K. Farouqi

1.4k total citations
32 papers, 837 citations indexed

About

K. Farouqi is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Instrumentation. According to data from OpenAlex, K. Farouqi has authored 32 papers receiving a total of 837 indexed citations (citations by other indexed papers that have themselves been cited), including 26 papers in Astronomy and Astrophysics, 20 papers in Nuclear and High Energy Physics and 3 papers in Instrumentation. Recurrent topics in K. Farouqi's work include Gamma-ray bursts and supernovae (21 papers), Astronomical and nuclear sciences (17 papers) and Nuclear physics research studies (17 papers). K. Farouqi is often cited by papers focused on Gamma-ray bursts and supernovae (21 papers), Astronomical and nuclear sciences (17 papers) and Nuclear physics research studies (17 papers). K. Farouqi collaborates with scholars based in Germany, United States and Switzerland. K. Farouqi's co-authors include Karl Kratz, B. Pfeiffer, F.‐K. Thielemann, T. Rauscher, J. W. Truran, J. J. Cowan, N. Christlieb, James W. Truran, C. Sneden and I. Dillmann and has published in prestigious journals such as SHILAP Revista de lepidopterología, The Astrophysical Journal and Astronomy and Astrophysics.

In The Last Decade

K. Farouqi

30 papers receiving 797 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
K. Farouqi Germany 14 677 481 126 77 47 32 837
Y.‐Z. Qian United States 18 1.2k 1.7× 1.0k 2.1× 153 1.2× 55 0.7× 35 0.7× 29 1.6k
Lih‐Sin The United States 18 798 1.2× 481 1.0× 99 0.8× 99 1.3× 46 1.0× 45 934
M. F. El Eid Lebanon 12 454 0.7× 272 0.6× 60 0.5× 39 0.5× 36 0.8× 38 542
Pavel A. Denissenkov Canada 22 1.4k 2.0× 313 0.7× 448 3.6× 43 0.6× 47 1.0× 57 1.5k
J. W. Truran United States 17 935 1.4× 340 0.7× 160 1.3× 43 0.6× 66 1.4× 57 1.1k
Eduardo Bravo Spain 19 1.4k 2.0× 982 2.0× 55 0.4× 105 1.4× 42 0.9× 75 1.7k
M. Hashimoto Japan 12 470 0.7× 325 0.7× 38 0.3× 53 0.7× 39 0.8× 30 585
Debra L. Burris United States 6 858 1.3× 350 0.7× 212 1.7× 28 0.4× 31 0.7× 7 938
N. P. M. Kuin United Kingdom 18 1.1k 1.6× 337 0.7× 73 0.6× 21 0.3× 44 0.9× 110 1.1k
L. Piersanti Italy 15 959 1.4× 285 0.6× 208 1.7× 29 0.4× 65 1.4× 41 1.0k

