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.
Observations of the Icy Universe
2015658 citationsA. C. A. Boogert, D. C. B. Whittet et al.profile →
Interstellar Ice: The Infrared Space Observatory Legacy
2004601 citationsD. C. B. Whittet, A. C. A. Boogert et al.profile →
Countries citing papers authored by D. C. B. Whittet
Since
Specialization
Citations
This map shows the geographic impact of D. C. B. Whittet'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 D. C. B. Whittet with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites D. C. B. Whittet more than expected).
Fields of papers citing papers by D. C. B. Whittet
This network shows the impact of papers produced by D. C. B. Whittet. 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 D. C. B. Whittet. The network helps show where D. C. B. Whittet may publish in the future.
Co-authorship network of co-authors of D. C. B. Whittet
This figure shows the co-authorship network connecting the top 25 collaborators of D. C. B. Whittet.
A scholar is included among the top collaborators of D. C. B. Whittet 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 D. C. B. Whittet. D. C. B. Whittet 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.
Zellner, N. E. B., J. W. Delano, T. D. Swindle, et al.. (2006). Did a Transient Increase in the Impact Flux Occur 800 Ma Ago. 37th Annual Lunar and Planetary Science Conference. 1745.1 indexed citations
2.
Zellner, N. E. B., et al.. (2005). Chemical and Isotopic Analyses of Apollo 16 Glasses: An Integrated Approach. 36th Annual Lunar and Planetary Science Conference. 1199.1 indexed citations
3.
Whittet, D. C. B.. (2005). Polarization Observations of Molecular Clouds. ASPC. 343. 321.3 indexed citations
4.
Zellner, N. E. B., J. W. Delano, T. D. Swindle, et al.. (2005). Earth-Moon Impacts at ~300 Ma and ~500 Ma Ago. 36th Annual Lunar and Planetary Science Conference. 1204.1 indexed citations
5.
Zellner, N. E. B., P. D. Spudis, J. W. Delano, D. C. B. Whittet, & T. D. Swindle. (2003). Geochemistry and Impact History at the Apollo 16 Landing Site. Lunar and Planetary Science Conference. 1007.5 indexed citations
Hassel, G. E., W. G. Roberge, D. C. B. Whittet, & S. Shenoy. (2003). Shock processing of icy grain mantles in protoplanetary disks. 788.1 indexed citations
8.
Spudis, P. D., et al.. (2002). Petrologic Mapping of the Moon: A New Approach. Lunar and Planetary Science Conference. 1104.9 indexed citations
9.
Chiar, J. E., A. G. G. M. Tielens, D. C. B. Whittet, et al.. (2000). The composition and distribution of dust along the line of sight toward the Galactic Center. University of Groningen research database (University of Groningen / Centre for Information Technology). 456. 45.1 indexed citations
10.
Kasting, J. F., D. C. B. Whittet, & W. R. Sheldon. (1996). The Effect of Ultraviolet Radiation on Planetary Habitability. LPI. 27. 655.1 indexed citations
11.
Roberge, W. G. & D. C. B. Whittet. (1996). Polarimetry of the interstellar medium : conference held at Rensselaer Polytechnic Institute, Troy, New York, 4-7 June 1995. Astronomical Society of the Pacific eBooks.1 indexed citations
12.
Whittet, D. C. B.. (1992). Books-Received - Dust in the Galactic Environment. Journal of the British Astronomical Association. 102. 230.1 indexed citations
13.
Davies, J. K., A. Evans, M. F. Bode, & D. C. B. Whittet. (1990). Photometric monitoring of pre-main-sequence stars. III, Variability of Herbig Ae/Be stars. Monthly Notices of the Royal Astronomical Society. 247(3). 517–522.7 indexed citations
14.
Adamson, A. J., D. C. B. Whittet, & W. W. Duley. (1990). The 3.4-mu.m interstellar absorption feature in CYG OB2 No 12.. Monthly Notices of the Royal Astronomical Society. 243(3). 400–404.46 indexed citations
15.
Assendorp, R., P. R. Wesselius, D. C. B. Whittet, & T. Prusti. (1990). A study of the Chamaeleon I dark cloud and T-association. II. High-resolution IRAS maps around HD 97048 and 97300.. Monthly Notices of the Royal Astronomical Society. 247(4). 624–631.7 indexed citations
16.
Whittet, D. C. B., W. W. Duley, & P. G. Martin. (1990). On the abundance of silicon carbide dust in the interstellar medium. Monthly Notices of the Royal Astronomical Society. 244(3). 427–431.32 indexed citations
17.
Whittet, D. C. B.. (1987). Infrared spectroscopy of interstellar dust.. Quarterly journal of the Royal Astronomical Society. 28. 303–311.1 indexed citations
18.
Whittet, D. C. B.. (1984). Bacteria in space: a limit based on ultraviolet absorption. Observatory. 104. 159–160.2 indexed citations
Whittet, D. C. B.. (1981). The Composition of Interstellar Grains. Quarterly journal of the Royal Astronomical Society. 22. 3.3 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.