Unresolved Source Fluctuations

Unresolved Source Fluctuations is a type of spatial intensity variation observed in deep cosmic infrared background measurements that arises from the collective, sub-threshold emission of faint, undetected astrophysical sources rather than from resolved individual objects or diffuse primordial radiation.

28

Publications

1.2K

Citations

102

Authors

69

Institutions

Publications per year

2017–2026

4

Authors

102

  1. AK
    A. Kashlinsky

    Goddard Space Flight Center, United States

    4 publications · 304 citations

    4

    h-index

  2. RG
    Richard G. Arendt

    Goddard Space Flight Center, United States

    4 publications · 304 citations

    4

    h-index

  3. SH
    S. H. Moseley

    Goddard Space Flight Center, United States

    3 publications · 230 citations

    3

    h-index

  4. RC
    Ranga‐Ram Chary

    California Institute of Technology, United States

    2 publications · 56 citations

    2

    h-index

  5. GG
    G. G. Fazio

    Center for Astrophysics Harvard & Smithsonian, United States

    2 publications · 216 citations

    2

    h-index

1–5 of 102

Venues

  1. The Astrophysical Journal

    ApJ · 10 publications · 679 citations

    10

    h-index

  2. 8

    h-index

  3. Infrared Physics

    1 publications · 12 citations

    1

    h-index

  4. Astronomy and Astrophysics

    1 publications · 33 citations

    1

    h-index

  5. Planetary and Space Science

    1 publications · 24 citations

    1

    h-index

1–5