Hardness-intensity Relations

Hardness-Intensity Relations is a diagnostic plot or graphical representation in X-ray astronomy that characterizes the spectral evolution of X-ray sources by correlating their hardness ratio, which reflects the relative flux in different energy bands, with their total X-ray intensity, thereby revealing physical changes in emission mechanisms or absorptions over time.

133

Publications

6.3K

Citations

357

Authors

214

Institutions

Publications per year

2017–2026

31

Variants

Hardness-intensity DiagramHid

Authors

357

  1. MV
    M. van der Klis

    University of Amsterdam, Netherlands

    12 publications · 762 citations

    12

    h-index

  2. TB
    T. Belloni

    Brera Astronomical Observatory, Italy

    11 publications · 854 citations

    11

    h-index

  3. EK
    E. Kuulkers

    European Space Astronomy Centre, Spain

    11 publications · 449 citations

    10

    h-index

  4. JH
    J. Homan

    University of Amsterdam, Netherlands

    10 publications · 668 citations

    10

    h-index

  5. MM
    Mariano Méndez

    University of Groningen, Netherlands

    9 publications · 465 citations

    9

    h-index

1–5 of 357

Venues

  1. The Astrophysical Journal

    ApJ · 39 publications · 2.3K citations

    27

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    37 publications · 1.9K citations

    26

    h-index

  3. Astronomy and Astrophysics

    22 publications · 929 citations

    20

    h-index

  4. The Astrophysical Journal Letters

    7 publications · 308 citations

    7

    h-index

  5. The Astronomical Journal

    AJ · 3 publications · 124 citations

    3

    h-index

1–5