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LISA Pathfinder micronewton cold gas thrusters: In-flight c..:

Armano, M ; Audley, H ; Baird, J...
This work has been made possible by the LISA Pathfinder mission, which is part of the space-science programme of the European Space Agency. The French contribution has been supported by the CNES (Accord Specifique de projet CNES 1316634/CNRS 103747), the CNRS, the Observatoire de Paris and the University Paris-Diderot. E. Plagnol and H. Inchausp´e would also like to acknowledge the financial support of the UnivEarthS Labex program at Sorbonne Paris Cit´e (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 Istituto Nazionale di Fisica Nucleare. The Spanish contribution has been supported by contracts AYA2010-15709 (MICINN), ESP2013-47637- P, and ESP2015-672.... , 2019

Link: https://hdl.handle.net/20.500.12412/4712

RT Journal
T1 <Title>LISA Pathfinder micronewton cold gas thrusters: In-flight characterization</Title>

UL https://suche.suub.uni-bremen.de/peid=base-ftunivloyola:oai:repositorio.uloyola.es:20.500.12412_4712&Exemplar=1&LAN=DE
				
A1 Armano, M
A1 Audley, H
A1 Baird, J
A1 Binetruy, P
A1 Born, M
A1 Bortoluzzi, D
A1 Castelli, E
A1 Cavalleri, A
A1 Cesarini, 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 Ferroni, V
A1 Fitzsimons, E. D
A1 Freschi, M
A1 Gesa, L
A1 Gibert, F
A1 Giardini, D
A1 Giusteri, R
A1 Grimani, C
A1 Grzymisch, J
A1 Harrison, I
A1 Heinzel, G
A1 Hewitson, M
A1 Hollington, D
A1 Hoyland, D
A1 Hueller, M
A1 Inchauspé, H
A1 Jennrich, O
A1 Jetzer, P
A1 Karnesis, N
A1 Kaune, B
A1 Korsakova, N
A1 Killow, C. J
A1 Lobo, J. A
A1 Lloro, I
A1 Liu, L
A1 López Zaragoza, J. P
A1 Maarschalkerweerd, R
A1 Mance, D
A1 Meshksar, N
A1 Martín, V
A1 Martín Polo, L
A1 Martino, J
A1 Martín Porqueras, F
A1 Mateos, I
A1 McNamara, P. W
A1 Mendes, J
A1 Mendes, L
A1 Nofrarias, M
A1 Paczkowski, S
A1 Perreur Lloyd, M
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 Russano, G
A1 Slutsky, J
A1 Sopuerta, C. F
A1 Sumner, T
A1 Texier, D
A1 Thorpe, J. I
A1 Vetrugno, D
A1 Vitale, S
A1 Wanner, G
A1 Ward, H
A1 Wass, P. J
A1 Weber, W. J
A1 Wissel, L
A1 Wittchen, A
A1 Zweifel, P
A1 LISA Pathfinder Collaboration, /
YR 2019
JF This work has been made possible by the LISA Pathfinder mission, which is part of the space-science programme of the European Space Agency. The French contribution has been supported by the CNES (Accord Specifique de projet CNES 1316634/CNRS 103747), the CNRS, the Observatoire de Paris and the University Paris-Diderot. E. Plagnol and H. Inchausp´e would also like to acknowledge the financial support of the UnivEarthS Labex program at Sorbonne Paris Cit´e (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 Istituto Nazionale di Fisica Nucleare. The Spanish contribution has been supported by contracts AYA2010-15709 (MICINN), ESP2013-47637- P, and ESP2015-672...
LK http://dx.doi.org/https://hdl.handle.net/20.500.12412/4712
DO https://hdl.handle.net/20.500.12412/4712
SF ELIB - SuUB Bremen

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