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LISA Pathfinder: Understanding DWS noise performance for the LISA mission

dc.contributor.authorWissel, L.
dc.contributor.authorArmano, M.
dc.contributor.authorAudley, H.
dc.contributor.authorAuger, G.
dc.contributor.authorBaird, J.
dc.contributor.authorBassan, M.
dc.contributor.authorBinetruy, P.
dc.contributor.authorBorn, M.
dc.contributor.authorBortoluzzi, D.
dc.contributor.authorBrandt, N.
dc.contributor.authorCaleno, M.
dc.contributor.authorCavalleri, A.
dc.contributor.authorCesarini, A.
dc.contributor.authorCruise, M.
dc.contributor.authorDanzmann, K.
dc.contributor.authorde Deus Silva, M.
dc.contributor.authorDe Rosa, R.
dc.contributor.authorDi Fiore, L.
dc.contributor.authorDiepholz, I.
dc.contributor.authorDolesi, R.
dc.contributor.authorDunbar, N.
dc.contributor.authorFerraioli, Luigi
dc.contributor.authorFerroni, V.
dc.contributor.authorFitzsimons, E. D.
dc.contributor.authorFlatscher, R.
dc.contributor.authorFreschi, M.
dc.contributor.authorGarcía Marirrodriga, C.
dc.contributor.authorGerndt, R.
dc.contributor.authorGesa, L.
dc.contributor.authorGibert, F.
dc.contributor.authorGiardini, D.
dc.contributor.authorGiusteri, R.
dc.contributor.authorGrado, A.
dc.contributor.authorGrimani, C.
dc.contributor.authorGrzymisch, J.
dc.contributor.authorHarrison, I.
dc.contributor.authorHeinzel, G.
dc.contributor.authorHewitson, M.
dc.contributor.authorHollington, D.
dc.contributor.authorHoyland, D.
dc.contributor.authorHueller, M.
dc.contributor.authorInchauspé, H.
dc.contributor.authorJennrich, O.
dc.contributor.authorJetzer, P.
dc.contributor.authorJohlander, B.
dc.contributor.authorKarnesis, N.
dc.contributor.authorKaune, B.
dc.contributor.authorKorsakova, N.
dc.contributor.authorKillow, C. J.
dc.contributor.authorLobo, A.
dc.contributor.authorLloro, I.
dc.contributor.authorLiu, L.
dc.contributor.authorLópez Zaragoza, J. P.
dc.contributor.authorMaarschalkerweerd, R.
dc.contributor.authorMance, D.
dc.contributor.authorMartín, V.
dc.contributor.authorMartín Polo, L.
dc.contributor.authorMartino, J.
dc.contributor.authorMartín Porqueras, F.
dc.contributor.authorMadden, S.
dc.contributor.authorMateos, I.
dc.contributor.authorMcNamara, P. W.
dc.contributor.authorMendes, J.
dc.contributor.authorMendel, L.
dc.contributor.authorNofrarias, M.
dc.contributor.authorPaczkowski, S.
dc.contributor.authorPerreur Lloyd, M.
dc.contributor.authorPetiteau, A.
dc.contributor.authorPivato, P.
dc.contributor.authorPlagnol, E.
dc.contributor.authorPrat, P.
dc.contributor.authorRagnit, U.
dc.contributor.authorRamos Castro, J.
dc.contributor.authorReiche, J.
dc.contributor.authorRobertson, D. I.
dc.contributor.authorRozemeijer, H.
dc.contributor.authorRivas García, Francisco
dc.contributor.authorRussano, G.
dc.contributor.authorSarra, P.
dc.contributor.authorSchleicher, A.
dc.contributor.authorShaul, D.
dc.contributor.authorSlutsky, J.
dc.contributor.authorSopuerta, C. F.
dc.contributor.authorStanga, R.
dc.contributor.authorSumner, T.
dc.contributor.authorTexier, D.
dc.contributor.authorThorpe, J. I.
dc.contributor.authorTrenkel, C.
dc.contributor.authorTroebs, M.
dc.contributor.authorVetrugno, D.
dc.contributor.authorVitale, S.
dc.contributor.authorWanner, G.
dc.contributor.authorWard, H.
dc.contributor.authorWass, P. J.
dc.contributor.authorWealthy, D.
dc.contributor.authorWeber, W. J.
dc.contributor.authorWissel, L.
dc.contributor.authorWittchen, A.
dc.contributor.authorZambotti, A.
dc.contributor.authorZanoni, C.
dc.contributor.authorZiegler, T.
dc.contributor.authorZweifel, P.
dc.contributor.authorLPF Collaboration
dc.date.accessioned2023-11-22T14:59:02Z
dc.date.available2023-11-22T14:59:02Z
dc.date.issued2017
dc.identifier.citationLennart Wissel and on behalf of the LPF collaboration 2017 J. Phys.: Conf. Ser. 840 012044es
dc.identifier.issn1742-6596
dc.identifier.issn1742-6588
dc.identifier.urihttps://hdl.handle.net/20.500.12412/4728
dc.description.abstractESA's L3 Laser Interferometer Space Antenna (LISA) mission contains a mechanism to compensate for out-of-plane angles between the received and emitted beams of the three satellites. Depending on the configuration of this Point-Ahead Angle Mechanism (PAAM) it is expected to contribute readout noise through Differential Wavefront Sensing (DWS). This was investigated with LISA Pathfinder (LPF) through a dedicated investigation. One of the two free-falling test masses was rotated via the on-board electrostatic actuators while the resulting angular noise in the differential interferometer between the two test masses was measured. For angles between −250 μrad to 250 μrad and corresponding contrast in the range of 59.4 % to 97.9 % an increased spectral density was found. The differential displacement noise remains almost unchanged for these misalignments.es
dc.description.sponsorshipThe Albert-Einstein-Institut acknowledges the support of the German Space Agency, DLR. The work is supported by the Federal Ministry for Economic Affairs and Energy based on a resolution of the German Bundestag (FKZ 50OQ0501 and FKZ 50OQ1601).es
dc.language.isoenges
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 Internacional*
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/*
dc.titleLISA Pathfinder: Understanding DWS noise performance for the LISA missiones
dc.typearticlees
dc.identifier.doi10.1088/1742-6596/840/1/012044
dc.issue.number012044es
dc.journal.titleJournal of Physics: Conference Serieses
dc.rights.accessRightsopenAccesses
dc.volume.number840es


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