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.
An Empirical Background Model for the NICER X-Ray Timing Instrument
2022137 citationsRonald A. Remillard, Michael Loewenstein et al.The Astronomical Journalprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
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Countries citing papers authored by Abigail Stevens
Since
Specialization
Citations
This map shows the geographic impact of Abigail Stevens'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 Abigail Stevens with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Abigail Stevens more than expected).
This network shows the impact of papers produced by Abigail Stevens. 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 Abigail Stevens. The network helps show where Abigail Stevens may publish in the future.
Co-authorship network of co-authors of Abigail Stevens
This figure shows the co-authorship network connecting the top 25 collaborators of Abigail Stevens.
A scholar is included among the top collaborators of Abigail Stevens 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 Abigail Stevens. Abigail Stevens is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Remillard, Ronald A., Michael Loewenstein, James F. Steiner, et al.. (2022). An Empirical Background Model for the NICER X-Ray Timing Instrument. The Astronomical Journal. 163(3). 130–130.137 indexed citations breakdown →
Homan, J., P. Uttley, Keith C. Gendreau, et al.. (2018). Continuing NICER observations of the state transition in ASASSN-18ey/MAXI J1820+070. UvA-DARE (University of Amsterdam). 11823. 1.1 indexed citations
8.
Homan, J., Abigail Stevens, D. Altamirano, et al.. (2018). MAXI J1820+070 continuing its rapid evolution toward the hard state. UvA-DARE (University of Amsterdam). 12068. 1.2 indexed citations
9.
Homan, J., P. Uttley, Keith C. Gendreau, et al.. (2018). A rapid state transition in MAXI J1820+070. UvA-DARE (University of Amsterdam). 11820. 1.3 indexed citations
Trbojevic, D., V.M. Biryukov, Michael Harrison, et al.. (1998). A Study of RHIC crystal collimation. University of North Texas Digital Library (University of North Texas). 2146–2148.1 indexed citations
Allinger, J., et al.. (1977). Stability of high field superconducting dipole magnets. University of North Texas Digital Library (University of North Texas). 78. 19432.1 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.