W. F. Hoffmann

6.9k total citations
120 papers, 1.8k citations indexed

About

W. F. Hoffmann is a scholar working on Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics and Instrumentation. According to data from OpenAlex, W. F. Hoffmann has authored 120 papers receiving a total of 1.8k indexed citations (citations by other indexed papers that have themselves been cited), including 86 papers in Astronomy and Astrophysics, 43 papers in Atomic and Molecular Physics, and Optics and 33 papers in Instrumentation. Recurrent topics in W. F. Hoffmann's work include Stellar, planetary, and galactic studies (62 papers), Astrophysics and Star Formation Studies (49 papers) and Adaptive optics and wavefront sensing (38 papers). W. F. Hoffmann is often cited by papers focused on Stellar, planetary, and galactic studies (62 papers), Astrophysics and Star Formation Studies (49 papers) and Adaptive optics and wavefront sensing (38 papers). W. F. Hoffmann collaborates with scholars based in United States, Germany and Netherlands. W. F. Hoffmann's co-authors include Joseph L. Hora, Philip M. Hinz, G. G. Fazio, Lynne K. Deutsch, Aditya Dayal, Michael R. Meyer, Eric E. Mamajek, P. M. Harvey, R. D. Gehrz and Nathan Smith and has published in prestigious journals such as Nature, Science and Journal of Geophysical Research Atmospheres.

In The Last Decade

W. F. Hoffmann

112 papers receiving 1.7k citations

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name h Career Trend Papers Cites
W. F. Hoffmann United States 23 1.6k 281 260 172 124 120 1.8k
Hirokazu Kataza Japan 21 1.3k 0.9× 165 0.6× 179 0.7× 201 1.2× 83 0.7× 136 1.5k
Michael E. Ressler United States 24 1.5k 1.0× 151 0.5× 231 0.9× 173 1.0× 135 1.1× 98 1.7k
C. H. Smith Australia 22 1.3k 0.9× 147 0.5× 128 0.5× 167 1.0× 173 1.4× 100 1.6k
A. Krabbe Germany 20 1.2k 0.8× 224 0.8× 213 0.8× 93 0.5× 76 0.6× 115 1.4k
Glenn Schneider United States 30 2.5k 1.6× 182 0.6× 473 1.8× 304 1.8× 131 1.1× 120 2.6k
Peter M. Onaka United States 11 1.3k 0.9× 126 0.4× 297 1.1× 102 0.6× 105 0.8× 32 1.5k
Hideo Matsuhara Japan 21 1.6k 1.1× 187 0.7× 502 1.9× 102 0.6× 82 0.7× 187 1.9k
G. L. Pilbratt Netherlands 16 1.6k 1.1× 143 0.5× 227 0.9× 354 2.1× 218 1.8× 46 1.8k
R. Millan‐Gabet United States 24 1.6k 1.1× 458 1.6× 424 1.6× 239 1.4× 60 0.5× 104 1.9k
G. Pilbratt Netherlands 8 1.6k 1.1× 121 0.4× 244 0.9× 316 1.8× 217 1.8× 18 1.8k

Countries citing papers authored by W. F. Hoffmann

Since Specialization
Citations

This map shows the geographic impact of W. F. Hoffmann'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 W. F. Hoffmann with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites W. F. Hoffmann more than expected).

Fields of papers citing papers by W. F. Hoffmann

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by W. F. Hoffmann. 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 W. F. Hoffmann. The network helps show where W. F. Hoffmann may publish in the future.