Countries citing papers authored by K. Farouqi

Since Specialization
Citations

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

Fields of papers citing papers by K. Farouqi

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of K. Farouqi

This figure shows the co-authorship network connecting the top 25 collaborators of K. Farouqi. A scholar is included among the top collaborators of K. Farouqi 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 K. Farouqi. K. Farouqi 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.
Farouqi, K., Anna Frebel, & F.‐K. Thielemann. (2025). Deciphering the origins of the elements through galactic archeology. The European Physical Journal A. 61(9).
2.
Farouqi, K., F.‐K. Thielemann, Stephan Rosswog, & K.L. Kratz. (2022). Correlations ofr-process elements in very metal-poor stars as clues to their nucleosynthesis sites. Astronomy and Astrophysics. 663. A70–A70. 21 indexed citations
3.
Thielemann, F.‐K., K. Farouqi, Stephan Rosswog, & Karl Kratz. (2022). r-Process Contributions to Low-Metallicity Stars. SHILAP Revista de lepidopterología. 260. 9002–9002. 3 indexed citations
4.
Akram, Waheed, et al.. (2020). Nucleosynthesis of light trans-Fe isotopes in ccSNe: Implications from presolar SiC-X grains. SHILAP Revista de lepidopterología. 227. 1009–1009. 2 indexed citations
5.
Kratz, Karl, K. Farouqi, & B. Pfeiffer. (2017). Nuclear-data input to the classical r-process: The case of β-decay properties. AIP conference proceedings. 1852. 30001–30001. 1 indexed citations
6.
Hill, V., N. Christlieb, Timothy C. Beers, et al.. (2017). The Hamburg/ESO R-process Enhanced Star survey (HERES). Astronomy and Astrophysics. 607. A91–A91. 34 indexed citations
7.
Farouqi, K., et al.. (2013). Origin of Anomalous Zr, Mo and Ru Abundances in SiC X-Grains: Indications of a Primary Charged-Particle Process. M&PSA. 76. 5082. 2 indexed citations
8.
Ott, U., Astrid Besmehn, K. Farouqi, et al.. (2012). New Attempts to Understand Nanodiamond Stardust. Publications of the Astronomical Society of Australia. 29(2). 90–97. 3 indexed citations
9.
Hansen, C. J., F. Primas, H. Hartman, et al.. (2012). Silver and palladium help unveil the nature of a second r-process. Springer Link (Chiba Institute of Technology). 57 indexed citations
10.
Arndt, O., Karl Kratz, W. B. Walters, et al.. (2011). Decay of ther-process nuclides137,138,139Sb, and theA=130solarr-process abundance peak. Physical Review C. 84(6). 12 indexed citations
11.
Thielemann, F.‐K., Almudena Arcones, Roger Käppeli, et al.. (2011). What are the astrophysical sites for the r-process and the production of heavy elements?. Progress in Particle and Nuclear Physics. 66(2). 346–353. 182 indexed citations
12.
13.
Farouqi, K., Karl Kratz, B. Pfeiffer, et al.. (2010). CHARGED-PARTICLE AND NEUTRON-CAPTURE PROCESSES IN THE HIGH-ENTROPY WIND OF CORE-COLLAPSE SUPERNOVAE. The Astrophysical Journal. 712(2). 1359–1377. 122 indexed citations
14.
Hayek, Wolfgang, N. Christlieb, Kimmo Eriksson, et al.. (2009). The Hamburg/ESO R-process enhanced star survey (HERES). Astronomy and Astrophysics. 504(2). 511–524. 56 indexed citations
15.
Farouqi, K., Karl Kratz, L. Mashonkina, et al.. (2009). NUCLEOSYNTHESIS MODES IN THE HIGH-ENTROPY WIND OF TYPE II SUPERNOVAE: COMPARISON OF CALCULATIONS WITH HALO-STAR OBSERVATIONS. The Astrophysical Journal. 694(1). L49–L53. 55 indexed citations
16.
Farouqi, K., Karl Kratz, J. J. Cowan, et al.. (2008). Nucleosynthesis Modes in the High‐Entropy‐Wind Scenario of Type II Supernovae. AIP conference proceedings. 309–314. 7 indexed citations
17.
Farouqi, K., Karl Kratz, L. Mashonkina, et al.. (2008). News from r-Process Nucleosynthesis: Consequences from the ESS to Early Stars. AIP conference proceedings. 1001. 245–253. 6 indexed citations
18.
Kratz, Karl, K. Farouqi, L. Mashonkina, et al.. (2008). The Astrophysical r-Process 50 Years after B[sup 2]FH. AIP conference proceedings. 972. 298–308. 2 indexed citations
19.
Kratz, Karl, K. Farouqi, B. Pfeiffer, et al.. (2007). Explorations of ther‐Processes: Comparisons between Calculations and Observations of Low‐Metallicity Stars. The Astrophysical Journal. 662(1). 39–52. 105 indexed citations
20.
Thielemann, F.‐K., I. V. Panov, E. Kolbe, et al.. (2007). THE R-PROCESS: SUPERNOVAE AND OTHER SOURCES OF THE HEAVIEST ELEMENTS. International Journal of Modern Physics E. 16(4). 1149–1163. 3 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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