Infrared Luminosity Density

Infrared Luminosity Density is a cosmological observable representing the total infrared luminosity emitted per unit comoving volume in the universe, distinguishing itself from other luminosity densities by its specific measurement of reprocessed starlight in the infrared band arising from dust-obscured star formation.

57

Publications

5.4K

Citations

359

Authors

215

Institutions

Publications per year

2017–2026

9

Authors

359

  1. EL
    E. Le Floc’h

    Commissariat à l'Énergie Atomique et aux Énergies Alternatives, France

    8 publications · 2K citations

    8

    h-index

  2. TT
    Tsutomu T. Takeuchi

    Nagoya University, Japan

    5 publications · 320 citations

    5

    h-index

  3. HI
    Hanae Inami

    Leiden University, Netherlands

    5 publications · 477 citations

    5

    h-index

  4. TG
    Tomotsugu Goto

    National Tsing Hua University, Taiwan

    4 publications · 232 citations

    4

    h-index

  5. GL
    G. Lagache

    Centre National de la Recherche Scientifique, France

    4 publications · 1.7K citations

    4

    h-index

1–5 of 359

Venues

  1. The Astrophysical Journal

    ApJ · 22 publications · 3.4K citations

    20

    h-index

  2. Astronomy and Astrophysics

    9 publications · 506 citations

    9

    h-index

  3. 6

    h-index

  4. The Astrophysical Journal Letters

    3 publications · 114 citations

    3

    h-index

  5. CERN Document Server (European Organization for Nuclear Research)

    Repository · 3 publications · 100 citations

    3

    h-index

1–5