文档介绍:Cardelli, J. A., Clayton, G. C. & Mathis, J. S. 1989. The Relationship between Infrared, Optical, and Ultraviolet Extinction. Astrophysical Journal 345:245-256.
D'Agostini, G. 2005. Fits, and Especially Linear Fits, with Errors on Both Axes, Extra Variance of the Data Points and Other Complications. arXiv:physics/0511182. [D05]
Draine, B. T. 2000. Gamma-Ray Bursts in Molecular Clouds: H2 Absorption and Fluorescence. Astrophysical Journal 532:273-280.
Fan, X., et al. 2006. Constraining the Evolution of the Ionizing Background and the Epoch of Reionization with z~6 Quasars. II. A Sample of 19 Quasars. Astronomical Journal 132:117-136.
Fitzpatrick, E. L. & Massa, D. 1988. An Analysis of the Shapes of Ultraviolet Extinction Curves. II - The Far-UV extinction. Astrophysical Journal 328:734-746.
Fitzpatrick, E. L. & Massa, D. 1990. An Analysis of the Shapes of Ultraviolet Extinction Curves. III - An Atlas of Ultraviolet Extinction Curves. Astrophysical Journal Supplement Series 72:163-189.
Gordon, K. D., Clayton, G. C., Misselt, K. A., Landolt, A. U. & Wolff, M. J. 2003. A Quantitative Comparison of the Small Magellanic Cloud, Large Magellanic Cloud, and Milky Way Ultraviolet to Near-Infrared Extinction Curves. Astrophysical Journal 594:279-293.
Reichart, D. E. 2001. Dust Extinction Curves and Lyα Forest Flux Deficits for Use in Modeling Gamma-Ray Burst Afterglows and All Other Extra