H. Wiesemeyer

5.8k citations
91 papers · 2.4k indexed · 1 hit paper · h-index 26
Topics
Astrophysics and Star Formation Studies (66 papers)Stellar, planetary, and galactic studies (46 papers)Atmospheric Ozone and Climate (25 papers)

In The Last Decade

H. Wiesemeyer

84 papers receiving 2.3k citations

Hit Papers

HERACLES: THE HERA CO LINE EXTRAGALACTIC SURVEY20092026201420202009100200300

Peers

H. Wiesemeyer
Comparison fields: 5 of 55
  • Astronomy and Astrophysics 2.1k
  • Spectroscopy 604
  • Atmospheric Science 423
  • Atomic and Molecular Physics, and Optics 286
  • Nuclear and High Energy Physics 207
Replace B. M. Swinyard with:
B. M. Swinyard United Kingdom
Tomoya Hirota Japan
T. R. Geballe United States
John H. Bieging United States
David M. Meyer United States
L. Decin Belgium
M. Schmidt Poland
David M. Mehringer United States
S. Hony France
T. R. Geballe United States
H. Wiesemeyer relative to B. M. Swinyard United Kingdom B. M. Swinyard's profile →
Citations per field
00.5×4.1×
B. M. Swinyard · 1×
Citations per year

Countries citing papers authored by H. Wiesemeyer

Since Specialization
Citations

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

Fields of papers citing papers by H. Wiesemeyer

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by H. Wiesemeyer. 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 H. Wiesemeyer. The network helps show where H. Wiesemeyer may publish in the future.

Co-authorship network of co-authors of H. Wiesemeyer

This figure shows the co-authorship network connecting the top 25 collaborators of H. Wiesemeyer. A scholar is included among the top collaborators of H. Wiesemeyer 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 H. Wiesemeyer. H. Wiesemeyer 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
#WorkIndexed citations
1 0
2 0
3 3
4 17
5 15
6 61
7 15
8 7
9 9
10 10
11 5
12 19
13 16
14 3
15 6
16 7
17 6
18 13
19
Structure and chemical composition of the silicate dust around OH/IR stars
18
20
ISOCAM observations of extremely young Class 0 candidates
1

About H. Wiesemeyer

H. Wiesemeyer is a scholar working on Astronomy and Astrophysics, Spectroscopy and Instrumentation, having authored 91 papers that have together received 2.4k indexed citations. Recurring topics across this work include Astrophysics and Star Formation Studies (66 papers), Stellar, planetary, and galactic studies (46 papers) and Atmospheric Ozone and Climate (25 papers). The work is most often cited by research in Astronomy and Astrophysics (2.1k citations), Instrumentation (174 citations) and Spectroscopy (604 citations). H. Wiesemeyer has collaborated with scholars based in Germany, France and United States. Frequent co-authors include R. Güsten, K. Schüster, C. Krämer, Fabian Walter, Frank Bigiel, W. J. G. de Blok, A. Usero, E. Brinks, Adam K. Leroy and K. M. Menten. Their work appears in journals such as Nature, Nature Communications and The Astrophysical Journal.

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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