This map shows the geographic impact of E. S. Howell'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 E. S. Howell with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites E. S. Howell more than expected).
This network shows the impact of papers produced by E. S. Howell. 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 E. S. Howell. The network helps show where E. S. Howell may publish in the future.
Co-authorship network of co-authors of E. S. Howell
This figure shows the co-authorship network connecting the top 25 collaborators of E. S. Howell.
A scholar is included among the top collaborators of E. S. Howell 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 E. S. Howell. E. S. Howell is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Hamilton, V. E., Amy Simon, H. H. Kaplan, et al.. (2019). The Global Mineralogy of (101955) Bennu from VNIR and TIR Observations During the Detailed Survey Phase of the OSIRIS-REx Mission. 2189. 2044.
8.
Moskovitz, Nicholas, David Polishook, F. E. DeMeo, et al.. (2014). Detection of aspect-dependent thermal emission as a signature of near-Earth asteroid pole orientation. 367.1 indexed citations
9.
Chesley, Steven R., M. C. Nolan, Davide Farnocchia, et al.. (2012). The Trajectory Dynamics of Near-Earth Asteroid 101955 (1999 RQ36). 1667. 6470.4 indexed citations
10.
Benner, L. A. M., M. Brozović, J. D. Giorgini, et al.. (2009). Arecibo and Goldstone Radar Images of Near-Earth Asteroid (136849) 1998 CS1. DPS.1 indexed citations
11.
Nolan, M. C., et al.. (2008). Physical Modeling of Triple Near-Earth Asteroid 153591 (2001 SN263). DPS. 213.2 indexed citations
12.
Margot, Jean‐Luc, Patrick Taylor, M. C. Nolan, et al.. (2008). Detailed Characterization Of Asteroid (35107) 1991 VH. 40.1 indexed citations
13.
Nolan, M. C., E. S. Howell, L. A. M. Benner, et al.. (2008). Arecibo Radar Imaging of 2001 SN263: A Near-Earth Triple Asteroid System. LPICo. 1405. 8258.7 indexed citations
14.
Harmon, J. K., M. C. Nolan, E. S. Howell, & J. D. Giorgini. (2008). Comet 8P/Tuttle. International Astronomical Union Circular. 8909. 1.2 indexed citations
15.
Howell, E. S., et al.. (2006). Correlating IRTF Spectra and Arecibo Radar Observations of Low-Albedo Main-Belt Asteroids. 38.1 indexed citations
16.
Howell, E. S., A. J. Lovell, Bryan Butler, & F. P. Schloerb. (2005). Radio OH Observations of Comet 9P/Tempel 1 before and after Deep Impact. DPS. 207.2 indexed citations
17.
Nolan, M. C., A. A. Hine, E. S. Howell, et al.. (2005). Extreme Diversity of Near-Earth Asteroid Physical Properties from Arecibo Radar Imaging. AAS. 207.1 indexed citations
18.
Grauer, A. D., E. Christensen, Petr Pravec, et al.. (2004). Physical Characteristics of the Binary PHA 2003 YT1. DPS.2 indexed citations
19.
Howell, E. S., A. S. Rivkin, Richard P. Binzel, & S. J. Bus. (1995). Spectral Observations of the Mars Trojan 5261 Eureka. LPI. 26. 633.1 indexed citations
20.
Howell, E. S., Erzsébet Merényi, & L. A. Lebofsky. (1991). Using Neural Networks to Classify Asteroid Spectra. Meteoritics and Planetary Science. 23. 1140.4 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.