Search Results - "Cameron, W. Doug"

Visible Opacity of M Dwarfs and Hot Jupiters: The TiO B 3Π−X 3Δ Band System by Doug Cameron, W., Bernath, Peter

“…The TiO B 3 Π − X 3 Δ electronic transition ( γ ′ system) is an important opacity source in the atmospheres of M dwarfs and hot Jupiter exoplanets. The 0–0,…”
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Near-infrared Opacity of Late M Dwarfs and Hot Jupiters: The E3Π–X3Δ Transition of TiO by Bernath, Peter, Cameron, W Doug

“…The TiO E 3Π–X 3Δ transition is an important opacity source in the near-infrared spectra of late M dwarfs. The 0–0 band of the 48Ti16O E 3Π–X 3Δ electronic…”
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Visible Opacity of M Dwarfs and Hot Jupiters: The TiO B3Π−X3Δ Band System by Cameron, W Doug, Bernath, Peter

“…The TiO B3Π − X3Δ electronic transition (γ′ system) is an important opacity source in the atmospheres of M dwarfs and hot Jupiter exoplanets. The 0–0, 1–0, and…”
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Near-infrared Opacity of Late M Dwarfs and Hot Jupiters: The E 3 Π–X 3 Δ Transition of TiO by Bernath, Peter, Cameron, W. Doug

“…The TiO E 3 Π– X 3 Δ transition is an important opacity source in the near-infrared spectra of late M dwarfs. The 0–0 band of the 48 Ti 16 O E 3 Π– X 3 Δ…”
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Near-infrared Opacity of Late M Dwarfs and Hot Jupiters: The E3 -X3Δ Transition of TiO by Bernath, Peter, Cameron, W. Doug

“…The TiO E3 -X3Δ transition is an important opacity source in the near-infrared spectra of late M dwarfs. The 0-0 band of the 48Ti16O E3 -X3Δ electronic…”
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Absorption cross sections of n-butane, n-pentane, cyclopentane and cyclohexane by Sorensen, Jason J., Bernath, Peter F., Johnson, Ryan M., Dodangodage, Randika, Cameron, W. Doug, LaBelle, Keith

“…•High resolution infrared Fourier transform spectroscopy.•Absorption cross sections of n-butane, n-pentane, cyclopentane and cyclohexane.•For remote sensing in…”
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