R. K. Sheth

2.4k total citations · 1 hit paper
9 papers, 1.6k citations indexed

About

R. K. Sheth is a scholar working on Astronomy and Astrophysics, Instrumentation and Statistical and Nonlinear Physics. According to data from OpenAlex, R. K. Sheth has authored 9 papers receiving a total of 1.6k indexed citations (citations by other indexed papers that have themselves been cited), including 8 papers in Astronomy and Astrophysics, 4 papers in Instrumentation and 2 papers in Statistical and Nonlinear Physics. Recurrent topics in R. K. Sheth's work include Galaxies: Formation, Evolution, Phenomena (8 papers), Astronomy and Astrophysical Research (4 papers) and Gamma-ray bursts and supernovae (2 papers). R. K. Sheth is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (8 papers), Astronomy and Astrophysical Research (4 papers) and Gamma-ray bursts and supernovae (2 papers). R. K. Sheth collaborates with scholars based in United States, Italy and Belgium. R. K. Sheth's co-authors include A. Cooray, Román Scoccimarro, G. Tormen, C. Giocoli, Jorge Moreno, Vincent Desjacques, Adi Nusser, Marcello Musso, V. Vikram and Claudia Maraston and has published in prestigious journals such as Physics Reports and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

R. K. Sheth

9 papers receiving 1.5k citations

Hit Papers

Halo models of large scale structure 2002 2026 2010 2018 2002 400 800 1.2k

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
R. K. Sheth United States 9 1.5k 518 480 168 146 9 1.6k
A. Cooray United States 11 1.7k 1.1× 510 1.0× 451 0.9× 145 0.9× 107 0.7× 12 1.8k
Cameron K. McBride United States 21 1.6k 1.0× 692 1.3× 304 0.6× 178 1.1× 129 0.9× 31 1.6k
F. Prada Spain 11 1.2k 0.8× 490 0.9× 330 0.7× 93 0.6× 90 0.6× 21 1.2k
Mark C. Neyrinck United States 23 1.5k 1.0× 473 0.9× 396 0.8× 107 0.6× 204 1.4× 55 1.6k
M. Plionis Greece 27 2.2k 1.4× 696 1.3× 790 1.6× 124 0.7× 230 1.6× 123 2.3k
L. Guzzo Italy 29 2.5k 1.6× 1.0k 2.0× 763 1.6× 144 0.9× 176 1.2× 79 2.6k
Ryan Scranton United States 21 1.5k 1.0× 554 1.1× 333 0.7× 220 1.3× 78 0.5× 26 1.5k
Donald P. Schneider United States 26 1.9k 1.3× 649 1.3× 368 0.8× 105 0.6× 70 0.5× 38 2.0k
P. Fosalba Spain 20 1.3k 0.9× 390 0.8× 375 0.8× 87 0.5× 100 0.7× 39 1.4k
S. D. M. White Germany 8 2.0k 1.3× 1.1k 2.0× 421 0.9× 166 1.0× 169 1.2× 9 2.0k

Countries citing papers authored by R. K. Sheth

Since Specialization
Citations

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

Fields of papers citing papers by R. K. Sheth

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of R. K. Sheth

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

All Works

9 of 9 papers shown
1.
Bernardi, Mariangela, A. Meert, R. K. Sheth, et al.. (2015). The massive end of the luminosity and stellar mass functions and clustering from CMASS to SDSS: evidence for and against passive evolution. Monthly Notices of the Royal Astronomical Society. 455(4). 4122–4135. 28 indexed citations
2.
Musso, Marcello & R. K. Sheth. (2014). The excursion set approach in non-Gaussian random fields. Monthly Notices of the Royal Astronomical Society. 439(3). 3051–3063. 12 indexed citations
3.
Giocoli, C., Jorge Moreno, R. K. Sheth, & G. Tormen. (2007). An improved model for the formation times of dark matter haloes. Monthly Notices of the Royal Astronomical Society. 376(3). 977–983. 57 indexed citations
4.
Desjacques, Vincent, Adi Nusser, & R. K. Sheth. (2006). The probability distribution function of the Lyman   transmitted flux from a sample of Sloan Digital Sky Survey quasars. Monthly Notices of the Royal Astronomical Society. 374(1). 206–219. 26 indexed citations
5.
Sheth, R. K.. (2005). The halo-model description of marked statistics. Monthly Notices of the Royal Astronomical Society. 364(3). 796–806. 36 indexed citations
6.
Sheth, R. K.. (2003). Substructure in dark matter haloes: towards a model of the abundance and spatial distribution of subclumps. Monthly Notices of the Royal Astronomical Society. 345(4). 1200–1204. 27 indexed citations
7.
Cooray, A. & R. K. Sheth. (2002). Halo models of large scale structure. Physics Reports. 372(1). 1–129. 1258 indexed citations breakdown →
8.
Scoccimarro, Román & R. K. Sheth. (2002). PTHALOS: a fast method for generating mock galaxy distributions. Monthly Notices of the Royal Astronomical Society. 329(3). 629–640. 114 indexed citations
9.
Sheth, R. K.. (1996). Galton-Watson branching processes and the growth of gravitational clustering. Monthly Notices of the Royal Astronomical Society. 281(4). 1277–1289. 16 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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