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

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CH 4 : Matrix diagonalization (Symmetry representation) 1,000,000 elements A1 A2 E E F 1 … 0 … 1,000,000 elements F 1 F 1 … 0 … F 2 F 2 F 2 T d (M) gns = 5 gns = 5 g ns = 2 g ns = 3 g ns = 3
C s C 2v C 3v D 3h C 2h … … Structure of the sub-matrix: ΔK=±2 factorization (J=8) K=0 K=1 K=2 K=3 … 0 … K=4 K=5 … 0 … K=6 K=7 K=8 Td (M)
Page 2: Cool atmospheres: dominated by mole
Page 5 and 6: 2012: (nearly) every star has plane
Page 7 and 8: HD189733b: Primary transit with Spi
Page 9 and 10: Pont et al., 2007 Swain et al., 200
Page 11 and 12: Exoplanet Characterisation Observat
Page 13 and 14: Why theory, not experiment?
Page 15 and 16: Absorption (T=300K) spectrum of NH
Page 17 and 18: Absorption (T=300K) spectrum of NH
Page 19 and 20: Completeness: Absorption of ammonia
Page 21 and 22: Ab initio calculations DMS PES Rovi
Page 23 and 24: Line list (in progress): C 2 Potent
Page 25 and 26: Potential energy Ab initio: solve f
Page 27: CH 4 : Matrix diagonalization (Symm
Page 31 and 32: Absorption of Methane (T=300 K) Int
Page 34 and 35: Energy file: N J sym n E/cm -1 v 1
Page 36 and 37: Obs: A. Coppalle & P. Vervisch, JQS
Page 38 and 39: Cross sections for NH 3 ν 2 band a
Page 40 and 41: As well as..... Remote detection of

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

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