Reference Star Selection

Reference Star Selection is the systematic process of identifying and choosing stable, well-characterized stars within a field of view to serve as positional fiducials in differential astrometry, distinguished by their photometric stability, astrometric precision, and spatial distribution relative to the target object.

46

Publications

2.4K

Citations

247

Authors

157

Institutions

Publications per year

2017–2026

14

Authors

247

  1. ES
    Eugene Serabyn

    Jet Propulsion Laboratory, United States

    3 publications · 125 citations

    3

    h-index

  2. AM
    A. Mérand

    Centre National de la Recherche Scientifique, France

    2 publications · 122 citations

    2

    h-index

  3. OA
    Olivier Absil

    University of Liège, Belgium

    2 publications · 105 citations

    2

    h-index

  4. NN
    N. Nardetto

    Centre National de la Recherche Scientifique, France

    2 publications · 122 citations

    2

    h-index

  5. LS
    L. Szabados

    Konkoly Observatory, Hungary

    2 publications · 122 citations

    2

    h-index

1–5 of 247

Venues

  1. The Astronomical Journal

    AJ · 8 publications · 297 citations

    8

    h-index

  2. Astronomy and Astrophysics

    8 publications · 572 citations

    8

    h-index

  3. The Astrophysical Journal Supplement Series

    5 publications · 200 citations

    5

    h-index

  4. 4

    h-index

  5. Space Science Reviews

    1 publications · 24 citations

    1

    h-index

1–5