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
Parents
220
MACS: A Quest for the Most Massive Galaxy Clusters in the Universe
H. Ebeling, A. C. Edge, J. P. Henry · The Astrophysical Journal · 2001 · 486 citations · Full text
Natural Sciences, Astronomy, Physics +15
X-ray variability of GX 339 - 4 in its very high state
Sigenori Miyamoto, Kazuhiro Kimura, Shunji Kitamoto et al. · The Astrophysical Journal · 1991 · 415 citations
1–5 of 220
804
Aryabhatta Research Institute of Observational Sciences, India
5 publications · 108 citations
6
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6
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6
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5
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5
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1–5 of 804
337
Max Planck Institute for Extraterrestrial Physics
Garching bei München, Germany
21 h-index
45 publications
3.4K citations

Centre National de la Recherche Scientifique
Paris, France
17 h-index
30 publications
1.8K citations
Goddard Space Flight Center
Greenbelt, United States
16 h-index
30 publications
4K citations
National Institute for Astrophysics
Rome, Italy
14 h-index
22 publications
1.6K citations

Brera Astronomical Observatory
Milan, Italy
14 h-index
21 publications
1.5K citations
University of Southampton
Southampton, United Kingdom
13 h-index
28 publications
1.1K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
12 h-index
29 publications
1.9K citations
National Astronomical Observatories
Beijing, China
11 h-index
19 publications
803 citations
1–8 of 337
ApJ · 70 publications · 4.4K citations
34
h-index
36 publications · 1.5K citations
24
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25 publications · 1.2K citations
19
h-index
7 publications · 311 citations
8
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6 publications · 196 citations
7
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1–5