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
Parents
133
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
A global spectral study of black hole X-ray binaries
Robert Dunn, R. P. Fender, Elmar Körding et al. · Monthly Notices of the Royal Astronomical Society · 2010 · 303 citations · Full text
Natural Sciences, Astronomy, Physics +14
1–5 of 133
357
12
h-index
11
h-index
10
h-index
10
h-index
9
h-index
1–5 of 357
214

University of Amsterdam
Amsterdam, The Netherlands
23 h-index
70 publications
3.9K citations

Brera Astronomical Observatory
Milan, Italy
17 h-index
32 publications
2.3K citations
Massachusetts Institute of Technology
Cambridge, United States
17 h-index
30 publications
1.4K citations
Goddard Space Flight Center
Greenbelt, United States
16 h-index
21 publications
1.2K citations
University of Southampton
Southampton, United Kingdom
15 h-index
28 publications
2.7K citations
University of California, Berkeley
Berkeley, United States
11 h-index
11 publications
603 citations
Institute of High Energy Physics
Beijing, China
11 h-index
52 publications
1.2K citations
National Institute for Astrophysics
Rome, Italy
10 h-index
29 publications
1.2K citations
1–8 of 214
ApJ · 39 publications · 2.3K citations
27
h-index
37 publications · 1.9K citations
26
h-index
22 publications · 929 citations
20
h-index
7 publications · 308 citations
7
h-index
AJ · 3 publications · 124 citations
3
h-index
1–5