Circumgalactic Absorption is an astrophysical phenomenon characterized by the preferential attenuation of electromagnetic radiation from background sources due to the presence of gaseous material in the circumgalactic medium surrounding a galaxy, distinguished from interstellar or intergalactic absorption by its spatial localization and kinematic association with galactic halos.
189
Publications
12.8K
Citations
407
Authors
245
Institutions
Publications per year
2017–2026
116
Publications
189
1–5 of 189
Authors
407
- JX
16
h-index
- JK
14
h-index
- GG
13
h-index
- HC
13
h-index
- BD
13
h-index
1–5 of 407
Institutions
245
University of California, Santa Cruz
Santa Cruz, United States
27 h-index
58 publications
5.3K citations
Space Telescope Science Institute
Baltimore, United States
25 h-index
67 publications
6.9K citations
Swinburne University of Technology
Melbourne, Australia
24 h-index
66 publications
3K citations
New Mexico State University
Las Cruces, United States
22 h-index
52 publications
2.7K citations
Leiden University
Leiden, The Netherlands
22 h-index
35 publications
2.8K citations
University of Chicago
Chicago, United States
21 h-index
38 publications
2.5K citations
University of Massachusetts Amherst
Amherst Center, United States
21 h-index
34 publications
3.4K citations
Carnegie Observatories
Pasadena, United States
18 h-index
28 publications
2.2K citations
1–8 of 245
Venues
- The Astrophysical Journal
ApJ · 79 publications · 6.6K citations
43
h-index
- Monthly Notices of the Royal Astronomical Society
64 publications · 3.3K citations
36
h-index
- The Astrophysical Journal Letters
8 publications · 696 citations
8
h-index
- The Astrophysical Journal Supplement Series
5 publications · 558 citations
5
h-index
- eScholarship (California Digital Library)
Repository · 5 publications · 197 citations
5
h-index
1–5