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 first gravitational-wave source from the isolated evolution of two stars in the 40–100 solar mass range
2016567 citationsKrzysztof Belczyński, D. E. Holz et al.profile →
Compact Object Modeling with the StarTrack Population Synthesis Code
2007468 citationsKrzysztof Belczyński, T. Bulik et al.profile →
ON THE MAXIMUM MASS OF STELLAR BLACK HOLES
2010404 citationsKrzysztof Belczyński, T. Bulik et al.The Astrophysical Journalprofile →
DOUBLE COMPACT OBJECTS. II. COSMOLOGICAL MERGER RATES
2013280 citationsKrzysztof Belczyński, Chris L. Fryer et al.The Astrophysical Journalprofile →
The effect of pair-instability mass loss on black-hole mergers
2016259 citationsKrzysztof Belczyński, Alexander Heger et al.Springer Link (Chiba Institute of Technology)profile →
MOCCA-SURVEY Database – I. Coalescing binary black holes originating from globular clusters
2016238 citationsAbbas Askar, D. Rosińska et al.profile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
hero ref
This map shows the geographic impact of T. Bulik'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 T. Bulik with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites T. Bulik more than expected).
This network shows the impact of papers produced by T. Bulik. 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 T. Bulik. The network helps show where T. Bulik may publish in the future.
Co-authorship network of co-authors of T. Bulik
This figure shows the co-authorship network connecting the top 25 collaborators of T. Bulik.
A scholar is included among the top collaborators of T. Bulik 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 T. Bulik. T. Bulik is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Belczynski, K., Jakub Klencki, G. Meynet, et al.. (2017). The origin of low spin of black holes in LIGO/Virgo mergers. arXiv (Cornell University).45 indexed citations
10.
Belczyński, Krzysztof, Alexander Heger, Wojciech Gładysz, et al.. (2016). The effect of pair-instability mass loss on black-hole mergers. Springer Link (Chiba Institute of Technology).259 indexed citations breakdown →
11.
Chruślińska, Martyna, Krzysztof Belczyński, T. Bulik, & Wojciech Gładysz. (2016). Constraints on the formation of double neutron stars from the observed eccentricities and current limits on merger rates. 67(1). 37–50.4 indexed citations
12.
Bulik, T. & I. Puerto-Giménez. (2011). The CTA site search. International Cosmic Ray Conference. 9. 223.1 indexed citations
13.
Bulik, T. & Krzysztof Belczyński. (2010). Observational evidence for stellar mass binary black holes and their coalescence rate. Memorie della Societa Astronomica Italiana. 81. 302.1 indexed citations
14.
Bulik, T., Krzysztof Belczyński, & Andrea Prestwich. (2008). IC10 X-1: the immediate progenitor of a double black hole binary. arXiv (Cornell University).1 indexed citations
Bulik, T., B. Rudak, & G. Madejski. (2005). Astrophysical sources of high energy particles and radiation : Toruń, Poland, 20-24 June 2005. American Institute of Physics eBooks.1 indexed citations
17.
Rosińska, D., T. Bulik, W. Kluźniak, J. L. Zdunik, & Éric Gourgoulhon. (2001). Innermost stable circular orbits around rotating compact quark stars and QPOs. CERN Bulletin. 459. 223–225.
18.
Bulik, T., et al.. (2000). Kilohertz QPOs, the marginally stable orbit, and the mass of the central sources - a maximum likelihood test. A&A. 361. 153–158.
Bulik, T., D. Rosińska, & W. Kluźniak. (1998). Kilohertz QPOs and strange stars. CERN Bulletin. 38. 77.1 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.