In-depth Analysis of LISA Pathfinder Performance Results: Time Evolution, Noise Projection, Physical Models, and Implications for LISA
M. Armano,H. Audley,J. Baird,P. Binetruy,M. Born,D. Bortoluzzi,E. Castelli,A. Cavalleri,A. Cesarini,V. Chiavegato,A. M. Cruise,D. Dal Bosco,K. Danzmann,M. De Deus Silva,I. Diepholz,G. Dixon,R. Dolesi,L. Ferraioli,V. Ferroni,E. D. Fitzsimons,M. Freschi,L. Gesa,D. Giardini,F. Gibert,R. Giusteri,C. Grimani,J. Grzymisch,I. Harrison,M. S. Hartig,G. Heinzel,M. Hewitson,D. Hollington,D. Hoyland,M. Hueller,H. Inchauspe,O. Jennrich,P. Jetzer,B. Johlander,N. Karnesis,B. Kaune,N. Korsakova,C. J. Killow,J. A. Lobo,J. P. Lopez-Zaragoza,R. Maarschalkerweerd,D. Mance,V. Martin,L. Martin-Polo,F. Martin-Porqueras,J. Martino,P. W. McNamara,J. Mendes,L. Mendes,N. Meshksar,M. Nofrarias,S. Paczkowski,M. Perreur-Lloyd,A. Petiteau,E. Plagnol,J. Ramos-Castro,J. Reiche,F. Rivas,D. I. Robertson,G. Russano,L. Sala,J. Slutsky,C. F. Sopuerta,T. Sumner,D. Texier,J. I. Thorpe,D. Vetrugno,S. Vitale,G. Wanner,H. Ward,P. Wass,W. J. Weber,L. Wissel,A. Wittchen,C. Zanoni,P. Zweifel PHYSICAL REVIEW D（2024）
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