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.
This map shows the geographic impact of D. Bohlender'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. Bohlender with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites D. Bohlender more than expected).
This network shows the impact of papers produced by D. Bohlender. 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. Bohlender. The network helps show where D. Bohlender may publish in the future.
Co-authorship network of co-authors of D. Bohlender
This figure shows the co-authorship network connecting the top 25 collaborators of D. Bohlender.
A scholar is included among the top collaborators of D. Bohlender 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. Bohlender. D. Bohlender is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Bohlender, D., Daniel Durand, & Patrick Dowler. (2009). Astronomical data analysis software and systems XVIII : proceedings of a workshop held at Hotel Loews Le Concorde, Québec City, QC, Canada 2-5 November 2008. Astronomical Society of the Pacific eBooks.2 indexed citations
Gaudet, Suzanne, et al.. (2006). Gemini PI Electronic Transfer and Distribution (PIETD). NPARC. 351. 723.1 indexed citations
11.
Smith, M. A., G. A. Wade, D. Bohlender, & C. T. Bolton. (2006). The magnetic Bp star 36 Lyncis. Astronomy and Astrophysics. 458(2). 581–590.7 indexed citations
Shkolnik, Evgenya L., D. Bohlender, & G. A. H. Walker. (2002). Modulation of Ca II H and K Emission by Short-Period Planets. NPARC. 294. 157–160.
14.
Chu, You‐Hua, N. B. Suntzeff, J. E. Hesser, & D. Bohlender. (2001). Book Review: New views of the magellanic clouds / Astronomical Society of the Pacific, 1999. Observatory. 121(1160). 68.3 indexed citations
Schade, D., Patrick Dowler, D. Durand, et al.. (2000). A Data Mining Model for Astronomy. ASPC. 216. 215.1 indexed citations
17.
Chu, You‐Hua, N. B. Suntzeff, J. E. Hesser, & D. Bohlender. (1999). New views of the magellanic clouds : proceedings of the 190th symposium of the International Astronomical Union held in Victoria, Canada, 12-17 July 1998. Astronomical Society of the Pacific eBooks.1 indexed citations
18.
Bohlender, D., et al.. (1998). Isotopic anomalies of platinum in the Hg/Mn star HR 7775.. JRASC. 92(6). 310–311.1 indexed citations
19.
Bohlender, D. & J. D. Landstreet. (1990). A search for magnetic fields in Lambda Bootis stars.. Monthly Notices of the Royal Astronomical Society. 247(4). 606–610.21 indexed citations
20.
Bohlender, D. & J. D. Landstreet. (1988). The Peculiar Helium-Strong Star Delta Orionis C. Bulletin of the American Astronomical Society. 20. 699.1 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.