Background Spectrum Modeling is a theoretical and computational framework that characterizes the diffuse extragalactic infrared emission by decomposing it into its constituent astrophysical components and deriving their spectral energy distributions to enable accurate comparison with observational data.
306
Publications
20K
Citations
1.6K
Authors
511
Institutions
Publications per year
2017–2026
85
Parents
Publications
306
1–5 of 306
Authors
1.6K
- GD
6
h-index
- PDPasquale Dario Serpico
Laboratoire d'Annecy de Physique Théorique, France
6 publications · 242 citations
6
h-index
- MT
6
h-index
- FA
5
h-index
- FC
5
h-index
1–5 of 1.6K
Institutions
511
Centre National de la Recherche Scientifique
Paris, France
29 h-index
201 publications
22.4K citations
Goddard Space Flight Center
Greenbelt, United States
20 h-index
68 publications
10.4K citations
University of California, Berkeley
Berkeley, United States
18 h-index
52 publications
3.4K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
14 h-index
26 publications
2.1K citations
Max Planck Institute for Extraterrestrial Physics
Garching bei München, Germany
13 h-index
36 publications
2.1K citations
Université Paris Cité
Paris, France
13 h-index
56 publications
6.4K citations
California Institute of Technology
Pasadena, United States
13 h-index
35 publications
3.3K citations
Sorbonne Université
Paris, France
12 h-index
36 publications
2.6K citations
1–8 of 511
Venues
- The Astrophysical Journal
ApJ · 62 publications · 6.4K citations
42
h-index
- Monthly Notices of the Royal Astronomical Society
56 publications · 3.4K citations
28
h-index
- Astronomy and Astrophysics
26 publications · 1.9K citations
20
h-index
- Physical review. D/Physical review. D.
PRD · 11 publications · 440 citations
11
h-index
- Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D, Particles, fields, gravitation, and cosmology
9 publications · 667 citations
9
h-index
1–5