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.
The Lyman-Continuum Fluxes and Stellar Parameters of O and Early B-Type Stars
1996528 citationsWilliam D. Vacca, C. D. Garmany et al.The Astrophysical Journalprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
hero ref
This map shows the geographic impact of C. D. Garmany'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 C. D. Garmany with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites C. D. Garmany more than expected).
This network shows the impact of papers produced by C. D. Garmany. 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 C. D. Garmany. The network helps show where C. D. Garmany may publish in the future.
Co-authorship network of co-authors of C. D. Garmany
This figure shows the co-authorship network connecting the top 25 collaborators of C. D. Garmany.
A scholar is included among the top collaborators of C. D. Garmany 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 C. D. Garmany. C. D. Garmany is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Pompea, Stephen M., C. D. Garmany, Constance E. Walker, & S. K. Croft. (2006). Astronomy in Research-Based Science Education (A-RBSE): A Review of a Decade of Professional Development Programs in Support of Teacher and Student Research at the National Optical Astronomy Observatory. AGUFM. 2006.
3.
Pompea, Stephen M., S. K. Croft, C. D. Garmany, & Constance E. Walker. (2005). Evolution of a Teacher Professional Development Program that Promotes Teacher and Student Research. AGUFM. 2005.1 indexed citations
4.
Vacca, William D., C. D. Garmany, & J. Michael Shull. (1996). The Lyman-Continuum Fluxes and Stellar Parameters of O and Early B-Type Stars. The Astrophysical Journal. 460. 914–914.528 indexed citations breakdown →
Garmany, C. D. & R. E. Stencel. (1992). Galactic OB associations in the northern Milky Way Galaxy. I - Longitudes 55 deg to 150 deg. Astronomy & Astrophysics Supplement Series. 94(2). 211–244.3 indexed citations
7.
Garmany, C. D. & R. E. Stencel. (1991). Galactic OB Associations in the Northern Milky Way Galaxy. Bulletin of the American Astronomical Society. 23. 909.1 indexed citations
8.
Garmany, C. D.. (1990). Properties of Hot Luminous Stars: Boulder-Munich Workshop. Astronomical Society of the Pacific eBooks. 7.3 indexed citations
9.
Willis, A. J., I. D. Howarth, L. J. Smith, C. D. Garmany, & Peter S. Conti. (1989). Ultraviolet P-Cygni profile variations in HD 50896. Astronomy & Astrophysics Supplement Series. 77(2). 269–319.1 indexed citations
10.
Baade, D., Peter S. Conti, C. D. Garmany, et al.. (1988). O stars and Wolf-Rayet stars. NASA Technical Reports Server (NASA). 497.28 indexed citations
11.
Garmany, C. D. & N. R. Walborn. (1987). New O3 giants in the Large Magellanic Cloud. Publications of the Astronomical Society of the Pacific. 99. 240–240.12 indexed citations
Willis, A. J., K. A. van der Hucht, Peter S. Conti, & C. D. Garmany. (1986). An atlas of high resolution IUE ultraviolet spectra of 14 Wolf-Rayet stars.. Astronomy & Astrophysics Supplement Series. 63(3). 417–599.2 indexed citations
14.
Lamers, H. J. G. L. M., L. B. F. M. Waters, C. D. Garmany, M. R. Pérez, & C. Waelkens. (1986). HR 4049 - The hottest proto-planetary nebula star or a run-away hypergiant at high galactic latitude surrounded by a dust cloud?. 154.
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.