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.
A scheme to unify low-power accreting black holes
2004449 citationsH. Falcke, Sera Markoff et al.profile →
Formation of precessing jets by tilted black hole discs in 3D general relativistic MHD simulations
2017210 citationsMatthew Liska, Alexander Tchekhovskoy et al.Monthly Notices of the Royal Astronomical Society Lettersprofile →
Black Hole Flares: Ejection of Accreted Magnetic Flux through 3D Plasmoid-mediated Reconnection
2022181 citationsBart Ripperda, Matthew Liska et al.The Astrophysical Journal Lettersprofile →
Author Peers
Peers are selected by citation overlap in the author's most active subfields.
citations ·
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This map shows the geographic impact of Sera Markoff'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 Sera Markoff with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Sera Markoff more than expected).
This network shows the impact of papers produced by Sera Markoff. 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 Sera Markoff. The network helps show where Sera Markoff may publish in the future.
Co-authorship network of co-authors of Sera Markoff
This figure shows the co-authorship network connecting the top 25 collaborators of Sera Markoff.
A scholar is included among the top collaborators of Sera Markoff 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 Sera Markoff. Sera Markoff is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Lucchini, Matteo, et al.. (2022). . UvA-DARE (University of Amsterdam).8 indexed citations
9.
Ripperda, Bart, Matthew Liska, Koushik Chatterjee, et al.. (2022). Black Hole Flares: Ejection of Accreted Magnetic Flux through 3D Plasmoid-mediated Reconnection. The Astrophysical Journal Letters. 924(2). L32–L32.181 indexed citations breakdown →
10.
Haggard, Daryl, Melania Nynka, Michael A. Nowak, et al.. (2019). UvA-DARE (University of Amsterdam).10 indexed citations
Beuchert, Tobias, M. Kadler, M. Perucho, et al.. (2018). . Springer Link (Chiba Institute of Technology).9 indexed citations
14.
Dieckmann, M. E., G. Sarri, Sera Markoff, M. Borghesi, & M. Zepf. (2015). . Springer Link (Chiba Institute of Technology).2 indexed citations
15.
Schellart, P., A. Nelles, S. Buitink, et al.. (2013). UvA-DARE (University of Amsterdam).51 indexed citations
16.
Nowak, Michael A., Joey Neilsen, Sera Markoff, et al.. (2012). UvA-DARE (University of Amsterdam).61 indexed citations
17.
Gallo, Elena, S. Migliari, Sera Markoff, et al.. (2007). The spectral energy distribution of quiescent black hole X-ray binaries: new constraints from Spitze. Dipòsit Digital de la Universitat de Barcelona (Universitat de Barcelona).59 indexed citations
18.
Yuan, Ye‐Fei, Sera Markoff, H. Falcke, & Peter L. Biermann. (2002). NGC 4258: A jet-dominated low-luminosity AGN?. Springer Link (Chiba Institute of Technology).58 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.