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, A. V. Filippenko et al.profile →
This map shows the geographic impact of B. Schmidt'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. Schmidt with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites B. Schmidt more than expected).
This network shows the impact of papers produced by B. Schmidt. 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. Schmidt. The network helps show where B. Schmidt may publish in the future.
Co-authorship network of co-authors of B. Schmidt
This figure shows the co-authorship network connecting the top 25 collaborators of B. Schmidt.
A scholar is included among the top collaborators of B. Schmidt 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. Schmidt. B. Schmidt is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Keller, Stefan, Andrew R. Casey, M. Asplund, et al.. (2015). HIGH-RESOLUTION SPECTROSCOPIC STUDY OF EXTREMELY METAL-POOR STAR CANDIDATES FROM THE SKYMAPPER SURVEY. DSpace@MIT (Massachusetts Institute of Technology).81 indexed citations
Monard, L. A. G., J. Brimacombe, M. Childress, et al.. (2014). Supernova 2014df in NGC 1448 = Psn J03442399-4440081. 3977. 1.
12.
Cahill, Reginald T., et al.. (2012). Discovery of Uniformly Expanding Universe. Progress in physics. 8. 65.5 indexed citations
13.
Cenko, S. B., D. B. Fox, A. Cucchiara, et al.. (2007). GRB070612A: Gemini spectroscopic redshift.. GCN. 6556. 1.1 indexed citations
14.
Ofek, E. O., S. B. Cenko, A. Gal‐Yam, et al.. (2006). GRB 060505 - OT candidate + galaxy spectrum.. GRB Coordinates Network. 5123. 1.3 indexed citations
15.
Soderberg, A. M., E. Berger, & B. Schmidt. (2006). GRB060218: optical spectroscopy of GRB-SN.. GRB Coordinates Network. 4804. 1.1 indexed citations
16.
Berger, E., N. Morrell, B. Schmidt, D. B. Fox, & P. B. Price. (2005). GRB 050412: LCO optical observations.. GRB Coordinates Network. 3239. 1.
17.
Schmidt, B., S. Keller, Paul Francis, & M. S. Bessell. (2005). The SkyMapper Telescope and Southern Sky Survey. 206.3 indexed citations
18.
Geisler, D., et al.. (2004). Wide-Field Washington Photometry of the NGC 5128 Globular Cluster System. 204.4 indexed citations
19.
Salvo, M., M. S. Bessell, & B. Schmidt. (2003). Supernova 2003hn in NGC 1448. IAUC. 8187. 1.1 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.