This map shows the geographic impact of S. Immler'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. Immler with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites S. Immler more than expected).
This network shows the impact of papers produced by S. Immler. 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. Immler. The network helps show where S. Immler may publish in the future.
Co-authorship network of co-authors of S. Immler
This figure shows the co-authorship network connecting the top 25 collaborators of S. Immler.
A scholar is included among the top collaborators of S. Immler 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. Immler. S. Immler 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.
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
Sturm, R., F. Haberl, W. Pietsch, & S. Immler. (2011). IGR J05414-6858 detected in X-ray outburst with SWIFT. ATel. 3537. 1.
4.
Ryder, S. D., et al.. (2010). Radio Non-Detection of the Type IIb Supernova 2009mk in ESO 293-34. ATel. 2450. 1.2 indexed citations
5.
Ryder, S. D., R. Covarrubias, S. W. Amy, et al.. (2010). Supernova 2010as in NGC 6000. 2242. 1.1 indexed citations
6.
Pritchard, T. A. & S. Immler. (2010). Swift/UVOT observations of GRB100901A.. GCN. 11176. 1.1 indexed citations
7.
Mangano, V., W. H. Baumgartner, N. Gehrels, et al.. (2009). Swift triggered on the HMXB 1A 1118-61.. GRB Coordinates Network. 8777. 1.1 indexed citations
8.
Stockdale, Chris, K. W. Weiler, S. Immler, et al.. (2008). Radio rebrightening of SN 2008bo in NGC 6643. ATel. 1484. 1.1 indexed citations
9.
Page, K. L., S. Immler, A. P. Beardmore, et al.. (2008). Observations of an X-ray transient in NGC 2770.. 110. 1.
10.
Immler, S. & P. J. Brown. (2007). Swift Observations of SN 2007od. ATel. 1259. 1.1 indexed citations
11.
Immler, S. & P. J. Brown. (2007). Swift Observations of SN 2007on. The astronomer's telegram. 1261. 1.1 indexed citations
12.
Pooley, D., S. Immler, & A. V. Filippenko. (2007). Chandra Observation of SN 2005kd: Very Luminous and Hard X-ray Emission. ATel. 1023. 1.2 indexed citations
Immler, S. & D. Pooley. (2007). Detection of X-Ray Emission from SN 2005ip with Swift. ATel. 1004. 1.2 indexed citations
15.
Immler, S., et al.. (2007). Supernova 1987A : 20 years after : Supernovae and Gamma-Ray Bursters : Aspen, Colorado, 19-23 February 2007. American Institute of Physics eBooks.14 indexed citations
16.
Immler, S., F. E. Marshall, S. T. Holland, & M. Stamatikos. (2007). GRB070420: Swift UVOT continuing observations.. GCN. 6336. 1.1 indexed citations
17.
Immler, S., K. W. Weiler, & Richard McCray. (2007). SUPERNOVA 1987A: 20 YEARS AFTER: Supernovae and Gamma-Ray Bursters. AIPC. 937.87 indexed citations
18.
Immler, S., et al.. (2007). Possible Detection of SN 2007pk in X-Rays with Swift. ATel. 1284. 1.2 indexed citations
19.
Immler, S., et al.. (2007). Swift Observations of SN 2007af. ATel. 1020. 1.
20.
Immler, S., M. Modjaz, & P. J. Brown. (2006). Detection of SN 2006jc in X-Rays with Chandra. ATel. 934. 1.
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.