Preliminary results on the suppression of sensing cross-talk in LISA Pathfinder

被引：20

作者：

Wanner, Gudrun ^{[1
]}

Karnesis, Nikolaos

Armano, M. ^{[2
]}

Audley, H. ^{[3
,4
]}

Auger, G. ^{[5
]}

Baird, J. ^{[6
]}

Bassan, M. ^{[7
,8
]}

Binetruy, P. ^{[5
]}

Born, M. ^{[3
,4
]}

Bortoluzzi, D. ^{[9
,10
]}

Brandt, N. ^{[11
]}

Caleno, M. ^{[12
]}

Cavalleri, A. ^{[13
,14
]}

Cesarini, A. ^{[13
,14
]}

Cruise, M. ^{[15
]}

Danzmann, K. ^{[3
,4
]}

de Deus Silva, M. ^{[2
]}

De Rosa, R. ^{[16
,17
]}

Di Fiore, L. ^{[17
]}

Diepholz, I. ^{[3
,4
]}

Dolesi, R. ^{[13
,14
]}

Dunbar, N. ^{[18
]}

Ferraioli, L. ^{[19
]}

Ferroni, V. ^{[13
,14
]}

Fitzsimons, E. ^{[20
]}

Flatscher, R. ^{[11
]}

Freschi, M. ^{[2
]}

Marrirodriga, C. Garcia ^{[12
]}

Gerndt, R. ^{[11
]}

Gesa, L. ^{[21
]}

Gibert, F. ^{[13
,14
]}

Giardini, D. ^{[19
]}

Giusteri, R. ^{[13
,14
]}

Grado, A. ^{[16
,17
]}

Grimani, C. ^{[22
]}

Grzymisch, J. ^{[12
]}

Harrison, I. ^{[23
]}

Heinzel, G. ^{[3
,4
]}

Hewitson, M. ^{[3
,4
]}

Hollington, D. ^{[6
]}

Hoyland, D. ^{[15
]}

Hueller, M. ^{[13
,14
]}

Inchauspe, H. ^{[5
]}

Jennrich, O. ^{[12
]}

Jetzer, P. ^{[24
]}

Johlander, B. ^{[12
]}

Karnesis, N. ^{[3
,4
]}

Kaune, B. ^{[3
,4
]}

Korsakova, N. ^{[3
,4
]}

Killow, C. ^{[25
]}

机构：

[1] Leibniz Univ Hannover, Albert Einstein Inst, Max Planck Inst Gravitat Phys, Hannover, Germany

[2] European Space Agcy, European Space Astron Ctr, Madrid 28692, Spain

[3] Max Planck Inst Gravitat Phys, Albert Einstein Inst, Callinstr 38, D-30167 Hannover, Germany

[4] Leibniz Univ Hannover, Callinstr 38, D-30167 Hannover, Germany

[5] Univ Paris Diderot, APC, CNRS IN2P3, CEA Irfu,Obs Paris,Sorbonne Paris Cite, Paris, France

[6] Imperial Coll London, High Energy Phys Grp, Blackett Lab, Phys Dept, Prince Consort Rd, London SW7 2BW, England

[7] Univ Roma Tor Vergata, Dipartimento Fis, I-00133 Rome, Italy

[8] INFN, Sez Roma Tor Vergata, I-00133 Rome, Italy

[9] Univ Trento, Dept Ind Engn, Via Sommar 9, I-38123 Trento, Italy

[10] INFN, Trento Inst Fundamental Phys & Applicat, Rome, Italy

[11] Airbus Def & Space, Claude Dornier Str, D-88090 Immenstaad, Germany

[12] European Space Agcy, European Space Technol Ctr, Keplerlaan 1, NL-2200 AG Noordwijk, Netherlands

[13] Univ Trento, Dipartimento Fis, I-38123 Povo, Trento, Italy

[14] INFN, Trento Inst Fundamental Phys & Applicat, I-38123 Povo, Trento, Italy

[15] Univ Birmingham, Dept Phys & Astron, Birmingham, W Midlands, England

[16] INAF, Osservatorio Astron Capodimonte, I-80131 Naples, Italy

[17] INFN, Sez Napoli, I-80126 Naples, Italy

[18] Airbus Def & Space, Gunnels Wood Rd, Stevenage SG1 2AS, Herts, England

[19] Swiss Fed Inst Technol, Inst Geophys, Sonneggstr 5, CH-8092 Zurich, Switzerland

[20] Royal Observ, UK Astron Technol Ctr, Blackford Hill, Edinburgh EH9 3HJ, Midlothian, Scotland

[21] Inst Ciencies Espai CSIC IEEC, Campus UAB,Carrer Can Magrans S-N, Cerdanyola Del Valles 08193, Spain

[22] Univ Urbino Carlo Bo, DISPEA, INFN, Via S Chiara 27, I-61029 Urbino, Italy

[23] European Space Agcy, European Space Operat Ctr, D-64293 Darmstadt, Germany

[24] Univ Zurich, Phys Inst, Winterthurerstr 190, CH-8057 Zurich, Switzerland

[25] Univ Glasgow, Sch Phys & Astron, SUPA, Inst Gravitat Res, Glasgow G12 8QQ, Lanark, Scotland

[26] Univ Politecn Cataluna, Dept Engn Elect, ES-08034 Barcelona, Spain

[27] Co Gen Spazio, CGS SpA, Via Gallarate 150, I-20151 Milan, Italy

[28] NASA, Goddard Space Flight Ctr, Gravitat Astrophys Lab, 8800 Greenbelt Rd, Greenbelt, MD 20771 USA

[29] Univ Firenze, Dipartimento Fis & Astron, I-50019 Florence, Italy

[30] INFN, Sez Firenze, I-50019 Florence, Italy

来源：

11TH INTERNATIONAL LISA SYMPOSIUM | 2017年 / 840卷

关键词：

D O I：

10.1088/1742-6596/840/1/012043

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In the original paper describing the first measurements performed with LISA Pathfinder, a bulge in the acceleration noise was shown in the 200mHz - 20mHz frequency band. This bulge noise originated from cross-coupling of spacecraft motion into the longitudinal readout and it was shown that it is possible to subtract this cross-talk noise. We discuss here the model that was used for subtraction as well as an alternative approach to suppress the cross talk by realignment of the test masses. Such a realignment was performed after preliminary analysis of a dedicated cross-talk experiment, and we show the resulting noise suppression. Since then, further experiments have been performed to investigate the cross-coupling behaviour, however analysis of these experiments is still on-going.

引用

页数：4

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