This map shows the geographic impact of A. Winnberg'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 A. Winnberg with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites A. Winnberg more than expected).
This network shows the impact of papers produced by A. Winnberg. 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 A. Winnberg. The network helps show where A. Winnberg may publish in the future.
Co-authorship network of co-authors of A. Winnberg
This figure shows the co-authorship network connecting the top 25 collaborators of A. Winnberg.
A scholar is included among the top collaborators of A. Winnberg 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 A. Winnberg. A. Winnberg is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Kalenskiĭ, S. V., et al.. (2000). Probing the properties of methyl cyanide sources. Chalmers Publication Library (Chalmers University of Technology).9 indexed citations
8.
Вальтц, И. Е., et al.. (1995). The discovery of methanol masers at 107 GHz.. 170. 469–830.3 indexed citations
9.
Lindqvist, M., Å. Sandqvist, A. Winnberg, L. E. B. Johansson, & L. Å. Nyman. (1995). C^18^O and HNCO in the Galactic Centre. I. Observational data.. Astronomy & Astrophysics Supplement Series. 113. 257.7 indexed citations
10.
Langevelde, Huib Jan van, et al.. (1993). Monitoring OH/IR stars at the galactic centre with the VLA. Astronomy & Astrophysics Supplement Series. 101(1). 109–126.1 indexed citations
11.
Lindqvist, M., A. Winnberg, H. J. Habing, & H. E. Matthews. (1992). OH/IR stars close to the Galactic Centre. I - Observational data. Leiden Repository (Leiden University). 92(1). 43–62.1 indexed citations
12.
Nyman, L.-Å., R. S. Booth, H. J. Habing, et al.. (1992). A survey of circumstellar CO emission from a sample of IRAS point sources. Leiden Repository (Leiden University). 93(1). 121–150.2 indexed citations
Winnberg, A.. (1990). Comet Levy Detected by SEST. Msngr. 62. 66–67.1 indexed citations
15.
Winnberg, A., et al.. (1987). Detection of HCN in comet P/Halley. A&A. 172. 335–341.9 indexed citations
16.
Irvine, William M., F. P. Schloerb, Daryl A. Swade, et al.. (1983). The Visual Light Curves of Comets IRAS-Araki-Alcock 1983d and Sugano-Saigusa-Fujikawa 1983e. Bulletin of the American Astronomical Society. 15. 803.2 indexed citations
17.
Winnberg, A., D. A. Graham, C. M. Walmsley, & R. S. Booth. (1981). A new 1720 MHz OH outburst in V1057 Cyg.. A&A. 93. 79–84.
18.
Olnon, F. M., A. Winnberg, H. E. Matthews, & G. V. Schultz. (1980). Maser emission from infrared stars. I. New OH and H2O observations.. Astronomy & Astrophysics Supplement Series. 42. 119–133.2 indexed citations
19.
Baud, B., H. J. Habing, H. E. Matthews, & A. Winnberg. (1979). A systematic search at 1612 MHz for OH maser sources. II - A large-scale survey between L of 10 and 150 deg and /b/ less than or about equal to 4.2 deg. Leiden Repository (Leiden University). 36. 193–211.
20.
Baud, B., H. J. Habing, H. E. Matthews, & A. Winnberg. (1979). A systematic search at 1612 MHz for OH maser sources. I - Survey near the Galactic Centre. Leiden Repository (Leiden University). 35. 179–192.
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.