LISA mission.
Volume
106
Issue
8
Start page
082001
Uri
http://hdl.handle.net/20.500.12386/35079
Url
https://api.elsevier.com/content/abstract/scopus_id/85142906654
https://journals.aps.org/prd/abstract/10.1103/PhysRevD.106.082001
Issn Identifier
2470-0010
Ads BibCode
2022PhRvD.106h2001A
Rights
open.access
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sensor_noise_OMS_PhysRevD.106.082001.pdf

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Format

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