Hardness Ratio Analysis

Hardness Ratio Analysis is a spectral analysis technique in X-ray astronomy that quantifies the relative flux of high-energy to low-energy X-ray photons to infer the spectral hardness of an astrophysical source without requiring full spectral modeling.

220

Publications

10.2K

Citations

804

Authors

337

Institutions

Publications per year

2017–2026

53

Authors

804

  1. AC
    Alok C. Gupta

    Aryabhatta Research Institute of Observational Sciences, India

    5 publications · 108 citations

    6

    h-index

  2. CV
    C. Vignali

    University of Bologna, Italy

    6 publications · 452 citations

    6

    h-index

  3. IM
    I. M. McHardy

    University of Southampton, United Kingdom

    6 publications · 235 citations

    6

    h-index

  4. FF
    F. Fiore

    Astronomical Observatory of Rome, Italy

    5 publications · 433 citations

    5

    h-index

  5. PT
    P. T. O’Brien

    University of Leicester, United Kingdom

    4 publications · 588 citations

    5

    h-index

1–5 of 804

Venues

  1. The Astrophysical Journal

    ApJ · 70 publications · 4.4K citations

    34

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    36 publications · 1.5K citations

    24

    h-index

  3. Astronomy and Astrophysics

    25 publications · 1.2K citations

    19

    h-index

  4. The Astrophysical Journal Letters

    7 publications · 311 citations

    8

    h-index

  5. 7

    h-index

1–5