C. Sneden

895 total citations
8 papers, 610 citations indexed

About

C. Sneden is a scholar working on Astronomy and Astrophysics, Instrumentation and Mechanics of Materials. According to data from OpenAlex, C. Sneden has authored 8 papers receiving a total of 610 indexed citations (citations by other indexed papers that have themselves been cited), including 8 papers in Astronomy and Astrophysics, 3 papers in Instrumentation and 2 papers in Mechanics of Materials. Recurrent topics in C. Sneden's work include Stellar, planetary, and galactic studies (6 papers), Astrophysics and Star Formation Studies (4 papers) and Astronomy and Astrophysical Research (3 papers). C. Sneden is often cited by papers focused on Stellar, planetary, and galactic studies (6 papers), Astrophysics and Star Formation Studies (4 papers) and Astronomy and Astrophysical Research (3 papers). C. Sneden collaborates with scholars based in United States, Italy and Germany. C. Sneden's co-authors include J. E. Lawler, E. A. Den Hartog, M. E. Wickliffe, J. J. Cowan, Jennifer Sobeck, E. Carretta, V. D’Orazi, A. Bragaglia, S. Lucatello and R. Gratton and has published in prestigious journals such as The Astrophysical Journal, The Astrophysical Journal Supplement Series and Astronomy and Astrophysics.

In The Last Decade

C. Sneden

8 papers receiving 592 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. Sneden United States 8 569 225 108 43 28 8 610
Tomer Holczer Israel 10 410 0.7× 117 0.5× 45 0.4× 80 1.9× 24 0.9× 14 479
Y. Q. Chen China 13 713 1.3× 287 1.3× 81 0.8× 26 0.6× 12 0.4× 14 738
R. B. C. Henry United States 16 845 1.5× 227 1.0× 103 1.0× 25 0.6× 19 0.7× 31 876
R. Faraggiana Italy 13 888 1.6× 304 1.4× 60 0.6× 47 1.1× 56 2.0× 49 933
J. B. Holberg United States 17 898 1.6× 334 1.5× 42 0.4× 44 1.0× 48 1.7× 32 922
E. Tognelli Italy 15 691 1.2× 235 1.0× 132 1.2× 49 1.1× 12 0.4× 38 790
A. Magazzù Spain 17 721 1.3× 231 1.0× 41 0.4× 28 0.7× 27 1.0× 38 736
Guillermo Garcı́a-Segura Mexico 23 1.4k 2.4× 192 0.9× 183 1.7× 41 1.0× 30 1.1× 55 1.4k
A. W. A. Pauldrach Germany 15 1.2k 2.2× 385 1.7× 67 0.6× 35 0.8× 52 1.9× 61 1.2k
M. Bryce United Kingdom 16 812 1.4× 176 0.8× 55 0.5× 55 1.3× 28 1.0× 50 835

Countries citing papers authored by C. Sneden

Since Specialization
Citations

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

Fields of papers citing papers by C. Sneden

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of C. Sneden

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

All Works

8 of 8 papers shown
1.
Preston, George W., et al.. (2015). A DETAILED STUDY OF GIANTS AND HORIZONTAL BRANCH STARS IN M68: ATMOSPHERIC PARAMETERS AND CHEMICAL ABUNDANCES. The Astronomical Journal. 149(6). 204–204. 7 indexed citations
2.
Marino, A. F., A. P. Milone, C. Sneden, et al.. (2012). The double sub-giant branch of NGC 6656 (M 22): a chemical characterization. Astronomy and Astrophysics. 541. A15–A15. 54 indexed citations
3.
Bragaglia, A., R. Gratton, E. Carretta, et al.. (2012). Searching for multiple stellar populations in the massive, old open cluster Berkeley 39. Astronomy and Astrophysics. 548. A122–A122. 56 indexed citations
4.
Spite, M., B. Barbuy, F. Spite, et al.. (2012). First stars. Astronomy and Astrophysics. 550. A122–A122. 60 indexed citations
5.
Hartog, E. A. Den, J. E. Lawler, Jennifer Sobeck, C. Sneden, & J. J. Cowan. (2011). IMPROVED log( gf ) VALUES OF SELECTED LINES IN Mn I AND Mn II FOR ABUNDANCE DETERMINATIONS IN FGK DWARFS AND GIANTS. The Astrophysical Journal Supplement Series. 194(2). 35–35. 85 indexed citations
6.
Bragaglia, A., E. Carretta, R. Gratton, et al.. (2010). X-SHOOTER OBSERVATIONS OF MAIN-SEQUENCE STARS IN THE GLOBULAR CLUSTER NGC 2808: FIRST CHEMICAL TAGGING OF A He-NORMAL AND A He-RICH DWARF. The Astrophysical Journal Letters. 720(1). L41–L45. 50 indexed citations
7.
Lawler, J. E., M. E. Wickliffe, E. A. Den Hartog, & C. Sneden. (2001). Improved Laboratory Transition Parameters for Euiiand Application to the Solar Europium Elemental and Isotopic Composition. The Astrophysical Journal. 563(2). 1075–1088. 265 indexed citations
8.
Sneden, C., et al.. (1995). A survey of weak diffuse interstellar bands in selected ranges between 5600 and 7000 Å. Planetary and Space Science. 43(10-11). 1195–1203. 33 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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