Resolved Source Counts

Resolved Source Counts is a methodological construct in observational astrophysics that refers to the statistical enumeration of individually detected infrared-emitting celestial sources contributing to the Cosmic Infrared Background, distinguished by their angular resolution and flux density measurements from deep-field surveys.

18

Publications

1.8K

Citations

119

Authors

78

Institutions

Publications per year

2017–2026

3

Authors

119

  1. EL
    E. L. Wright

    University of California, Los Angeles, United States

    2 publications · 316 citations

    2

    h-index

  2. GL
    G. Lagache

    Centre National de la Recherche Scientifique, France

    2 publications · 422 citations

    2

    h-index

  3. KI
    K. I. Caputi

    Centre National de la Recherche Scientifique, France

    2 publications · 364 citations

    2

    h-index

  4. HD
    H. Dole

    Centre National de la Recherche Scientifique, France

    2 publications · 422 citations

    2

    h-index

  5. JD
    J. D. Vieira

    California Institute of Technology, United States

    1 publications · 33 citations

    1

    h-index

1–5 of 119

Venues

  1. The Astrophysical Journal

    ApJ · 4 publications · 148 citations

    4

    h-index

  2. 3

    h-index

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

    Repository · 2 publications · 303 citations

    2

    h-index

  4. Astronomy and Astrophysics

    2 publications · 183 citations

    2

    h-index

  5. The Astrophysical Journal Supplement Series

    2 publications · 517 citations

    2

    h-index

1–5