Instrumental Line Spread Function

The Instrumental Line Spread Function is a spectral response function that characterizes the finite resolution of an ultraviolet spectroscopic instrument by describing the distribution of measured intensity as a function of wavelength deviation from a monochromatic input line, thereby distinguishing it from other broadening mechanisms through its intrinsic dependence on the instrument's optical and detection characteristics.

43

Publications

3.6K

Citations

333

Authors

104

Institutions

Publications per year

2017–2026

13

Variants

Instrumental FunctionInstrumental ProfileLsf

Authors

333

  1. JW
    Ji Wang

    The Ohio State University, United States

    2 publications · 35 citations

    2

    h-index

  2. NJ
    Nemanja Jovanović

    California Institute of Technology, United States

    2 publications · 35 citations

    2

    h-index

  3. PM
    P. Montegriffo

    University of Cambridge, United Kingdom

    2 publications · 122 citations

    2

    h-index

  4. JW
    Jerry W. Xuan

    California Institute of Technology, United States

    2 publications · 35 citations

    2

    h-index

  5. JM
    J. M. Carrasco

    Universitat de Barcelona, Spain

    2 publications · 122 citations

    2

    h-index

1–5 of 333

Venues

  1. The Astrophysical Journal

    ApJ · 4 publications · 126 citations

    4

    h-index

  2. 4

    h-index

  3. Journal of Applied Crystallography

    3 publications · 142 citations

    3

    h-index

  4. Astronomy and Astrophysics

    2 publications · 529 citations

    2

    h-index

  5. The Astronomical Journal

    AJ · 2 publications · 129 citations

    2

    h-index

1–5