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.
A luminous quasar at a redshift of z = 7.085
2011931 citationsD. Mortlock, S. J. Warren et al.Natureprofile →
Author Peers
Peers are selected by citation overlap in the author's most active subfields.
citations ·
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This map shows the geographic impact of A. Lawrence'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 A. Lawrence with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites A. Lawrence more than expected).
This network shows the impact of papers produced by A. Lawrence. 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 A. Lawrence. The network helps show where A. Lawrence may publish in the future.
Co-authorship network of co-authors of A. Lawrence
This figure shows the co-authorship network connecting the top 25 collaborators of A. Lawrence.
A scholar is included among the top collaborators of A. Lawrence 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 A. Lawrence. A. Lawrence is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Lawrence, A., Meredith L. Rawls, Moriba Jah, et al.. (2022). The case for space environmentalism. Nature Astronomy. 6(4). 428–435.67 indexed citations
4.
Charalampopoulos, P., G. Leloudas, D. Malesani, et al.. (2022). . Radboud Repository (Radboud University).36 indexed citations
5.
Nicholl, M., P. Short, A. Lawrence, Nicholas P. Ross, & S. J. Smartt. (2019). C-SNAILS spectra of optical transients. 59. 1.
6.
Cross, N. J. G., R. S. Collins, Robert G. Mann, et al.. (2012). The VISTA Science Archive. Astronomy and Astrophysics. 548. A119–A119.119 indexed citations
7.
Mortlock, D., S. J. Warren, Bram Venemans, et al.. (2011). A luminous quasar at a redshift of z = 7.085. Nature. 474(7353). 616–619.931 indexed citations breakdown →
Efstathiou, G., N. Kaiser, W. Saunders, et al.. (1990). Large scale clustering of IRAS galaxies. Monthly Notices of the Royal Astronomical Society. 247(2). 10–14.20 indexed citations
17.
Rowan-Robinson, M., A. Lawrence, W. Saunders, et al.. (1990). A sparse-sampled redshift survey of IRAS galaxies. I. The convergence of the IRAS dipole and the origin of our motion with respect to the microwave background.. Monthly Notices of the Royal Astronomical Society. 247(1). 1–18.50 indexed citations
18.
Lawrence, A.. (1987). Book Review: Light on dark matter. / Reidel, 1986.. Observatory. 107. 86.1 indexed citations
Schwartz, D., Michael Garcia, Maureen A. Conroy, et al.. (1980). Precise Location of 3A 2352+28: The High Galactic Latitude Transient A0000+28. Bulletin of the American Astronomical Society. 12. 513.1 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.