Integral Field Spectroscopy

Integral Field Spectroscopy is a spectroscopic technique in astronomical instrumentation that, unlike conventional spectroscopy, simultaneously acquires spatially resolved spectra across a two-dimensional field of view by employing an array of spatial elements to sample the target region in three dimensions (two spatial and one spectral).

1.3K

Publications

80.7K

Citations

5.2K

Authors

900

Institutions

Publications per year

2017–2026

431

Authors

5.2K

  1. SF
    S. F. Sánchez

    Universidad Nacional Autónoma de México, Mexico

    86 publications · 7.1K citations

    48

    h-index

  2. JB
    Joss Bland‐Hawthorn

    The University of Sydney, Australia

    57 publications · 5K citations

    38

    h-index

  3. SA
    Santiago Arribas

    Centro de Astrobiología, Spain

    61 publications · 3.9K citations

    33

    h-index

  4. RB
    Roland Bacon

    Université Claude Bernard Lyon 1, France

    50 publications · 4.4K citations

    32

    h-index

  5. LW
    L. Wisotzki

    Leibniz Institute for Astrophysics Potsdam, Germany

    39 publications · 3.4K citations

    32

    h-index

1–5 of 5.2K

Venues

  1. Astronomy and Astrophysics

    253 publications · 16.8K citations

    73

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    313 publications · 20K citations

    73

    h-index

  3. The Astrophysical Journal

    ApJ · 171 publications · 15.3K citations

    66

    h-index

  4. 36

    h-index

  5. The Astronomical Journal

    AJ · 39 publications · 2.8K citations

    24

    h-index

1–5