Point Spread Function Photometry

Point Spread Function Photometry is a photometric method that models the spatial distribution of stellar light as a mathematical point spread function to achieve precise flux measurements by fitting the expected instrumental response to observed point-source images in ultraviolet and stellar photometry.

84

Publications

11.8K

Citations

546

Authors

299

Institutions

Publications per year

2017–2026

26

Authors

546

  1. DM
    D. Minniti

    Pontificia Universidad Católica de Chile, Chile

    5 publications · 91 citations

    5

    h-index

  2. AE
    Andrew E. Dolphin

    RTX (United States), United States

    3 publications · 163 citations

    3

    h-index

  3. LC
    Leigh C. Smith

    University of Hertfordshire, United Kingdom

    3 publications · 61 citations

    3

    h-index

  4. DN
    D. Nardiello

    Osservatorio Astronomico di Padova, Italy

    3 publications · 196 citations

    3

    h-index

  5. LR
    L. R. Bedin

    Osservatorio Astronomico di Padova, Italy

    3 publications · 196 citations

    3

    h-index

1–5 of 546

Venues

  1. 15

    h-index

  2. The Astrophysical Journal

    ApJ · 14 publications · 902 citations

    13

    h-index

  3. The Astronomical Journal

    AJ · 11 publications · 552 citations

    11

    h-index

  4. Publications of the Astronomical Society of the Pacific

    PASP · 10 publications · 7.1K citations

    10

    h-index

  5. Astronomy and Astrophysics

    9 publications · 246 citations

    8

    h-index

1–5