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.
Interstellar Ice: The Infrared Space Observatory Legacy
This map shows the geographic impact of E. L. Gibb'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. L. Gibb with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites E. L. Gibb more than expected).
This network shows the impact of papers produced by E. L. Gibb. 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. L. Gibb. The network helps show where E. L. Gibb may publish in the future.
Co-authorship network of co-authors of E. L. Gibb
This figure shows the co-authorship network connecting the top 25 collaborators of E. L. Gibb.
A scholar is included among the top collaborators of E. L. Gibb 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. L. Gibb. E. L. Gibb is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
DiSanti, M. A., Neil Dello Russo, B. P. Bonev, et al.. (2017). Compositional Study of Jupiter Family Comet 45P/Honda-Mrkos-Pajdusakova Near Perihelion Using iSHELL at the NASA-Infrared Telescope Facility. LPI. 2899.1 indexed citations
Bonev, B. P., E. L. Gibb, G. L. Villanueva, et al.. (2014). OH* prompt emission and near-infrared searches for HDO in the moderately bright comets C/2007 N3 Lulin and 103P/Hartley 2. 54.1 indexed citations
DiSanti, M. A., B. P. Bonev, E. L. Gibb, et al.. (2014). The chemical composition of comet C/2012 S1 (ISON) between 1.2 au and 0.35 au from the Sun. 136.2 indexed citations
14.
Bonev, B. P., E. L. Gibb, G. L. Villanueva, et al.. (2009). Spin And Rotational Temperatures Of Water And Methane: Comets C/2007 N3 (Lulin) And C/2007 W1 (Boattini). 41.1 indexed citations
15.
Salyk, Colette, Geoffrey A. Blake, M. J. Mumma, et al.. (2007). Comet 17P/Holmes. International Astronomical Union Circular. 8890. 1.2 indexed citations
16.
Mumma, M. J., M. A. DiSanti, Neil Dello Russo, et al.. (2002). The organic volatile composition of Oort cloud comets: evidence for chemical diversity in the giant-planets' nebular region. ESASP. 500. 753–762.8 indexed citations
17.
DiSanti, M. A., et al.. (2002). A Comparison of the Volatile Carbon-Oxygen Chemistry in Several Oort Cloud Comets. 34.1 indexed citations
18.
Russo, Neil Dello, M. A. DiSanti, K. Magee‐Sauer, E. L. Gibb, & M. J. Mumma. (2002). Production of C 2 H 6 and H 2 O in comet 2002 C1 Ikeya-Zhang on UT 2002 April 13.7 - 13.9. ESASP. 500. 689–692.1 indexed citations
19.
Magee‐Sauer, K., Neil Dello Russo, M. A. DiSanti, E. L. Gibb, & M. J. Mumma. (2002). CSHELL Observations of Comet C/2002 C1 (Ikeya-Zhang) in the 3.0-Micron Region. 34.1 indexed citations
20.
Gibb, E. L., M. J. Mumma, M. A. DiSanti, Neil Dello Russo, & K. Magee‐Sauer. (2002). An infrared search for HDO in comets. 500(500). 705–708.3 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.