C. De Santis

6.4k total citations
30 papers, 803 citations indexed

About

C. De Santis is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics. According to data from OpenAlex, C. De Santis has authored 30 papers receiving a total of 803 indexed citations (citations by other indexed papers that have themselves been cited), including 18 papers in Astronomy and Astrophysics, 7 papers in Instrumentation and 6 papers in Nuclear and High Energy Physics. Recurrent topics in C. De Santis's work include Galaxies: Formation, Evolution, Phenomena (9 papers), Astronomy and Astrophysical Research (7 papers) and Earthquake Detection and Analysis (5 papers). C. De Santis is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (9 papers), Astronomy and Astrophysical Research (7 papers) and Earthquake Detection and Analysis (5 papers). C. De Santis collaborates with scholars based in Italy, Germany and United States. C. De Santis's co-authors include A. Grazian, A. Fontana, E. Giallongo, S. Gallozzi, S. Salimbeni, E. Vanzella, S. Cristiani, M. Nonino, L. Pentericci and N. Menci and has published in prestigious journals such as SHILAP Revista de lepidopterología, IEEE Transactions on Electron Devices and Astronomy and Astrophysics.

In The Last Decade

C. De Santis

27 papers receiving 788 citations

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name h Career Trend Papers Cites
C. De Santis Italy 14 736 460 98 43 41 30 803
A. Calamida Italy 16 591 0.8× 313 0.7× 30 0.3× 11 0.3× 16 0.4× 59 652
S. N. Tandon India 14 496 0.7× 161 0.3× 160 1.6× 18 0.4× 17 0.4× 54 604
Håkon Dahle Norway 19 937 1.3× 385 0.8× 141 1.4× 5 0.1× 19 0.5× 45 959
Lia F. Sartori Switzerland 12 583 0.8× 152 0.3× 158 1.6× 7 0.2× 5 0.1× 27 672
S. Béland United States 10 462 0.6× 166 0.4× 34 0.3× 9 0.2× 20 0.5× 43 534
Daisuke Yonetoku Japan 15 574 0.8× 52 0.1× 192 2.0× 9 0.2× 45 1.1× 67 631
G. J. Fishman United States 10 1.4k 2.0× 87 0.2× 566 5.8× 35 0.8× 13 0.3× 40 1.5k
S. T. Holland United States 25 1.6k 2.2× 237 0.5× 409 4.2× 5 0.1× 19 0.5× 126 1.6k
Rachel A. Osten United States 25 1.5k 2.0× 162 0.4× 79 0.8× 5 0.1× 13 0.3× 76 1.5k
Derek L. Buzasi United States 18 693 0.9× 264 0.6× 22 0.2× 7 0.2× 16 0.4× 61 736

Countries citing papers authored by C. De Santis

Since Specialization
Citations

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

Fields of papers citing papers by C. De Santis

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by C. De Santis. 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. De Santis. The network helps show where C. De Santis may publish in the future.

Co-authorship network of co-authors of C. De Santis

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

All Works

20 of 20 papers shown
1.
Scotti, V., Antonio Anastasio, A. Boiano, et al.. (2025). The Cherenkov Camera for the PBR mission. ArXiv.org. 391–391.
2.
Nozzoli, F., et al.. (2023). Search for electron capture in Lu176 with a lutetium yttrium oxyorthosilicate scintillator. Physical review. C. 107(4). 2 indexed citations
3.
Santis, C. De & S. Ricciarini. (2021). The High Energy Particle Detector (HEPD-02) for the second China Seismo-Electromagnetic Satellite (CSES-02). Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021). 58–58. 6 indexed citations
4.
Diego, Piero, Jianping Huang, Mirko Piersanti, et al.. (2020). The Electric Field Detector on Board the China Seismo Electromagnetic Satellite—In-Orbit Results and Validation. SHILAP Revista de lepidopterología. 5(1). 1–1. 24 indexed citations
5.
Conti, L., G. Ambrosi, R. Battiston, et al.. (2018). Study of the correlations between precipitating Van-Allen particles and seismic events: the methodology and the HEPD particle detector of CSES satellite.. EGU General Assembly Conference Abstracts. 17098.
6.
Omizzolo, A., G. Fasano, D. Paya, et al.. (2013). U-band photometry of 17 WINGS clusters. Astronomy and Astrophysics. 561. A111–A111. 14 indexed citations
7.
Fino, Luca Di, M. Casolino, C. De Santis, et al.. (2011). Heavy-Ion Anisotropy Measured by ALTEA in the International Space Station. Radiation Research. 176(3). 397–406. 23 indexed citations
8.
Casolino, M., C. De Santis, N. De Simone, et al.. (2011). Measurements of He isotopic ratio in cosmic rays in the 100 MeV – 1 GeV range with the PAMELA experiment. Florence Research (University of Florence). 7(4). 465–469. 5 indexed citations
9.
Zaconte, V., M. Casolino, C. De Santis, et al.. (2010). The radiation environment in the ISS-USLab measured by ALTEA: Spectra and relative nuclear abundances in the polar, equatorial and SAA regions. Advances in Space Research. 46(6). 797–799. 13 indexed citations
10.
Santini, P., A. Fontana, A. Grazian, et al.. (2009). Star formation and mass assembly in high redshift galaxies. Springer Link (Chiba Institute of Technology). 149 indexed citations
11.
Salimbeni, S., M. Castellano, L. Pentericci, et al.. (2009). A comprehensive study of large-scale structures in the GOODS-SOUTH field up to ${\mathsf z} \sim $ 2.5. Astronomy and Astrophysics. 501(3). 865–877. 24 indexed citations
12.
Schwope, A., T. Erben, J. Kohnert, et al.. (2009). The isolated neutron star RBS1774 revisited. Astronomy and Astrophysics. 499(1). 267–272. 14 indexed citations
13.
Grazian, A., S. Salimbeni, L. Pentericci, et al.. (2007). A comparison of LBGs, DRGs, and BzK galaxies: their contribution tothe stellar mass density in the GOODS-MUSIC sample. Astronomy and Astrophysics. 465(2). 393–404. 57 indexed citations
14.
Pentericci, L., A. Grazian, A. Fontana, et al.. (2007). Physical properties of z ~ 4 LBGs: differences between galaxies with and without Lyα emission. Astronomy and Astrophysics. 471(2). 433–438. 42 indexed citations
15.
Grazian, A., A. Fontana, L. Moscardini, et al.. (2006). The clustering evolution of distant red galaxies in the GOODS-MUSIC sample. Springer Link (Chiba Institute of Technology). 26 indexed citations
16.
Grazian, A., A. Fontana, C. De Santis, et al.. (2006). The GOODS-MUSIC sample: a multicolour catalog of near-IR selectedgalaxies in the GOODS-South field. Springer Link (Chiba Institute of Technology). 132 indexed citations
17.
Fontana, A., S. Salimbeni, A. Grazian, et al.. (2006). The Galaxy mass function up toz$\mathsf{=4}$ in the GOODS-MUSIC sample: into the epoch of formation of massive galaxies. Astronomy and Astrophysics. 459(3). 745–757. 212 indexed citations
18.
Grazian, A., et al.. (2004). The Large Binocular Camera Image Simulator. Publications of the Astronomical Society of the Pacific. 116(822). 750–761. 6 indexed citations
19.
Santis, C. De, et al.. (1980). Circuitless electron beam amplifier (CEBA). 318–320. 1 indexed citations
20.
Santis, C. De, et al.. (1973). An array technique for reducing ground losses in the HF range. IRE Transactions on Antennas and Propagation. 21(6). 769–773. 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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