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Astrophysical Journal, Supplement Series, 1990 The basic data needed to produce UV extinction curves for a sample of 78 stars, including spectral types, visual photometry, parameters used to produce fits to the UV extinction curves, distances to the program stars, and line-of-sight H I column densities, are presented.
Derck Massa
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Extinction in the far ultraviolet
Physica, 1969Interstellar grain model consisting of elongated dielectric particles represented by infinite circular cylinders reproducing observed interstellar extinction in IF far UV ...
J.M. Greenberg, G.A. Shah
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Far-ultraviolet extinction in σ Scorpii
Astrophysics and Space Science, 1975It was found earlier from OAO-2 data (Bless and Savage, 1972) that considerable variability with direction in space is present in both the shape and level (relative to B-V color excess) of the interstellar extinction curve in the far ultraviolet. The star σ Sco was shown to be a case of extremely low UV extinction, but there was some question of ...
Theodore P. Snow, Donald G. York
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Empirical extinction coefficients for the Swift-UVOT optical-through-ultraviolet passbands
Monthly Notices of the Royal Astronomical Society, 2023 We calculated empirical reddening and extinction coefficients with respect to the dust reddening map of Schlegel et al. for the Swift-UVOT passbands, using the 'star pair' method and photometric data from the UVOT Serendipitous Source Catalogue and ...
Ruoyi Zhang
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