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 6dF Galaxy Survey: baryon acoustic oscillations and the local Hubble constant
20111.6k citationsFlorian Beutler, Cullen H. Blake et al.Monthly Notices of the Royal Astronomical Societyprofile →
The 6dF Galaxy Survey: z≈ 0 measurements of the growth rate and σ8
2012318 citationsFlorian Beutler, Cullen H. Blake et al.Monthly Notices of the Royal Astronomical Societyprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
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Countries citing papers authored by Cullen H. Blake
Since
Specialization
Citations
This map shows the geographic impact of Cullen H. Blake'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 Cullen H. Blake with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Cullen H. Blake more than expected).
This network shows the impact of papers produced by Cullen H. Blake. 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 Cullen H. Blake. The network helps show where Cullen H. Blake may publish in the future.
Co-authorship network of co-authors of Cullen H. Blake
This figure shows the co-authorship network connecting the top 25 collaborators of Cullen H. Blake.
A scholar is included among the top collaborators of Cullen H. Blake 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 Cullen H. Blake. Cullen H. Blake is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Tröster, Tilman, Ariel G. Sánchez, Marika Asgari, et al.. (2019). Cosmology from large-scale structure. Astronomy and Astrophysics. 633. L10–L10.96 indexed citations
8.
Beichman, Charles, Cullen H. Blake, Justin R. Crepp, et al.. (2019). The need for single-mode fiber-fed spectrographs. Bulletin of the American Astronomical Society. 51(7). 122.
Beutler, Florian, Cullen H. Blake, Matthew Colless, et al.. (2012). The 6dF Galaxy Survey: z ≈0 measurement of the growth rate and sigma_8. arXiv (Cornell University).5 indexed citations
13.
Beutler, Florian, Cullen H. Blake, Matthew Colless, et al.. (2011). The 6dF Galaxy Survey: baryon acoustic oscillations and the local Hubble constant. Monthly Notices of the Royal Astronomical Society. 416(4). 3017–3032.1650 indexed citations breakdown →
Prochaska, J. X., M. Cooper, Jeffrey A. Newman, et al.. (2005). Keck/DEIMOS spectrum of possible host galaxy for GRB050509b.. GRB Coordinates Network. 3390. 1.
17.
Blake, Cullen H. & J. S. Bloom. (2004). GRB 041219: infrared afterglow candidate.. GRB Coordinates Network. 2870. 1.
18.
Blake, Cullen H.. (2004). A Torch for Passion. Journal of Hand Therapy. 17(1). 88–92.2 indexed citations
Mallén-Ornelas, G., Sara Seager, H. K. C. Yee, et al.. (2001). The EXPLORE Project: A Deep Search for Transiting Extrasolar Planets. American Astronomical Society Meeting Abstracts. 199. 14.2 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.