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.
Cold gas accretion in galaxies
2008361 citationsFilippo Fraternali, Tom Oosterloo et al.profile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
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Countries citing papers authored by J. M. van der Hulst
Since
Specialization
Citations
This map shows the geographic impact of J. M. van der Hulst'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 J. M. van der Hulst with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites J. M. van der Hulst more than expected).
Fields of papers citing papers by J. M. van der Hulst
This network shows the impact of papers produced by J. M. van der Hulst. 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 J. M. van der Hulst. The network helps show where J. M. van der Hulst may publish in the future.
Co-authorship network of co-authors of J. M. van der Hulst
This figure shows the co-authorship network connecting the top 25 collaborators of J. M. van der Hulst.
A scholar is included among the top collaborators of J. M. van der Hulst 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 J. M. van der Hulst. J. M. van der Hulst is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Verheijen, Marc, Bianca M. Poggianti, A. Moretti, et al.. (2022). GASP XXXIX: MeerKAT hunts Jellyfish in A2626. Monthly Notices of the Royal Astronomical Society. 516(2). 2683–2696.9 indexed citations
Molnár, D. Cs., P. Serra, J. M. van der Hulst, et al.. (2021). The Westerbork Coma Survey. Astronomy and Astrophysics. 659. A94–A94.13 indexed citations
McGaugh, Stacy, W. J. G. de Blok, & J. M. van der Hulst. (1996). Reverse Baryon Catastrophe in Extremely Dark Matter Dominated Galaxies. AAS. 189.1 indexed citations
14.
Hulst, J. M. van der. (1991). Intoxicatie met koolmonoxide. Nederlandsch tijdschrift voor geneeskunde/Nederlands tijdschrift voor geneeskunde/NTvG-databank. 135(15).1 indexed citations
15.
Hummel, E., J. M. van der Hulst, William C. Keel, & R. C. Kennicutt. (1987). The effects of interactions on spiral galaxies. III - A radio continuum survey of galactic nuclei at 1.49 GHz. Leiden Repository (Leiden University). 70. 517–530.2 indexed citations
16.
Hulst, J. M. van der & E. Hummel. (1985). The first detection of a radio continuum bridge between interacting galaxies.. A&A. 150.
17.
Sramek, R. A., K. W. Weiler, J. M. van der Hulst, & N. Panagia. (1984). The First Radio Light Curve for a Type I Supernova. Bulletin of the American Astronomical Society. 16. 541.2 indexed citations
18.
Albada, G.D. van & J. M. van der Hulst. (1982). New high resolution radio observations of NGC 4258.. A&A. 115. 263–269.1 indexed citations
19.
Weiler, K. W., J. M. van der Hulst, R. A. Sramek, & N. Panagia. (1980). A radio supernova in M100.. Bulletin of the American Astronomical Society. 12. 752.1 indexed citations
20.
Bosma, A., et al.. (1977). A neutral hydrogen study of the spiral galaxy NGC 4736.. Data Archiving and Networked Services (DANS). 57(3). 373–381.7 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.