Ultraviolet Background Emissivity

Ultraviolet Background Emissivity is a radiative property that quantifies the intrinsic emission rate of ultraviolet photons per unit volume, wavelength, and time from diffuse sources in the intergalactic medium, distinguishing it from related radiative transfer quantities by characterizing the specific contribution of pervasive, non-local sources to the cosmic ultraviolet background radiation field.

36

Publications

2K

Citations

118

Authors

74

Institutions

Publications per year

2017–2026

9

Authors

118

  1. MG
    Martin G. Haehnelt

    University of Cambridge, United Kingdom

    2 publications · 194 citations

    2

    h-index

  2. SL
    Seong-Kook Lee

    Seoul National University, South Korea

    1 publications · 19 citations

    1

    h-index

  3. SH
    Sungyong Hwang

    Peking University, China

    1 publications · 19 citations

    1

    h-index

  4. JS
    James S. Bolton

    University of Nottingham, United Kingdom

    1 publications · 315 citations

    1

    h-index

  5. DC
    David C. Catling

    University of Washington, United States

    1 publications · 139 citations

    1

    h-index

1–5 of 118

Venues

  1. 10

    h-index

  2. The Astrophysical Journal

    ApJ · 5 publications · 152 citations

    5

    h-index

  3. Planetary and Space Science

    3 publications · 211 citations

    3

    h-index

  4. Journal of Physics E Scientific Instruments

    2 publications · 52 citations

    2

    h-index

  5. Journal of Non-Crystalline Solids

    1 publications · 24 citations

    1

    h-index

1–5