Foreground Reddening

Foreground Reddening is a type of interstellar extinction process in which ultraviolet radiation from distant astronomical sources is preferentially absorbed and scattered by intervening dust and gas located between the observer and the source, leading to an observed reddening of the source's spectrum.

97

Publications

4.7K

Citations

465

Authors

258

Institutions

Publications per year

2017–2026

11

Authors

465

  1. AV
    A. V. Ahumada

    Argentine National Observatory, Argentina

    3 publications · 50 citations

    3

    h-index

  2. EB
    E. Bica

    Universidade Federal do Rio Grande do Sul, Brazil

    3 publications · 67 citations

    3

    h-index

  3. KO
    Knut Olsen

    Cerro Tololo Inter-American Observatory, Chile

    3 publications · 52 citations

    3

    h-index

  4. SS
    Smitha Subramanian

    Indian Institute of Astrophysics, India

    3 publications · 96 citations

    3

    h-index

  5. WE
    William E. Harris

    McMaster University, Canada

    2 publications · 35 citations

    2

    h-index

1–5 of 465

Venues

  1. The Astrophysical Journal

    ApJ · 28 publications · 1.5K citations

    20

    h-index

  2. The Astronomical Journal

    AJ · 14 publications · 560 citations

    14

    h-index

  3. 12

    h-index

  4. Astronomy and Astrophysics

    12 publications · 614 citations

    11

    h-index

  5. Publications of the Astronomical Society of the Pacific

    PASP · 5 publications · 133 citations

    5

    h-index

1–5