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Planetary transits

Planetary transits. Sherwood observatory. First transiting exoplanet: HD209458b. Henry et al. 2000, ApJ 529, L41 Charbonneau et al. 2000, ApJ 529, L45. Wide Angle Search for Planets (WASP). Mass-radius relation. Jupiter. Pont et al. 2005. Charbonneau et al 2007, ApJ 658, 1327.

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Planetary transits

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  1. Planetary transits Sherwood observatory

  2. First transiting exoplanet: HD209458b Henry et al. 2000, ApJ 529, L41 Charbonneau et al. 2000, ApJ 529, L45

  3. Wide Angle Search for Planets (WASP)

  4. Mass-radius relation Jupiter

  5. Pont et al. 2005

  6. Charbonneau et al 2007, ApJ 658, 1327

  7. Pollacco et al. 2008

  8. Composition of solar system planets Stevenson 1982 AREPS 10, 257

  9. Gillon et al. 2007

  10. Transits from space: CoRoT-7b Leger et al. 2009

  11. Kepler

  12. Keith Horne

  13. HD209458b with HST Brown et al. 2001, ApJ 529, L41

  14. Transmission spectroscopy Brown 2001

  15. Detection of sodium in the atmosphere of HD209458b Charbonneau et al. 2002 ApJ 568, 377

  16. Detection of sodium in the atmosphere of HD209458b Charbonneau et al. 2002 ApJ 568, 377

  17. HD209458b Sing et al. 2008 ApJ 686 658 Transmission spectroscopy with HST Pont et al. 2008 MNRAS 385 109 HD189733b

  18. Evaporation of HD209458b Vidal-Madjar et al 2003, Nature 422, 143

  19. The Sun in X-rays Lx < 10-3 LBol

  20. Rossiter-McLaughlin effect

  21. Radial Velocity of 51 Peg b Mayor & Queloz 1995, Nature 378, 23

  22. Rossiter-McLaughlin effect in HD 209458 Measures spin of star Shows 4deg misaligned but same direction as planet orbit Winn et al 2005 ApJ 631, 1215

  23. Retrograde orbit of WASP-17b Anderson et al. 2009

  24. Secondary eclipses Spitzer Space Telescope

  25. HD 209458 at 24 microns Deming et al 2005 Nature 434, 740 Eclipse depth 0.26%

  26. HD209458b at a range of wavelengths Knutson et al. 2008 ApJ 673, 526

  27. CO H20 H20 Knutson et al. 2008, ApJ 673, 526 Temperature inversion in HD209458b

  28. Burrows, Sudarsky & Hubeny 2006 Temperature inversion due to TiO opacity? 4.5 microns 8 microns with Tio/VO without TiO/VO

  29. HD189733b around half an orbitKnutson et al. 2007, Nature 447, 183

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