S. Dos Santos

5.8k total citations
12 papers, 241 citations indexed

About

S. Dos Santos is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Materials Chemistry. According to data from OpenAlex, S. Dos Santos has authored 12 papers receiving a total of 241 indexed citations (citations by other indexed papers that have themselves been cited), including 9 papers in Astronomy and Astrophysics, 6 papers in Nuclear and High Energy Physics and 2 papers in Materials Chemistry. Recurrent topics in S. Dos Santos's work include Galaxies: Formation, Evolution, Phenomena (9 papers), Astrophysical Phenomena and Observations (7 papers) and Astrophysics and Cosmic Phenomena (4 papers). S. Dos Santos is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (9 papers), Astrophysical Phenomena and Observations (7 papers) and Astrophysics and Cosmic Phenomena (4 papers). S. Dos Santos collaborates with scholars based in United Kingdom, France and Italy. S. Dos Santos's co-authors include Olivier Doré, R. F. Mushotzky, S. Molendi, I. Sakelliou, Kyoko Matsushita, G. C. Stewart, H. Böhringer, J. A. Kennea, M. Ehle and E. Belsole and has published in prestigious journals such as Monthly Notices of the Royal Astronomical Society, Astronomy and Astrophysics and Nuclear Instruments and Methods in Physics Research Section B Beam Interactions with Materials and Atoms.

In The Last Decade

S. Dos Santos

11 papers receiving 235 citations

Peers

S. Dos Santos
U. Morita Japan
Michael Garcia United States
Minsun Kim South Korea
R.B. Kidman United States
J. E. Carlstrom United States
J. W. Menzies South Africa
B. Sams Germany
U. Morita Japan
S. Dos Santos
Citations per year, relative to S. Dos Santos S. Dos Santos (= 1×) peers U. Morita

Countries citing papers authored by S. Dos Santos

Since Specialization
Citations

This map shows the geographic impact of S. Dos Santos'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 S. Dos Santos with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites S. Dos Santos more than expected).

Fields of papers citing papers by S. Dos Santos

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by S. Dos Santos. 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 S. Dos Santos. The network helps show where S. Dos Santos may publish in the future.

Co-authorship network of co-authors of S. Dos Santos

This figure shows the co-authorship network connecting the top 25 collaborators of S. Dos Santos. A scholar is included among the top collaborators of S. Dos Santos 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 S. Dos Santos. S. Dos Santos is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

12 of 12 papers shown
2.
Bertarelli, A., Federico Carra, F. Cerutti, et al.. (2013). Behaviour of advanced materials impacted by high energy particle beams. Journal of Physics Conference Series. 451. 12005–12005. 8 indexed citations
3.
Bertarelli, A., V. Boccone, Federico Carra, et al.. (2013). An experiment to test advanced materials impacted by intense proton pulses at CERN HiRadMat facility. Nuclear Instruments and Methods in Physics Research Section B Beam Interactions with Materials and Atoms. 308. 88–99. 23 indexed citations
4.
Willis, J. P., F. Pacaud, I. Valtchanov, et al.. (2005). The XMM Large-Scale Structure survey: an initial sample of galaxy groups and clusters to a redshift z < 0.6. Monthly Notices of the Royal Astronomical Society. 363(2). 675–691. 38 indexed citations
5.
Valtchanov, I., M. Pierre, J. P. Willis, et al.. (2004). The XMM-LSS survey. Astronomy and Astrophysics. 423(1). 75–85. 28 indexed citations
6.
Valtchanov, I., J. P. Willis, S. Dos Santos, et al.. (2003). The XMM-LSS Survey. First high redshift galaxy clusters: relaxed and collapsing systems. ArXiv.org. 1 indexed citations
7.
Santos, S. Dos & Olivier Doré. (2002). Competition between shocks and entropy floor: Unifying groupsand clusters of galaxies. Springer Link (Chiba Institute of Technology). 21 indexed citations
8.
Durret, F., E. Slezak, Richard Lieu, S. Dos Santos, & Massimiliano Bonamente. (2002). The extreme ultraviolet excess emission in five clusters of galaxiesrevisited. Astronomy and Astrophysics. 390(2). 397–406. 13 indexed citations
9.
Böhringer, H., E. Belsole, J. A. Kennea, et al.. (2001). XMM-Newton observations of M 87 and its X-ray halo. Springer Link (Chiba Institute of Technology). 101 indexed citations
10.
Nevalainen, J., D. Lumb, S. Dos Santos, et al.. (2001). Discovery of an absorbed cluster of galaxies (XMMU J183225.4-103645) close to the Galactic plane with XMM-Newton. Springer Link (Chiba Institute of Technology). 3 indexed citations
11.
Santos, S. Dos. (2001). The steady-state conduction-driven temperature profile in clusters of galaxies. Monthly Notices of the Royal Astronomical Society. 323(4). 930–938. 4 indexed citations
12.
Santos, S. Dos & G. A. Mamon. (1999). Clumpy diffuse X-ray emission from the spiral-rich compact galaxy group HCG 16. 352(1). 1–18. 1 indexed citations

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.

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