Co-authorship network of co-authors of W. F. Hoffmann

This figure shows the co-authorship network connecting the top 25 collaborators of W. F. Hoffmann. A scholar is included among the top collaborators of W. F. Hoffmann 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 W. F. Hoffmann. W. F. Hoffmann 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.
Isbell, J. W., Steve Ertel, Jörg‐Uwe Pott, et al.. (2025). Direct imaging of active galactic nucleus outflows and their origin with the 23 m Large Binocular Telescope. Nature Astronomy. 9(3). 417–427. 2 indexed citations
2.
Leisenring, Jarron, Dani Atkinson, W. F. Hoffmann, et al.. (2023). Evaluating the GeoSnap 13‐μ$$ \mu $$m cutoff HgCdTe detector for mid‐IR ground‐based astronomy. Astronomische Nachrichten. 344(8-9).
3.
Vitale, Michael G., Hiroko Matsumoto, Michael W. Kessler, W. F. Hoffmann, & David P. Roye. (2007). Osteogenesis Imperfecta. Journal of Pediatric Orthopaedics. 27(2). 228–232. 9 indexed citations
4.
Brandl, Bernhard R., W. F. Hoffmann, Joseph L. Hora, et al.. (2003). SIRTF-CTA optical performance test results. Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE. 4850. 30–30. 5 indexed citations
5.
Kraemer, K. E., James M. Jackson, Marc Kassis, et al.. (2003). Five Star‐forming Cores in the Galactic Ring Survey: A Mid‐Infrared Study. The Astrophysical Journal. 588(2). 918–930. 7 indexed citations
6.
Kraemer, K. E., James M. Jackson, Lynne K. Deutsch, et al.. (2001). Dust Characteristics of Massive Star‐forming Sites in the Mid‐Infrared. The Astrophysical Journal. 561(1). 282–298. 16 indexed citations
7.
Hinz, Philip M., J. R. P. Angel, N. J. Woolf, W. F. Hoffmann, & Donald W. McCarthy. (1999). Imaging Extra-solar Systems from the Ground: The MMT and LBT Nulling Interferometers. ASPC. 194. 401. 3 indexed citations
8.
Fernández, Y. R., Michael F. A’Hearn, C. M. Lisse, et al.. (1997). Physical Properties of the Nucleus of Comet Hale-Bopp. American Astronomical Society Meeting Abstracts. 191. 2 indexed citations
9.
Lisse, C. M., Y. R. Fernández, M. F. A’Hearn, et al.. (1997). Infrared Observations of the Dust Emitted by Comet Hale-Bopp. 4 indexed citations
10.
Fernández, Y. R., et al.. (1996). The Nucleus of Comet Hyakutake (C/1996 B2). 28. 2 indexed citations
11.
Marley, Mark S., Aditya Dayal, L. K. Deutsch, et al.. (1994). A Search for Seismic Waves Launched by the Impact of Comet Shoemaker-Levy/9. DPS. 26. 1580. 2 indexed citations
12.
Yanamandra-Fisher, P. A., W. F. Hoffmann, A. J. Friedson, et al.. (1993). 1993 SEB Revival: Expansion Phase. 25. 1 indexed citations
13.
Fazio, G. G., et al.. (1987). Structure in the nucleus of NGC 1068 at 10 microns. The Astrophysical Journal. 312. 542–542. 14 indexed citations
14.
Fazio, G. G., David Koch, Gary J. Melnick, et al.. (1984). A Wide Field and Diffraction Limited Array Camera for the Space Infrared Telescope Facility (SIRTF). Bulletin of the American Astronomical Society. 16. 906.
15.
Harvey, P. M., et al.. (1977). High-resolution far-infrared observations of H II regions - Sagittarius B2, W49, DR 21-W75. The Astrophysical Journal. 211. 786–786. 28 indexed citations
16.
Harvey, P. M., et al.. (1975). Far-infrared observations of W51 with high spatial resolution. The Astrophysical Journal. 196. L31–L31. 1 indexed citations
17.
Emery, R. J., C. Frederick, & W. F. Hoffmann. (1971). 100 Micron Map of the Galactic Center Region. Bulletin of the American Astronomical Society. 3. 15. 3 indexed citations
18.
Woolf, N. J., W. F. Hoffmann, C. Frederick, & F. J. Low. (1969). A discussion on infared astronomy - A far infrared sky survey. Philosophical Transactions of the Royal Society of London Series A Mathematical and Physical Sciences. 264(1150). 267–271. 1 indexed citations
19.
Hoffmann, W. F. & C. Frederick. (1969). Far-Infrared Observation of the Galactic-Center Region at 100 Microns. The Astrophysical Journal. 155. L9–L9. 31 indexed citations
20.
Hoffmann, W. F.. (1962). a Pendulum Gravimeter for Measurement of Periodic Annual Variations in the Gravitational Constant.. PhDT. 2 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.

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