"undereddened" meaning in English

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  "etymology_text": "From un- + dereddened.",
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      "expansion": "undereddened (not comparable)",
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  "lang": "English",
  "lang_code": "en",
  "pos": "adj",
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      "examples": [
        {
          "bold_text_offsets": [
            [
              72,
              84
            ]
          ],
          "ref": "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 288:",
          "text": "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.",
          "type": "quote"
        },
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              73,
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          "ref": "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 211:",
          "text": "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.",
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          "ref": "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:",
          "text": "Note 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.",
          "type": "quote"
        }
      ],
      "glosses": [
        "Not dereddened."
      ],
      "id": "en-undereddened-en-adj-JgufAWOG",
      "links": [
        [
          "dereddened",
          "dereddened"
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      ],
      "tags": [
        "not-comparable"
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  "word": "undereddened"
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  "etymology_text": "From un- + dereddened.",
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  "lang_code": "en",
  "pos": "adj",
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          "ref": "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 288:",
          "text": "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.",
          "type": "quote"
        },
        {
          "bold_text_offsets": [
            [
              73,
              85
            ]
          ],
          "ref": "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 211:",
          "text": "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.",
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        {
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          "ref": "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:",
          "text": "Note 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.",
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      ],
      "glosses": [
        "Not dereddened."
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          "dereddened"
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  "word": "undereddened"
}