Jonathan Tennyson Molecular Line Lists for Exoplanets and Other ...

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Cool atmospheres: dominated by molecular absorption The molecular opacity problem M-dwarf <strong>Exoplanets</strong>? M Dwarf Brown Dwarfs Planet Marley & Leggett (2008)
Page 4 and 5: Sub-stellar objects: CO less import
Page 6 and 7: Radial velocity / Occultation HD 20
Page 8 and 9: Tinetti et al., Nature, 448, 163 (2
Page 10 and 11: Giovanna Tinetti, UCL So far discov
Page 12 and 13: Molecular line lists for exoplanet
Page 14 and 15: Exoplanets
Page 16 and 17: Absorption (T=300K) spectrum of NH
Page 18 and 19: Absorption (T=300K) spectrum of NH
Page 20 and 21: Intensity / [cm/mole] Absorption sp
Page 22 and 23: Ab initio: solve for motion of elec
Page 24 and 25: 300 K line list, Clara Sousa-Silva
Page 26 and 27: Intensity (cm/molecule) 1x10 -20 1x
Page 28 and 29: CH 4 : Matrix diagonalization (Symm
Page 30 and 31: Intensity (cm/molecule) 2x10 -19 1x
Page 32: Absorption spectra of CH 4 : Temper
Page 35 and 36: Transitions file: N f N i A if 12.8
Page 37 and 38: ExoCross: T-dependent cross section
Page 39 and 40: Brown and M-dwarfs Atmosphere of Ve
Page 41: Molecular line lists for exoplanet

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