Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies
if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the
same subfield and year (this is the minimum needed to enter the top 1%, not the average
within it), or reaches the top citation threshold in at least one of its specific research
topics.
AGN Dusty Tori. II. Observational Implications of Clumpiness
2008459 citationsMaia Nenkova, Robert Nikutta et al.The Astrophysical Journalprofile →
AGN Dusty Tori. I. Handling of Clumpy Media
2008366 citationsMaia Nenkova, Željko Ivezić et al.The Astrophysical Journalprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
hero ref
This map shows the geographic impact of Moshe Elitzur'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 Moshe Elitzur with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Moshe Elitzur more than expected).
This network shows the impact of papers produced by Moshe Elitzur. 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 Moshe Elitzur. The network helps show where Moshe Elitzur may publish in the future.
Co-authorship network of co-authors of Moshe Elitzur
This figure shows the co-authorship network connecting the top 25 collaborators of Moshe Elitzur.
A scholar is included among the top collaborators of Moshe Elitzur 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 Moshe Elitzur. Moshe Elitzur is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Pogrebenko, S. V., Leonid Gurvits, Moshe Elitzur, et al.. (2009). Water masers in the Saturnian system. Astronomy and Astrophysics. 494(2). L1–L4.5 indexed citations
7.
Elitzur, Moshe. (2008). Disk-outflow connection and the molecular dusty torus. Memorie della Societa Astronomica Italiana. 79. 1124.1 indexed citations
8.
Elitzur, Moshe. (2007). The AGN Obscuring Torus. 40095.1 indexed citations
9.
Hao, Lei, D. W. Weedman, H. W. W. Spoon, et al.. (2007). The Distribution of Silicate Strength of AGNs and ULIRGs. ASPC. 373. 574.1 indexed citations
10.
Justtanont, K., P. Bergman, Bengt Larsson, et al.. (2005). W Hya through the eye of Odin. Astronomy and Astrophysics. 439(2). 627–633.26 indexed citations
11.
Vinković, Dejan, Željko Ivezić, & Moshe Elitzur. (2002). LELUYA -- the First Exact General 2D Radiative Transfer Solver. AAS. 200.
12.
Nenkova, Maia, Moshe Elitzur, & Željko Ivezić. (2001). Modeling AGN Dust Distributions with the Continuum Radiative Transfer Code DUSTY. ASPC. 247. 383.
13.
Ivezić, Željko, Maia Nenkova, & Moshe Elitzur. (1999). DUSTY: Radiation transport in a dusty environment. ascl.5 indexed citations
14.
Ivezić, Željko & Moshe Elitzur. (1996). Starspots on CG Cygni during 1994 and 1995.. Bulletin of the American Astronomical Society. 188(2). 943.
15.
Ivezić, Željko & Moshe Elitzur. (1994). Infrared Emission and Dynamics of Outflows in Late-Type Stars. CERN Bulletin. 64. 711.1 indexed citations
Elitzur, Moshe & Benjamin F Cooke. (1984). Water Masers in Late-Type Stars. Bulletin of the American Astronomical Society. 16. 941.2 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.