Sky Background Subtraction

Sky Background Subtraction is a data processing technique in near-infrared astronomy that distinguishes itself from other photometric correction methods by selectively removing diffuse atmospheric and thermal emission contributions from observational frames to isolate the true flux of celestial sources.

402

Publications

31.4K

Citations

2.5K

Authors

640

Institutions

Publications per year

2017–2026

83

Authors

2.5K

  1. RH
    Robert H. Lupton

    Princeton University, United States

    8 publications · 4.4K citations

    8

    h-index

  2. JB
    Joss Bland‐Hawthorn

    The University of Sydney, Australia

    7 publications · 857 citations

    7

    h-index

  3. JL
    Jon Lawrence

    Australian Astronomical Observatory, Australia

    7 publications · 451 citations

    7

    h-index

  4. DJ
    David J. Schlegel

    Lawrence Berkeley National Laboratory, United States

    7 publications · 4.3K citations

    7

    h-index

  5. JB
    J. Brinkmann

    Princeton University, United States

    6 publications · 3.7K citations

    6

    h-index

1–5 of 2.5K

Venues

  1. The Astrophysical Journal

    ApJ · 68 publications · 6K citations

    35

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    67 publications · 5.3K citations

    34

    h-index

  3. Astronomy and Astrophysics

    31 publications · 2K citations

    22

    h-index

  4. The Astronomical Journal

    AJ · 25 publications · 2.8K citations

    22

    h-index

  5. Publications of the Astronomical Society of the Pacific

    PASP · 27 publications · 1.5K citations

    18

    h-index

1–5