Meanings
- not comparableNot dereddened.
A good rectification of the 2200 A dip, which is clearly visible in the undereddened spectrum, is obtained for 0.4<E_(B-V)<0.5.
1981, L. Chiappetti, L. Maraschi, E.G. Tanzi, A. Treves, “Ultraviolet Study of V1341 Cyg = Cyg X-2. Observation of an Accretion Disk”, in R[olf] D. Andresen, editor, X-Ray Astronomy: Proceedings of the XV ESLAB Symposium Held in Amsterdam, […], Dordrecht: D. Reidel Publishing Company, →OCLC, session 4 (Galactic Astronomy: SNR and Other Galactic Sources), page 2882 more examples
The linear fit gives A = 0.067 ± 10⁻³; B = 6.77 ± 0.04; σ = 0.17 for the undereddened sample with (B − V) > −0.09 and |(d− < d >)| ≤ 1.5Σ.
1989, M. Alongi, C. Chiosi, “LMC Star Clusters: Age Calibrations and Mass Estimates”, in Astrophysical Ages and Dating Methods: Proceedings of the Fifth IAP Workshop, Gif-sur-Yvette: Editions Frontières, published 1990, →ISBN, part III (Stellar Ages: Magellanic Clouds), page 211Note that Jones et al. 1992 actually consider 17 type ab RR Lyrae stars, but we are unable to reconstruct the undereddened photometry for one of these, SS Leo, from their sources, Liu & Janes 1990 and Jones, Carney, & Latham 1988.
1998, Andrew Gould, Piotr Popowski, “Systematics of RR Lyrae Statistical Parallax III: Apparent Magnitudes and Extinctions”, in The Astrophysical Journal, Bristol: IOP Publishing for the American Astronomical Society, →ISSN, →OCLC, page 9
Origin
Cite this entry
undereddened. (n.d.). In WatkinsX Dictionary. Retrieved November 3, 2026, from https://dictionary.watkinsx.com/word/undereddened
“undereddened.” WatkinsX Dictionary, https://dictionary.watkinsx.com/word/undereddened. Accessed November 3, 2026.
WatkinsX Dictionary, s.v. “undereddened,” accessed November 3, 2026, https://dictionary.watkinsx.com/word/undereddened.
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