TPF-I SWG Report - Exoplanet Exploration Program - NASA

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C HAPTER 3 Nguyen, H. T., Kallivayalil, N., Werner, M. W., Alcock, C., Patten, B. M., and Stern, D., “Spitzer Space Telescope observations of the aftermath of microlensing event MACHO-LMC-5,” Astrophys. J. Supp. Ser. 154, 266–270 (2004). Reach, W. T., Kuchner, M. J., von Hippel, T., Burrows, A., Mullally, F., Kilic, M., and Winget, D. E., “The dust cloud around the white dwarf G29-38,” Astrophys. J. 635, L161–L164 (2005). Reid, M. J., and Menten, K. M., “Radio photospheres of long-period variable stars,” Astrophys. J. 476, 327–346 (1997). Reipurth, B., “Disintegrating multiple systems in early stellar evolution,” Astron. J. 120, 3177–3191 (2000). Reipurth, B., and Bally, J., “Herbig-Haro flows: Probes of early stellar evolution,” Ann. Rev. Astron. Astrophys. 39, 403–455 (2001). Rosati, P., Tozzi, P., Giacconi, R., et al., “Chandra Deep Field South: The 1 million second exposure,” Astrophys. J. 566, 667–674 (2002). Röttgering, H. J. A., D’Arcio, L., Eiroa, C., et al. “Astrophysical Imaging with the Darwin IR interferometer,” Towards Other Earths: Darwin/<strong>TPF</strong> and the Search for Extrasolar Terrestrial Planets, Proc. ESA-SP 539, European Space Agency: Noordwijk, The Netherlands, pp. 299–308 (2003). Sandin, C. and Höfner, S., “Three-component modeling of C-rich AGB star winds. I. Method and first results,” Astron. Astrophys. 398, 253–266 (2003). Siess, L., Dufour, E., and Forestini, M., “An internet server for pre-main sequence tracks of low- and intermediate-mass stars,” Astron. Astrophys. 358, 593–599 (2000). (http://astropc0.ulb.ac.be/~siess/index.html) Smail, I., Ivison, R. J., and Blain, A. W., “A deep sub-millimeter survey of lensing clusters: A new window on galaxy formation and evolution,” Astrophys. J. 490, L5–L8 (1997). Steidel, C. C., Adelberger, K. L., Giavalisco, M., Dickinson, M., and Pettini, M., “Lyman-break galaxies at z>4 and the evolution of the ultraviolet luminosity density at high redshift,” Astrophys. J. 519, 1–17 (1999). Tan, J. C., Krumholz, M. R., and McKee, C. F., “Equilibrium star cluster formation,” Astrophys. J. 641, L121–124 (2006). Tan, J. C, “The Becklin-Neugebauer Object as a runaway B star, ejected 4000 years ago from the θ1 Orionis C system,” Astrophys. J. 607, L47–L50 (2004). Throop, H. B., and Bally, J., “Can photoevaporation trigger planetesimal formation” Astrophys. J. 623, L149–L152 (2005). 56
G ENERAL A STROPHYSICS Venemans, B. P., Kurk, J. D., Miley, G. K., et al., “The most distant structure of galaxies known: A protocluster at z=4.1,” Astrophys. J. 569, L11–L14 (2002). Yusef-Zadeh, F., and Morris, M., “A windswept cometary tail on the Galactic supergiant IRS 7,” Astrophys. J. 371, L59–L62 (1991). Zijlstra A. A., Matsuura, M., Wood, P. R., et al., “A Spitzer mid-infrared spectral survey of mass-losing carbon stars in the Large Magellanic Cloud,” Mon. Not. R. Astron. Soc. 370, 1961–1978 (2006). 57
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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
Page 19 and 20: I NTRODUCTION Standard Interferomet
Page 21: I NTRODUCTION 1.4 References Angel,
Page 24 and 25: C HAPTER 2 0.7 to 1.5 AU scaled by
Page 26 and 27: C HAPTER 2 Table 2-2. Illustrative
Page 28 and 29: C HAPTER 2 Classical interferometry
Page 30 and 31: C HAPTER 2 trivial in the absence o
Page 32 and 33: C HAPTER 2 Figure 2-3. Simulated mi
Page 34 and 35: C HAPTER 2 would be in atmospheres
Page 36 and 37: C HAPTER 2 Figure 2-6. The mid-infr
Page 38 and 39: C HAPTER 2 Lines of constant stella
Page 40 and 41: C HAPTER 2 presence of zodiacal clo
Page 42 and 43: C HAPTER 2 S EZ 2π ∫ θ max ∫
Page 44 and 45: C HAPTER 2 Figure 2-11. Observation
Page 46 and 47: C HAPTER 2 Figure 2-12. Models of t
Page 48 and 49: C HAPTER 2 Beichman, C. A., Fridlun
Page 50 and 51: C HAPTER 2 2.7.4 Suitable Targets E
Page 52 and 53: C HAPTER 2 Reach, W. T., Franz, B.
Page 54 and 55: C HAPTER 3 3.1.1 Darwin/TPF-I Prope
Page 56 and 57: C HAPTER 3 clouds or an OB associat
Page 58 and 59: C HAPTER 3 Figure 3-3. Three possib
Page 60 and 61: C HAPTER 3 the circumstellar disk,
Page 62 and 63: C HAPTER 3 Figure 3-6. (Left panel)
Page 64 and 65: C HAPTER 3 Continuum interferometry
Page 66 and 67: C HAPTER 3 Figure 3-9: Simulated im
Page 68 and 69: C HAPTER 3 3.3 Conclusions Darwin/T
Page 73 and 74: D ESIGN AND A R C H I T E C T U R E
Page 111: D ESIGN AND A R C H I T E C T U R E
Page 114 and 115: C HAPTER 5 Heavy launch vehicle. Th
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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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F UTURE D EVELOPMENTS 7 Preparatory
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F UTURE D EVELOPMENTS • To comple
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F UTURE D EVELOPMENTS Table 7-1. Pr
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D ISCUSSION AND C ONCLUSION 8 Discu
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Appendices 167
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T E C H N O L O G Y A DVISORY C O M
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F L I G H T S YSTEM C ONFIGURATION
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F L I G H T S YSTEM C ONFIGURATION
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A PPENDIX C 2. Identical FACS fligh
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A PPENDIX C 2. Recall that the coef
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A PPENDIX C Once the formation has
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A PPENDIX C Figure C-3. Example of
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A PPENDIX C Figure C-4. FAST Flight
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A PPENDIX C The “true” time of
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A PPENDIX C References Cohen, S., a
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A PPENDIX D DC DCB DM DM DOCS DOD D
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A PPENDIX D NaCl NAR NASA NASTRAN N
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A PPENDIX E Appendix E TPF-I Review
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A PPENDIX F Alice Quillen, Universi
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A PPENDIX F Figure 3-1 - Original f
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