Sky Background Estimation

Sky Background Estimation is a photometric measurement technique that determines the ambient flux contribution from the night sky in astronomical observations by isolating and quantifying non-source illumination within a defined observational field.

348

Publications

20.7K

Citations

2.1K

Authors

587

Institutions

Publications per year

2017–2026

90

Authors

2.1K

  1. RP
    Richard Perez

    University at Albany, State University of New York, United States

    6 publications · 1.1K citations

    6

    h-index

  2. MC
    M. C. B. Ashley

    UNSW Sydney, Australia

    5 publications · 250 citations

    5

    h-index

  3. JW
    J. W. V. Storey

    UNSW Sydney, Australia

    5 publications · 250 citations

    5

    h-index

  4. SC
    Samir Choudhuri

    Indian Institute of Technology Kharagpur, India

    4 publications · 162 citations

    4

    h-index

  5. JD
    Judd D. Bowman

    Arizona State University, United States

    4 publications · 254 citations

    4

    h-index

1–5 of 2.1K

Venues

  1. Monthly Notices of the Royal Astronomical Society

    56 publications · 4.1K citations

    32

    h-index

  2. The Astrophysical Journal

    ApJ · 45 publications · 2.7K citations

    27

    h-index

  3. Solar Energy

    18 publications · 1.7K citations

    16

    h-index

  4. Astronomy and Astrophysics

    16 publications · 970 citations

    15

    h-index

  5. The Astronomical Journal

    AJ · 16 publications · 1.3K citations

    14

    h-index

1–5