Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies
if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the
same subfield and year (this is the minimum needed to enter the top 1%, not the average
within it), or reaches the top citation threshold in at least one of its specific research
topics.
THE DENSE MATTER EQUATION OF STATE FROM NEUTRON STAR RADIUS AND MASS MEASUREMENTS
2016248 citationsC. O. Heinke, Sébastien Guillot et al.The Astrophysical Journalprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
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This map shows the geographic impact of C. O. Heinke'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 C. O. Heinke with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites C. O. Heinke more than expected).
This network shows the impact of papers produced by C. O. Heinke. 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 C. O. Heinke. The network helps show where C. O. Heinke may publish in the future.
Co-authorship network of co-authors of C. O. Heinke
This figure shows the co-authorship network connecting the top 25 collaborators of C. O. Heinke.
A scholar is included among the top collaborators of C. O. Heinke 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 C. O. Heinke. C. O. Heinke is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Eijnden, J. van den, N. Degenaar, T. D. Russell, et al.. (2021). A new radio census of neutron star X-ray binaries. Monthly Notices of the Royal Astronomical Society. 507(3). 3899–3922.41 indexed citations
Shaw, A. W., John A. Tomsick, K. Mukai, et al.. (2018). Measuring the masses of intermediate polars with NuSTAR. cosp. 42.1 indexed citations
13.
Eijnden, J. van den, N. Degenaar, R. Wijnands, et al.. (2018). VLA radio detection of the very-faint X-ray transient IGR J17285-2922. UvA-DARE (University of Amsterdam). 11487. 1.
Homan, J., G. R. Sivakoff, D. Pooley, et al.. (2016). Chandra identification of the X-ray transient MAXI J0911-635/Swift J0911.9-6452 in NGC 2808. ATel. 8971. 1.1 indexed citations
Bahramian, Arash, C. O. Heinke, G. R. Sivakoff, et al.. (2013). No indication of X-ray activity in Terzan 1 from a short Swift/XRT observation. UvA-DARE (University of Amsterdam). 5116. 1.
18.
Gladstone, Jeanette C., et al.. (2011). Optical counterparts to ultraluminous x-ray sources. 77.1 indexed citations
19.
Sivakoff, G. R., C. O. Heinke, J. C. A. Miller‐Jones, et al.. (2011). Chandra HRC confirms that M15 X-2 is the currently flaring source in M15. UvA-DARE (University of Amsterdam). 3393. 1.
20.
Patruno, Alessandro, D. Altamirano, Anna L. Watts, et al.. (2010). Detection of pulsations and identification of SAX J1748.9-2021 as the X-ray transient in NGC 6440.. UvA-DARE (University of Amsterdam). 2407. 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.