Unresolved Source Contributions

Unresolved Source Contributions is a type of astrophysical emission component in diffuse gamma-ray background models that consists of the cumulative radiation from numerous faint or distant point sources below the detection threshold of current instruments, thereby indistinguishable from truly diffuse processes.

149

Publications

8.4K

Citations

1.1K

Authors

369

Institutions

Publications per year

2017–2026

43

Authors

1.1K

  1. QY
    Qi Ying

    Texas A&M University, United States

    4 publications · 413 citations

    4

    h-index

  2. MR
    M. R. Hogerheijde

    Leiden University, Netherlands

    3 publications · 144 citations

    3

    h-index

  3. ML
    Mariangela Lisanti

    Princeton University, United States

    3 publications · 413 citations

    3

    h-index

  4. NL
    Nicholas L. Rodd

    Lawrence Berkeley National Laboratory, United States

    3 publications · 159 citations

    3

    h-index

  5. GA
    Geoffrey A. Blake

    California Institute of Technology, United States

    3 publications · 144 citations

    3

    h-index

1–5 of 1.1K

Venues

  1. The Astrophysical Journal

    ApJ · 35 publications · 2K citations

    26

    h-index

  2. 14

    h-index

  3. Atmospheric Environment

    10 publications · 657 citations

    10

    h-index

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

    Repository · 7 publications · 346 citations

    7

    h-index

  5. The Astronomical Journal

    AJ · 6 publications · 210 citations

    6

    h-index

1–5