This map shows the geographic impact of S. Söderhjelm'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 S. Söderhjelm with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites S. Söderhjelm more than expected).
This network shows the impact of papers produced by S. Söderhjelm. 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 S. Söderhjelm. The network helps show where S. Söderhjelm may publish in the future.
Co-authorship network of co-authors of S. Söderhjelm
This figure shows the co-authorship network connecting the top 25 collaborators of S. Söderhjelm.
A scholar is included among the top collaborators of S. Söderhjelm 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 S. Söderhjelm. S. Söderhjelm 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.
Arenou, F. & S. Söderhjelm. (2008). Gaia Data Reduction Tasks for Double and Multiple Stars. Lund University Publications (Lund University).1 indexed citations
Söderhjelm, S.. (2005). Census of binaries - The big picture. Lund University Publications (Lund University). 576. 97–104.
5.
Söderhjelm, S.. (2004). Observing binaries with Gaia - the global picture. Lund University Publications (Lund University). 318. 413–421.1 indexed citations
Söderhjelm, S.. (1999). Possible detection of the planet transits of HD 209458 in the Hipparcos photometry. Information Bulletin on Variable Stars. 4816. 1.2 indexed citations
8.
Söderhjelm, S.. (1999). Visual binary orbits and masses POST HIPPARCOS. 341(1). 121–140.22 indexed citations
9.
Söderhjelm, S. & F. Mignard. (1998). Arcturus as a double star. Observatory. 118. 365–366.6 indexed citations
10.
Mignard, F., S. Söderhjelm, H.-H. Bernstein, et al.. (1995). Astrometry of double stars with HIPPARCOS. A&A. 304. 94.1 indexed citations
Lindegren, L., F. van Leeuwen, C S Petersen, M. A. C. Perryman, & S. Söderhjelm. (1992). Positions and parallaxes from the Hipparcos satellite. A first attempt at a global astrometric solution. Research at the University of Copenhagen (University of Copenhagen). 258(1). 134–141.2 indexed citations
13.
Lindegren, L., E. Høg, F. van Leeuwen, et al.. (1992). The NDAC Hipparcos data analysis consortium. Overview of the reduction methods. Research at the University of Copenhagen (University of Copenhagen). 258(1). 18–30.5 indexed citations
14.
Söderhjelm, S.. (1986). NDAC simulations of double and multiple stars: detectability and astrometric accuracy.. 155.1 indexed citations
Söderhjelm, S.. (1984). Third-order and tidal effects in the stellar three-body problem. A&A. 141(1). 232–240.3 indexed citations
17.
Söderhjelm, S.. (1982). Studies of the stellar three-body problem. 107(1). 54–60.6 indexed citations
18.
Söderhjelm, S. & L. Lindegren. (1982). Inertial Frame Determination Using Minor Planets. a Simulation of Hipparcos-Observations. 110. 156–162.4 indexed citations
19.
Söderhjelm, S.. (1980). Geometry and dynamics of the Algol system. 89. 100–112.7 indexed citations
20.
Söderhjelm, S.. (1978). MR Cyg and u Her: two similar eclipsing binaries.. 66. 161–168.4 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.