TPF-I SWG Report - Exoplanet Exploration Program - NASA

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A PPENDIX E Appendix E TPF-I Review Papers The following publications provide a broad overview of progress with technology development for TPF-I since 2002. The papers are listed in reverse chronological order. Lawson, P. R., Ahmed, A., Gappinger, R. O., Ksendzov, A., Lay, O. P., Martin, S. R., Peters, R. D., Scharf, D. P., Wallace, J. K., and Ware, B., “Terrestrial Planet Finder Interferometer: Technology status and plans,” Advances in Stellar Interferometry, Proc. SPIE 6268, edited by J. D. Monnier, M. Schöller, and W. C. Danchi, 626828 (2006). Beichman, C., Lawson, P., Lay, O., Ahmed, A., Unwin, S., Johnston, K., “Status of the Terrestrial Planet Finder Interferometer,” Advances in Stellar Interferometry, Proc. SPIE 6268, edited by J. D. Monnier, M. Schöller, and W. C. Danchi, 62680S (2006). Henry, C., “Terrestrial Planet Finder Interferometer 2005: Overview of system design studies and technology development,” in Techniques and Instrumentation for Detection of Exoplanets II, edited by D. R. Coulter, Proc. SPIE 5905, 1–7 (2005). Henry, C., Lay, O. P., Aung, M., Gunter, S. M., Dubovitsky, S., and Blackwood, G. H., “Terrestrial Planet Finder interferometer: Architecture, mission design, and technology development,” New Frontiers in Stellar Interferometry, Proc. SPIE 5491, edited by W. A. Traub, 265–274 (2004). Blackwood, G. H., Serabyn, E., Dubovitsky, S., Aung, M., Gunter, S. M., Henry, C., “System design and technology development for the Terrestrial Planet Finder infrared interferometer,” Techniques and Instrumentation for Detection of Exoplanets, Proc. SPIE 5170, edited by D. R. Coulter, 129-143 (2003). Beichman, C. A., Coulter, D. R., Lindensmith, C., Lawson, P. R., “Selected mission architectures for the Terrestrial Planet Finder (TPF): Large, Medium, and Small,” Future Research Direction and Visions for Astronomy, Proc. SPIE 4835, edited by A. M. Dressler, 115–121 (2002). 194
C ONTRIBUTORS AND C REDITS Appendix F Contributors and Credits The editors are grateful to the individuals who were responsible for specific chapters, as listed below. Introduction Charles Beichman, California Institute of Technology Kenneth J. Johnston, U.S. Naval Observatory Peter R. Lawson, Jet Propulsion Laboratory Oliver P. Lay, Jet Propulsion Laboratory Exoplanet Science Charles A. Beichman, California Institute of Technology Kenneth J. Johnston, U.S. Naval Observatory John Bally, University of Colorado David Crisp, Jet Propulsion Laboratory Lisa Kaltenegger, Smithsonian Astrophysical Observatory Peter R. Lawson, Jet Propulsion Laboratory Oliver P. Lay, Jet Propulsion Laboratory Huub Röttgering, University of Leiden Eugene Serabyn, Jet Propulsion Laboratory Transforming Astrophysics with TPF-I John Bally, University of Colorado Huub Röttgering, University of Leiden Charles Beichman, California Institute of Technology Maria-Rosa Cioni, University of Edinburgh, UK Malcolm Fridlund, European Space Agency Roland den Hartogg, European Space Agency Jan-Willem den Herder, Space Research Organization Netherlands M. Hoogerheijde, University of Leiden Ivo Labbé, Carnegie Observatories, Pasadena Oliver Lay, Jet Propulsion Laboratory Réne Liseau, Stockholm University 195
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JPL Publication 07-1 Terrestrial Pl
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Abstract Over the past two years, t
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Acknowledgements Twenty-two represe
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Table of Contents 1 Introduction...
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4.8.3 Post-Nulling Calibration.....
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6.4.5 Double Fourier Interferometry
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I NTRODUCTION 1 Introduction Over 2
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I NTRODUCTION et al. 2004), and res
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I NTRODUCTION Standard Interferomet
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I NTRODUCTION 1.4 References Angel,
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C HAPTER 2 0.7 to 1.5 AU scaled by
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C HAPTER 2 Table 2-2. Illustrative
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C HAPTER 2 Classical interferometry
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C HAPTER 2 trivial in the absence o
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C HAPTER 2 Figure 2-3. Simulated mi
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C HAPTER 2 would be in atmospheres
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C HAPTER 2 Figure 2-6. The mid-infr
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C HAPTER 2 Lines of constant stella
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C HAPTER 2 presence of zodiacal clo
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C HAPTER 2 S EZ 2π ∫ θ max ∫
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C HAPTER 2 Figure 2-11. Observation
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C HAPTER 2 Figure 2-12. Models of t
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C HAPTER 2 Beichman, C. A., Fridlun
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C HAPTER 2 2.7.4 Suitable Targets E
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C HAPTER 2 Reach, W. T., Franz, B.
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C HAPTER 3 3.1.1 Darwin/TPF-I Prope
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C HAPTER 3 clouds or an OB associat
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C HAPTER 3 Figure 3-3. Three possib
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C HAPTER 3 the circumstellar disk,
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C HAPTER 3 Figure 3-6. (Left panel)
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C HAPTER 3 Continuum interferometry
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C HAPTER 3 Figure 3-9: Simulated im
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C HAPTER 3 3.3 Conclusions Darwin/T
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C HAPTER 3 Nguyen, H. T., Kallivaya
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D ESIGN AND A R C H I T E C T U R E
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C HAPTER 5 Heavy launch vehicle. Th
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C HAPTER 5 5.3.2 Combiner Spacecraf
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C HAPTER 5 5.3.5 Beam Transfer betw
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C HAPTER 5 Figure 5-8. Control sche
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C HAPTER 5 Figure 5-9. First sectio
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C HAPTER 5 Figure 5-9 shows the fir
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C HAPTER 5 5.4.4 Shear Metrology Sh
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C HAPTER 5 Figure 5-15. TPF-I Fligh
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C HAPTER 5 secondary mirror along t
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C HAPTER 5 a) c) b) d) IWA = 43 mas
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C HAPTER 5 planets found. Figure 5-
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C HAPTER 5 30 25 5 M earth 3 M eart
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C HAPTER 5 5.8.4 Angular Resolution
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C HAPTER 5 Table 5-3. Angular Resol
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C HAPTER 5 The optimization works b
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T E C H N O L O G Y R OADMAP FOR TP
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Page 157 and 158: T E C H N O L O G Y R OADMAP FOR TP
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