Main Sequence Scatter
Main Sequence Scatter is a statistical metric in astrophysics that quantifies the dispersion in star formation rates among galaxies at a given stellar mass, serving as a probe of the intrinsic variability and evolutionary processes within the star-forming galaxy population.
20
Publications
2.5K
Citations
82
Authors
76
Institutions
Publications per year
2017–2026
11
20
Starbursts in and out of the star-formation main sequence
Astronomy and Astrophysics · 2018 · 165 citations · Full text
Natural Sciences, Astronomy, Physics +14
1–5 of 20
82
1
h-index
1
h-index
1
h-index
1
h-index
1
h-index
1–5 of 82
76

Centre National de la Recherche Scientifique
Paris, France
4 h-index
21 publications
2.1K citations
Swinburne University of Technology
Melbourne, Australia
3 h-index
3 publications
108 citations

University of the Western Cape
Cape Town, South Africa
3 h-index
5 publications
169 citations
Leiden University
Leiden, The Netherlands
2 h-index
3 publications
409 citations
Queen's University
Kingston, Canada
2 h-index
4 publications
86 citations

The University of Western Australia
Perth, Australia
2 h-index
4 publications
86 citations
International Centre for Radio Astronomy Research
Crawley, Australia
2 h-index
4 publications
86 citations
Ludwig-Maximilians-Universität München
Munich, Germany
2 h-index
2 publications
287 citations
1–8 of 76
7 publications · 418 citations
7
h-index
ApJ · 3 publications · 151 citations
3
h-index
2 publications · 97 citations
2
h-index
AJ · 2 publications · 83 citations
2
h-index
2 publications · 1.5K citations
2
h-index
1–5