Main Sequence Scatter

Main Sequence Scatter is a statistical metric in astrophysics that quantifies the dispersion in star formation rates among galaxies at a given stellar mass, serving as a probe of the intrinsic variability and evolutionary processes within the star-forming galaxy population.

20

Publications

2.5K

Citations

82

Authors

76

Institutions

Publications per year

2017–2026

11

Authors

82

  1. LM
    L. Morselli

    Osservatorio Astronomico di Padova, Italy

    1 publications · 122 citations

    1

    h-index

  2. JF
    Jonathan Florez

    The University of Texas at Austin, United States

    1 publications · 14 citations

    1

    h-index

  3. IW
    Isak Wold

    Goddard Space Flight Center, United States

    1 publications · 14 citations

    1

    h-index

  4. BK
    B. K. Gibson

    University of Lancashire, United Kingdom

    1 publications · 65 citations

    1

    h-index

  5. GR
    G. R. Meurer

    Johns Hopkins University, United States

    1 publications · 15 citations

    1

    h-index

1–5 of 82

Venues

  1. 7

    h-index

  2. The Astrophysical Journal

    ApJ · 3 publications · 151 citations

    3

    h-index

  3. 2

    h-index

  4. The Astronomical Journal

    AJ · 2 publications · 83 citations

    2

    h-index

  5. The Astrophysical Journal Supplement Series

    2 publications · 1.5K citations

    2

    h-index

1–5