This map shows the geographic impact of R. Sturm'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 R. Sturm with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites R. Sturm more than expected).
This network shows the impact of papers produced by R. Sturm. 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 R. Sturm. The network helps show where R. Sturm may publish in the future.
Co-authorship network of co-authors of R. Sturm
This figure shows the co-authorship network connecting the top 25 collaborators of R. Sturm.
A scholar is included among the top collaborators of R. Sturm 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 R. Sturm. R. Sturm is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Maggi, P., R. Sturm, F. Haberl, G. Vasilopoulos, & A. Udalski. (2014). Swift J010745.0-722740, a new SMC Be/X-ray binary with possibly a very long orbital period. The astronomer's telegram. 5778. 1.1 indexed citations
5.
Vasilopoulos, G., R. Sturm, P. Maggi, & F. Haberl. (2014). The X-ray outburst of RX J0520.5-6932 is reaching the Eddington luminosity. ATel. 5760. 1.1 indexed citations
6.
Sturm, R. & F. Haberl. (2014). The diffuse X-ray emission of the Small Magellanic Cloud. 191.1 indexed citations
Vasilopoulos, G., P. Maggi, R. Sturm, et al.. (2013). X-ray outburst of RX J0520.5-6932, confirmed as a Be/X-ray binary. ATel. 4748. 1.1 indexed citations
10.
Maggi, P., R. Sturm, F. Haberl, & G. Vasilopoulos. (2013). Confirmation of XMMU J010429.4-723136 as a high-mass X-ray binary. ATel. 5674. 1.1 indexed citations
Haberl, F., R. Sturm, Masahiro Tsujimoto, et al.. (2012). SXP523 = Suzaku J0102-7204 = 2XMM J010247.4-720449, a Be/X-ray binary pulsar in the SMC. ATel. 4648. 1.1 indexed citations
16.
Sturm, R., F. Haberl, & W. Pietsch. (2011). Swift J053041.9-665426: a new LMC X-ray transient. The astronomer's telegram. 3747. 1.1 indexed citations
17.
Sturm, R., F. Haberl, W. Pietsch, & S. Immler. (2011). IGR J05414-6858 detected in X-ray outburst with SWIFT. ATel. 3537. 1.
18.
Sturm, R., F. Haberl, W. Pietsch, S. Immler, & A. Udalski. (2011). New SWIFT X-ray transient in the SMC: A new Be/X-ray binary?. ATel. 3575. 1.1 indexed citations
19.
Sturm, R., F. Haberl, & W. Pietsch. (2011). Swift J053041.9-665426 is most likely a Be/X-ray binary. The astronomer's telegram. 3753. 1.1 indexed citations
20.
Sturm, R., F. Haberl, W. Pietsch, & A. Udalski. (2011). 2XMM J010247.4-720449 is a Be/X-ray binary, detected in outburst with Swift. ATel. 3761. 1.1 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.