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.
Type Ia Supernova Explosion Models
2000623 citationsW. Hillebrandt, J. C. Niemeyerprofile →
Three-dimensional delayed-detonation models with nucleosynthesis for Type Ia supernovae
2012290 citationsI. R. Seitenzahl, F. Ciaraldi-Schoolmann et al.Monthly Notices of the Royal Astronomical Societyprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
hero ref
Countries citing papers authored by W. Hillebrandt
Since
Specialization
Citations
This map shows the geographic impact of W. Hillebrandt'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 W. Hillebrandt with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites W. Hillebrandt more than expected).
This network shows the impact of papers produced by W. Hillebrandt. 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 W. Hillebrandt. The network helps show where W. Hillebrandt may publish in the future.
Co-authorship network of co-authors of W. Hillebrandt
This figure shows the co-authorship network connecting the top 25 collaborators of W. Hillebrandt.
A scholar is included among the top collaborators of W. Hillebrandt 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 W. Hillebrandt. W. Hillebrandt is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Seitenzahl, I. R., F. Ciaraldi-Schoolmann, F. K. Röpke, et al.. (2012). Three-dimensional delayed-detonation models with nucleosynthesis for Type Ia supernovae. Monthly Notices of the Royal Astronomical Society. 429(2). 1156–1172.290 indexed citations breakdown →
Röpke, F. K., W. Hillebrandt, & С. И. Блинников. (2006). On the mechanism of type Ia supernovae. Max Planck Institute for Plasma Physics. 637. 16.4 indexed citations
Stehle, M., P. A. Mazzali, S. Benetti, & W. Hillebrandt. (2004). Abundance Tomography of Type Ia Supernovae: I. The Case of SN 2002bo. arXiv (Cornell University).1 indexed citations
Hillebrandt, W., et al.. (1986). Nucleosynthesis in He-flashes on accreting white dwarfs.. 233. 125–136.1 indexed citations
17.
Kratz, Karl, W. Ziegert, W. Hillebrandt, & F.‐K. Thielemann. (1983). Determination of stellar neutron-capture rates for radioactive nuclei with the aid of beta-delayed neutron emission. CERN Document Server (European Organization for Nuclear Research). 125(2). 381–387.2 indexed citations
18.
Kratz, K.L., et al.. (1983). Beta-delayed neutron emission as the inverse process to neutron-capture on radioactive isotopes. Max Planck Institute for Plasma Physics. 90. 111–112.1 indexed citations
19.
Eid, M. F. El & W. Hillebrandt. (1980). A new equation of state of supernova matter.. Astronomy & Astrophysics Supplement Series. 42. 215–226.10 indexed citations
20.
Takahashi, K., M. F. El Eid, & W. Hillebrandt. (1978). Beta transition rates in hot and dense matter.. A&A. 67(2). 185–197.1 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.