C. S. Kochanek
- Astronomy and Astrophysics top 5%
- Instrumentation top 5%
- Nuclear and High Energy Physics
- Computational Mechanics
- Atomic and Molecular Physics, and Optics
- Co-authors
- J. R. WilsonR. L. BowersB. J. ShappeeT. W. S. HoloienJ. L. PrietoBuell T. JannuziTomoki MorokumaM. J. I. Brown
- Topics
- Gamma-ray bursts and supernovae (5 papers)Stellar, planetary, and galactic studies (3 papers)Astronomy and Astrophysical Research (2 papers)
- Journals
- The Astrophysical JournalMonthly Notices of the Royal Astronomical SocietyAstronomy and Astrophysics
- Partner nations
- United StatesChileAustralia
In The Last Decade
C. S. Kochanek
8 papers receiving 343 citations
Peers
Comparison fields: 5 of 33
- Astronomy and Astrophysics 310
- Instrumentation 129
- Nuclear and High Energy Physics 62
- Computational Mechanics 42
- Atomic and Molecular Physics, and Optics 31
Countries citing papers authored by C. S. Kochanek
This map shows the geographic impact of C. S. Kochanek's research. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by C. S. Kochanek with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites C. S. Kochanek more than expected).
Fields of papers citing papers by C. S. Kochanek
This network shows the impact of papers produced by C. S. Kochanek. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the papers produced by C. S. Kochanek. The network helps show where C. S. Kochanek may publish in the future.
Co-authorship network of co-authors of C. S. Kochanek
This figure shows the co-authorship network connecting the top 25 collaborators of C. S. Kochanek. A scholar is included among the top collaborators of C. S. Kochanek based on the total number of citations received by their joint publications. Widths of edges represent the number of papers authors have co-authored together. Node borders signify the number of papers an author published with C. S. Kochanek. C. S. Kochanek is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 39 | |
| 2 | 10 | |
| 3 | 19 | |
| 4 | 27 | |
| 5 | 88 | |
| 6 | Further Properties of the Candidate Progenitor of SN 2011dh in M51 | 1 |
| 7 | 118 | |
| 8 | 72 |
About C. S. Kochanek
C. S. Kochanek is a scholar working on Instrumentation, Astronomy and Astrophysics and Nuclear and High Energy Physics, having authored 8 papers that have together received 374 indexed citations. Recurring topics across this work include Gamma-ray bursts and supernovae (5 papers), Stellar, planetary, and galactic studies (3 papers) and Astronomy and Astrophysical Research (2 papers). The work is most often cited by research in Instrumentation (129 citations), Astronomy and Astrophysics (310 citations) and Nuclear and High Energy Physics (62 citations). C. S. Kochanek has collaborated with scholars based in United States, Chile and Australia. Frequent co-authors include J. R. Wilson, R. L. Bowers, B. J. Shappee, T. W. S. Holoien, J. L. Prieto, Buell T. Jannuzi, Tomoki Morokuma, M. J. I. Brown, Anthony H. Gonzalez and N. Cantale. Their work appears in journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Astronomy and Astrophysics.
Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive bibliographic database. While OpenAlex provides broad and valuable coverage of the global research landscape, it—like all bibliographic datasets—has inherent limitations. These include incomplete records, variations in author disambiguation, differences in journal indexing, and delays in data updates. As a result, some metrics and network relationships displayed in Rankless may not fully capture the entirety of a scholar's output or impact.