Photometric Sensitivity

Photometric Sensitivity is the minimum detectable flux or radiant power of electromagnetic radiation in specific infrared wavelengths that a space-based infrared observatory can reliably measure, distinguishing it from other observational capabilities by quantifying the instrument's ability to detect weak astronomical sources under given noise conditions.

101

Publications

4.1K

Citations

523

Authors

241

Institutions

Publications per year

2017–2026

13

Authors

523

  1. BM
    B. M. Swinyard

    Rutherford Appleton Laboratory, United Kingdom

    4 publications · 65 citations

    4

    h-index

  2. GD
    G. Djurašević

    Astronomical Observatory, Serbia

    3 publications · 156 citations

    3

    h-index

  3. KJ
    K. J. King

    Cardiff University, United Kingdom

    2 publications · 34 citations

    2

    h-index

  4. VP
    Victor Pollak

    University of Saskatchewan, Canada

    2 publications · 43 citations

    2

    h-index

  5. JG
    Jason Glenn

    University of Colorado Boulder, United States

    2 publications · 44 citations

    2

    h-index

1–5 of 523

Venues

  1. 8

    h-index

  2. Astrophysics and Space Science

    6 publications · 201 citations

    6

    h-index

  3. 6

    h-index

  4. Journal of the Optical Society of America

    JOSA · 6 publications · 411 citations

    6

    h-index

  5. Applied Optics

    4 publications · 171 citations

    4

    h-index

1–5