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Temperature stability in the sub-milliHertz band with LISA ..:
Audley, H
;
Baird, J
;
Binetruy, P
...
This work has been made possible by the LISA Pathfinder mission, which is part of the space-science program of the European Space Agency. The French contribution has been supported by CNES (Accord Specific de projet CNES 1316634/CNRS 103747), the CNRS, the Observatoire de Paris and the University Paris-Diderot. EP and HI would also like to acknowledge the financial support of the UnivEarthS Labex program at Sorbonne Paris Cité (ANR-10-LABX-0023 and ANR-11-IDEX-0005-02). The 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). The Italian contribution has been supported by Agenzia Spaziale Italiana and Instituto Nazionale di Fisica Nucleare. The Spanish contribution has been supported by Contracts No. AYA2010-15709 (Ministerio de Ciencia, Innovacion y Universidades, MICINN), No. ESP201.... , 2019
Link:
https://hdl.handle.net/20.500.12412/4766
RT Journal T1
Temperature stability in the sub-milliHertz band with LISA Pathfinder
UL https://suche.suub.uni-bremen.de/peid=base-ftunivloyola:oai:repositorio.uloyola.es:20.500.12412_4766&Exemplar=1&LAN=DE A1 Audley, H A1 Baird, J A1 Binetruy, P A1 Born, M A1 Bortoluzzi, D A1 Castelli, E A1 Cavalleri, A A1 Cruise, A. M A1 Danzmann, K A1 de Deus Silva, M A1 Diepholz, I A1 Dixon, G A1 Dolesi, R A1 Ferraioli, L A1 Fitzsimons, E. D A1 Freschi, M A1 Gesa, L A1 Gibert, F A1 Giardini, D A1 Giusteri, R A1 Grimani, C A1 Harrison, I A1 Heinzel, G A1 Hewitson, M A1 Hollington, D A1 Hoyland, D A1 Hueller, M A1 Inchauspé, H A1 Jetzer, P A1 Karnesis, N A1 Kaune, B A1 Korsakova, N A1 Killow, C. J A1 Lobo, J. A A1 Lloro, I A1 López Zaragoza, J. P A1 Maarschalkerweerd, R A1 Mance, D A1 Mansanet, C A1 Martín, V A1 Martín Polo, L A1 Martino, J A1 Mateos, I A1 McNamara, P. W A1 Mendes, J A1 Mendes, L A1 Meshksar, N A1 Nofrarias, M A1 Paczkowski, S A1 Petiteau, A A1 Pivato, P A1 Plagnol, E A1 Ramos Castro, J A1 Reiche, J A1 Robertson, D. I A1 Rivas García, Francisco A1 Sanjuan, J A1 Slutsky, J A1 Sopuerta, C. F A1 Sumner, T A1 Texier, D A1 Thorpe, J. I A1 Trenkel, C A1 Vitale, S A1 Wanner, G A1 Ward, H A1 Wass, P. J A1 Wealthy, D A1 Weber, W. J A1 Wissel, L A1 Zweifel, P A1 Cesarini, A A1 Ferroni, V A1 Grzymisch, J A1 Jennrich, O A1 Liu, L A1 Martín Porqueras, F A1 Perreur Lloyd, M A1 Russano, G A1 Vetrugno, D A1 Wittchen, A YR 2019 K1 Gravitational Waves K1 Space vehicles JF This work has been made possible by the LISA Pathfinder mission, which is part of the space-science program of the European Space Agency. The French contribution has been supported by CNES (Accord Specific de projet CNES 1316634/CNRS 103747), the CNRS, the Observatoire de Paris and the University Paris-Diderot. EP and HI would also like to acknowledge the financial support of the UnivEarthS Labex program at Sorbonne Paris Cité (ANR-10-LABX-0023 and ANR-11-IDEX-0005-02). The 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). The Italian contribution has been supported by Agenzia Spaziale Italiana and Instituto Nazionale di Fisica Nucleare. The Spanish contribution has been supported by Contracts No. AYA2010-15709 (Ministerio de Ciencia, Innovacion y Universidades, MICINN), No. ESP201... LK http://dx.doi.org/https://hdl.handle.net/20.500.12412/4766 DO https://hdl.handle.net/20.500.12412/4766 SF ELIB - SuUB Bremen
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