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Citation: R. Moreno et al., Jovian stratospheric temperature during the two months following the impacts of comet Shoemaker-Levy 9, PLANET SPAC, 49(5), 2001, pp. 473-486
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Citation: E. Lellouch et al., The 2.4-45 mu m spectrum of Mars observed with the Infrared Space Observatory, PLANET SPAC, 48(12-14), 2000, pp. 1393-1405
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Citation: C. Cottaz et al., Line positions and intensities in the 2 nu(2)/nu(4) vibrational system of (NH3)-N-14 near 5-7 mu m, J MOL SPECT, 203(2), 2000, pp. 285-309
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Citation: Mj. Burgdorf et al., ISO observations of Mars: An estimate of the water vapor vertical distribution and the surface emissivity, ICARUS, 145(1), 2000, pp. 79-90
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Citation: T. Fouchet et al., ISO-SWS observations of Jupiter: Measurement of the ammonia tropospheric profile and of the N-15/N-14 isotopic ratio, ICARUS, 143(2), 2000, pp. 223-243
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Citation: Ji. Moses et al., Photochemistry of Saturn's atmosphere - I. Hydrocarbon chemistry and comparisons with ISO observations, ICARUS, 143(2), 2000, pp. 244-298
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Citation: Ea. Bergin et al., Submillimeter Wave Astronomy Satellite observations of Jupiter and Saturn:Detection of 557 GHz water emission from the upper atmosphere, ASTROPHYS J, 539(2), 2000, pp. L147-L150
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Citation: T. Encrenaz et al., The ISO spectra of Uranus and Neptune between 2.5 and 4.2 mu m: constraints on albedos and H-3(+) (vol 358, pg L83, 2000), ASTRON ASTR, 362(3), 2000, pp. 1174-L87
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Citation: T. Encrenaz et al., The ISO spectra of Uranus and Neptune between 2.5 and 4.2 mu m: constraints on albedos and H-3(+), ASTRON ASTR, 358(3), 2000, pp. L83-L87
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Citation: T. Fouchet et al., Jupiter's hydrocarbons observed with ISO-SWS: vertical profiles of C2H6 and C2H2, detection of CH3C2H, ASTRON ASTR, 355(1), 2000, pp. L13-L17
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Citation: T. Encrenaz et al., The atmospheric composition and structure of Jupiter and Saturn from ISO observations: a preliminary review, PLANET SPAC, 47(10-11), 1999, pp. 1225-1242
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Citation: N. Jacquinet-husson et al., The 1997 spectroscopic GEISA databank, J QUAN SPEC, 62(2), 1999, pp. 205-254
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Citation: H. Feuchtgruber et al., Detection of HD in the atmospheres of Uranus and Neptune: a new determination of the D/H ratio, ASTRON ASTR, 341(1), 1999, pp. L17-L21