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.
Direct Imaging of Multiple Planets Orbiting the Star HR 8799
2008871 citationsChristian Marois, Bruce Macintosh et al.profile →
Images of a fourth planet orbiting HR 8799
2010464 citationsChristian Marois, B. Zuckerman et al.profile →
Author Peers
Peers are selected by citation overlap in the author's most active subfields.
citations ·
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Countries citing papers authored by Bruce Macintosh
Since
Specialization
Citations
This map shows the geographic impact of Bruce Macintosh'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 Bruce Macintosh with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Bruce Macintosh more than expected).
This network shows the impact of papers produced by Bruce Macintosh. 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 Bruce Macintosh. The network helps show where Bruce Macintosh may publish in the future.
Co-authorship network of co-authors of Bruce Macintosh
This figure shows the co-authorship network connecting the top 25 collaborators of Bruce Macintosh.
A scholar is included among the top collaborators of Bruce Macintosh 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 Bruce Macintosh. Bruce Macintosh is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Douglas, Ewan S., et al.. (2018). WFIRST: Update on the Coronagraph Science Requirements. 231.1 indexed citations
8.
Galicher, R., Christian Marois, Bruce Macintosh, et al.. (2016). The International Deep Planet Survey. Astronomy and Astrophysics. 594. A63–A63.68 indexed citations
Soummer, Rémi, et al.. (2006). The Gemini Planet Imager Apodized Pupil Lyot Coronagraph. American Astronomical Society Meeting Abstracts. 209.1 indexed citations
13.
Guenther, E. W., Diane B. Paulson, William D. Cochran, et al.. (2005). Low-mass companions to Hyades stars. Springer Link (Chiba Institute of Technology).14 indexed citations
14.
Gibbard, S. G., et al.. (2003). Spatially-Resolved 2 micron Spectroscopy of Titan from the W.M. Keck Telescope.1 indexed citations
15.
Roe, H. G., et al.. (2001). The Morphology and Motions of storm features on Neptune on minute and hour timescales. DPS. 33.1 indexed citations
16.
Gibbard, S. G., et al.. (2001). 2-micron Adaptive Optics Images of Titan from the W.M. Keck Telescope. AAS. 199.1 indexed citations
17.
Gibbard, S. G., Bruce Macintosh, C. E. Max, et al.. (2000). The Surface of Titan from Adaptive Optics Observations. 24. 11.1 indexed citations
18.
Gavel, Donald T., et al.. (1997). Direct Imaging of Extra-solar Planets. University of North Texas Digital Library (University of North Texas). 134. 262.1 indexed citations
19.
Macintosh, Bruce, et al.. (1997). Volcanoes on Io: High-Resolution Infrared Images Using Speckle Interferometry with the Keck Telescope. Bulletin of the American Astronomical Society. 29. 745.1 indexed citations
20.
McLean, Ian S., Bruce Macintosh, Tao Liu, et al.. (1994). Performance and results with a double-beam infrared camera.. Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE. 2198. 457–466.3 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.