Check the chronological order of apparition (not publication). Which are in the Rosetta stone?
1999→ M. Tinto and J. W. Armstrong, "Cancellation of Laser Noise in an Unequal-Arm Interferometer Detector of Gravitational Radiation", Phys. Rev. D 59, 102003 (1999). PRD→ J. W. Armstrong, F. B. Estabrook, and M. Tinto, "Time-Delay Interferometry for Space-Based Gravitational Wave Searches", Astrophys. J. 527, 814 (1999). ApJ
2000→ F. B. Estabrook, M. Tinto, and J. W. Armstrong, "Time-Delay Analysis of LISA Gravitational Wave Data: Elimination of Spacecraft Motion Effects", Phys. Rev. D. 62, 042002 (2000). PRD
2001→ M. Tinto, J. W. Armstrong, and F. B. Estabrook, "Discriminating a Gravitational Wave Background from Instrumental Noise in the LISA Detector", Phys Rev. D. 63, 021101(R) (2001). PRD→ J. W. Armstrong, F. B. Estabrook, and M. Tinto, "Sensitivities of Alternate LISA Configurations", Class. Quantum Grav. 18, 4059 (2001). CQG
2002→ M. Tinto, F. B. Estabrook, and J. W. Armstrong, "Time-Delay Interferometry for LISA", Phys. Rev. D 65, 082003 (2002). PRD→ S. V. Dhurandhar, K. Rajesh Nayak, and J.-Y. Vinet, "Algebraic Approach to Time-Delay Data Analysis for LISA", Phys. Rev. D. 65, 102002 (2002). PRD → T. A. Prince, M. Tinto, S. L. Larson, and J. W. Armstrong, "The LISA Optimum Sensitivity", Phys. Rev. D 66, 122002 (2002). PRD
2003→ J. W. Armstrong, F. B. Estabrook, and M. Tinto, "Time Delay Interferometry", Class. Quantum Grav. 20, S283 (2003). CQG→ N. J. Cornish and R. W. Hellings, "The Effects of Orbital Motion on LISA Time Delay Interferometry", Class. Quantum Grav. 20, 4851 (2003). CQG Show that modified-TDI Michelson-type observables cancel noise in rotating configurations; verify that first-generation Sagnac-type observables don't; propose 12-link Sagnac-type observables that do (including zeta); point out problem with modified-TDI Michelson-type in flexing configurations. → M. Tinto, D. Shaddock, J. Sylvestre, and J. W. Armstrong, "Implementation of Time Delay Interferometry for LISA", Phys Rev. D. 67, 122003 (2003). PRD → D. A. Shaddock, M. Tinto, F. B. Estabrook, and J. W. Armstrong, "Data Combinations Accounting for LISA Spacecraft Motion", Phys. Rev. D 68, 061303(R) (2003). PRD Discuss laser-noise cancellation problems with first-generation TDI in rotating and flexing configurations; define second-generation TDI Michelson-type and quasi-second-generation TDI Sagnac-type observables. → F. B. Estabrook, J. W. Armstrong, M. Tinto, and W. Folkner, "SyZyGy: A Straight Interferometer for Gravity Wave Detection", Phys. Rev. D 68, 062001 (2003). PRD → J. Sylvestre and M. Tinto, "Noise characterization for LISA", Phys. Rev. D 68, 102002 (2003). PRD → K. Rajesh Nayak, S. V. Dhurandhar, A. Pai, and J.-Y. Vinet, "Optimizing the directional sensitivity of LISA", Phys. Rev. D 68, 122001 (2003) PRD
2004→ D. A. Shaddock, "Operating LISA as a Sagnac interferometer," Phys. Rev. D 69, 022001 (2004). PRDDiscuss problem of Sagnac-type observables in rotating configurations; propose 12-link alpha-type observables that do. → M. Tinto, F. B. Estabrook, and J. W. Armstrong, "Time delay interferometry with moving spacecraft arrays," Phys. Rev. D 69, 082001 (2004). PRD Extend second-generation TDI to all other six-oriented-arm observables, and to zeta. → A. Królak, M. Tinto, and M. Vallisneri, "Optimal filtering of the LISA data", Phys. Rev. D 70, 022003 (2004). PRD → M. Tinto and S. L. Larson, "LISA time-delay interferometry zero-signal solution: Geometrical properties", Phys. Rev. D 70, 062002 (2004). PRD → D. A. Shaddock, B. Ware, R. E. Spero, and M. Vallisneri, "Post-processed time-delay interferometry for LISA", Phys. Rev. D 70, 081101(R) (2004) PRD
2005→ D. Summers and D. Hoyland, "Results from the LISA phase measurement system project," Class. Quantum Grav. 22 S249 (2005). CQG→ M. Vallisneri, "Synthetic LISA: Simulating Time Delay Interferometry in a Model LISA", Phys. Rev. D 71, 022001 (2005). PRD → M. Tinto, M. Vallisneri, and J. W. Armstrong, ‘TDIR: Time-Delay Interferometric Ranging for space-borne gravitational-wave detectors’, Phys. Rev. D 71, 041101(R) (2005). PRD → M. Vallisneri, ‘Geometric Time Delay Interferometry’, Phys. Rev. D 72, 042003 (2005). PRD → B. Chauvineau, T. Regimbau, J.-Y. Vinet, and S. Pireaux, "Relativistic analysis of the LISA long range optical links", Phys. Rev. D 72, 122003 (2005). PRD → M. Tinto and S. V. Dhurandhar, "Time-Delay Interferometry", Living Rev. Relativity 8, 4 (2005). Living Reviews |