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.
Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
199811.5k citationsAdam G. Riess, P. Garnavich et al.profile →
Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
20042.7k citationsAdam G. Riess, J. Tonry et al.The Astrophysical Journalprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
hero ref
This map shows the geographic impact of B. Leibundgut'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 B. Leibundgut with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites B. Leibundgut more than expected).
This network shows the impact of papers produced by B. Leibundgut. 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 B. Leibundgut. The network helps show where B. Leibundgut may publish in the future.
Co-authorship network of co-authors of B. Leibundgut
This figure shows the co-authorship network connecting the top 25 collaborators of B. Leibundgut.
A scholar is included among the top collaborators of B. Leibundgut 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 B. Leibundgut. B. Leibundgut is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Leibundgut, B., et al.. (2003). Metrics to Measure ESO's Scientific Success. Msngr. 114. 46–49.1 indexed citations
16.
Napiwotzki, R., N. Christlieb, H. Drechsel, et al.. (2003). SPY - the ESO Supernovae type Ia Progenitor survey. University of Hertfordshire Research Archive (University of Hertfordshire). 112. 25–30.51 indexed citations
17.
Nakano, S., R. H. McNaught, S. Benetti, et al.. (1996). Novalike Variable in Sagittarius. International Astronomical Union Circular. 6322. 1.2 indexed citations
18.
Leibundgut, B., J. Spyromilio, J. R. Walsh, et al.. (1995). Discovery of a supernova (SN 1995K) at a redshift of 0.478.. The Messenger. 81. 19–20.2 indexed citations
19.
Mattarelli, Gianfranco & B. Leibundgut. (1991). [Initial experiences with prostaglandin E1 and PGE1 prepared injections].. PubMed. 58(3). 335–7.1 indexed citations
20.
Leibundgut, B., et al.. (1991). Supernova studies. VII : An atlas of light curves of supernovae type I. Astronomy & Astrophysics Supplement Series. 89(3). 537–579.1 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.