Progenitor Radius Estimates

Progenitor Radius Estimates is a scientific metric that quantifies the physical size of a star immediately prior to its collapse or explosion as a supernova, distinguishing it from other progenitor properties by specifically characterizing the stellar radius at the pre-supernova stage.

36

Publications

2.3K

Citations

254

Authors

146

Institutions

Publications per year

2017–2026

14

Authors

254

  1. SV
    S. Valenti

    Las Cumbres Observatory Global Telescope Network, United States

    8 publications · 554 citations

    8

    h-index

  2. AG
    A. Gal‐Yam

    Weizmann Institute of Science, Israel

    7 publications · 629 citations

    7

    h-index

  3. DA
    D. A. Howell

    Las Cumbres Observatory Global Telescope Network, United States

    5 publications · 545 citations

    5

    h-index

  4. SB
    S. Benetti

    Osservatorio Astronomico di Padova, Italy

    5 publications · 328 citations

    5

    h-index

  5. PO
    P. Ochner

    Osservatorio Astronomico di Padova, Italy

    4 publications · 292 citations

    4

    h-index

1–5 of 254

Venues

  1. The Astrophysical Journal

    ApJ · 13 publications · 911 citations

    13

    h-index

  2. The Astrophysical Journal Letters

    9 publications · 823 citations

    9

    h-index

  3. 7

    h-index

  4. Springer Link (Chiba Institute of Technology)

    Repository · 2 publications · 53 citations

    2

    h-index

  5. The Astronomical Journal

    AJ · 1 publications · 100 citations

    1

    h-index

1–5