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.
Superluminal motion of a relativistic jet in the neutron-star merger GW170817
2018333 citationsK. P. Mooley, Gregg Hallinan et al.profile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
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This map shows the geographic impact of A. Horesh'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. Horesh with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites A. Horesh more than expected).
This network shows the impact of papers produced by A. Horesh. 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. Horesh. The network helps show where A. Horesh may publish in the future.
Co-authorship network of co-authors of A. Horesh
This figure shows the co-authorship network connecting the top 25 collaborators of A. Horesh.
A scholar is included among the top collaborators of A. Horesh 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. Horesh. A. Horesh is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Tremou, Evangelia, Ian Heywood, S. D. Vergani, et al.. (2019). GRB 190114C: MeerKAT radio observation.. GCN. 23760. 1.1 indexed citations
9.
Jencson, J., M. M. Kasliwal, S. M. Adams, et al.. (2018). . Liverpool John Moores University.5 indexed citations
10.
Sfaradi, Itai, Joe Bright, A. Horesh, et al.. (2018). GRB 180720B: AMI-LA 15.5 GHz observation.. GRB Coordinates Network. 23037. 1.1 indexed citations
11.
Torres, M. A. P., Peter Lundqvist, J. Moldón, et al.. (2018). Radio constraints on the mass-loss rate of the Type Ia SN 2018gv. ATel. 11211. 1.1 indexed citations
Gezari, Suvi, T. Hung, N. Blagorodnova, et al.. (2016). iPTF16fnl: Likely Tidal Disruption Event at 65 Mpc. CaltechAUTHORS (California Institute of Technology). 9433. 1.
Arcavi, I., A. Gal‐Yam, Sagi Ben-Ami, et al.. (2012). PTF12os / PSN J14595904+0153251 is a Type IIb Supernova. The astronomer's telegram. 3881. 1.1 indexed citations
17.
Dyk, Schuyler D. Van, A. Gal‐Yam, I. Arcavi, M. M. Kasliwal, & A. Horesh. (2012). A Search for the Progenitor of Supernova PTF12os (PSN J14595904+0153251). ATel. 3884. 1.1 indexed citations
18.
Horesh, A., M. M. Kasliwal, John M. Carpenter, et al.. (2011). Radio observations of the young supernova PTF11iqb. ATel. 3512. 1.
19.
Arcavi, I., A. Gal‐Yam, David Polishook, et al.. (2011). PTF11eon/SN2011dh is Possibly a Type IIb Event. The astronomer's telegram. 3413. 1.1 indexed citations
20.
Kasliwal, M. M., S. R. Kulkarni, E. O. Ofek, et al.. (2010). PTF10acbp: A Luminous Red Nova in the Spiral UGC11973. ATel. 3094. 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.