G. Nelemans

108.8k total citations
218 papers, 6.8k citations indexed

About

G. Nelemans is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics. According to data from OpenAlex, G. Nelemans has authored 218 papers receiving a total of 6.8k indexed citations (citations by other indexed papers that have themselves been cited), including 209 papers in Astronomy and Astrophysics, 36 papers in Instrumentation and 25 papers in Nuclear and High Energy Physics. Recurrent topics in G. Nelemans's work include Gamma-ray bursts and supernovae (150 papers), Stellar, planetary, and galactic studies (113 papers) and Astrophysical Phenomena and Observations (103 papers). G. Nelemans is often cited by papers focused on Gamma-ray bursts and supernovae (150 papers), Stellar, planetary, and galactic studies (113 papers) and Astrophysical Phenomena and Observations (103 papers). G. Nelemans collaborates with scholars based in Netherlands, Belgium and United Kingdom. G. Nelemans's co-authors include Simon Portegies Zwart, L. R. Yungelson, Silvia Toonen, D. Steeghs, F. Verbunt, P. Groot, P. G. Jonker, T. R. Marsh, G. H. A. Roelofs and J. P. Lasota and has published in prestigious journals such as Nature, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

G. Nelemans

209 papers receiving 6.5k citations

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name h Career Trend Papers Cites
G. Nelemans Netherlands 43 6.6k 988 715 401 271 218 6.8k
Philipp Podsiadlowski United Kingdom 53 9.6k 1.5× 1.6k 1.6× 1.1k 1.5× 588 1.5× 277 1.0× 172 9.9k
Krzysztof Belczyński Poland 45 7.2k 1.1× 530 0.5× 1.1k 1.5× 389 1.0× 100 0.4× 140 7.4k
S. E. de Mink Netherlands 52 9.8k 1.5× 2.8k 2.8× 775 1.1× 204 0.5× 277 1.0× 157 10.1k
R. H. D. Townsend United States 36 7.8k 1.2× 2.0k 2.0× 491 0.7× 313 0.8× 371 1.4× 104 8.1k
Matteo Cantiello United States 32 8.5k 1.3× 2.6k 2.7× 560 0.8× 253 0.6× 252 0.9× 78 8.7k
A. Udalski Poland 38 5.5k 0.8× 1.9k 1.9× 576 0.8× 180 0.4× 341 1.3× 301 5.6k
A. Merloni Germany 38 5.5k 0.8× 1.1k 1.1× 2.0k 2.9× 166 0.4× 155 0.6× 147 5.8k
P. P. Eggleton Russia 34 7.3k 1.1× 1.8k 1.8× 446 0.6× 376 0.9× 234 0.9× 101 7.5k
A. S. Fruchter United States 40 5.5k 0.8× 1.2k 1.2× 1.2k 1.6× 237 0.6× 68 0.3× 140 5.7k
N. Gehrels United States 46 8.1k 1.2× 731 0.7× 2.7k 3.8× 300 0.7× 179 0.7× 201 8.4k

Countries citing papers authored by G. Nelemans

Since Specialization
Citations

This map shows the geographic impact of G. Nelemans'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 G. Nelemans with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites G. Nelemans more than expected).

Fields of papers citing papers by G. Nelemans

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by G. Nelemans. 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 G. Nelemans. The network helps show where G. Nelemans may publish in the future.

Co-authorship network of co-authors of G. Nelemans

This figure shows the co-authorship network connecting the top 25 collaborators of G. Nelemans. A scholar is included among the top collaborators of G. Nelemans 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 G. Nelemans. G. Nelemans is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

20 of 20 papers shown
1.
Kupfer, Thomas, Valeriya Korol, T. B. Littenberg, et al.. (2024). LISA Galactic Binaries with Astrometry from Gaia DR3. The Astrophysical Journal. 963(2). 100–100. 30 indexed citations
2.
Bhattacharyya, Saptashwa, Roberto Ruiz de Austri, S. Caron, et al.. (2023). AutoSourceID-Classifier. Astronomy and Astrophysics. 680. A109–A109. 8 indexed citations
3.
Austri, Roberto Ruiz de, Saptashwa Bhattacharyya, S. Caron, et al.. (2023). AutoSourceID-FeatureExtractor. Astronomy and Astrophysics. 680. A108–A108. 4 indexed citations
4.
Tak, F. van der, L. Burtscher, Simon Portegies Zwart, et al.. (2021). The carbon footprint of astronomy research in the Netherlands. Nature Astronomy. 5(12). 1195–1198. 11 indexed citations
5.
Klencki, Jakub, G. Nelemans, Alina Istrate, & Onno R. Pols. (2020). Massive donors in interacting binaries: effect of metallicity. Springer Link (Chiba Institute of Technology). 55 indexed citations
6.
Chruślińska, Martyna, Tereza Jeřabková, G. Nelemans, & Zhiqiang Yan. (2020). The effect of the environment-dependent IMF on the formation and metallicities of stars over the cosmic history. Springer Link (Chiba Institute of Technology). 27 indexed citations
7.
Winckel, H. Van, et al.. (2019). Modelling depletion by re-accretion of gas from a dusty disc in post-AGB stars. Springer Link (Chiba Institute of Technology). 34 indexed citations
8.
Harst, Pim van der, G. Nelemans, Else Starkenburg, et al.. (2017). White dwarfs in the building blocks of the Galactic spheroid. Springer Link (Chiba Institute of Technology). 1 indexed citations
9.
Ghosh, Shaon, S. Bloemen, G. Nelemans, P. Groot, & Larry R. Price. (2016). Tiling strategies for optical follow-up of gravitational-wave triggers by telescopes with a wide field of view. Springer Link (Chiba Institute of Technology). 20 indexed citations
10.
Nelemans, G., et al.. (2015). Population synthesis of classical low-mass X-ray binaries in the Galactic Bulge. Springer Link (Chiba Institute of Technology). 11 indexed citations
11.
Harst, Pim van der, G. Nelemans, Silvia Toonen, et al.. (2014). Binary white dwarfs in the halo of the Milky Way. Springer Link (Chiba Institute of Technology). 9 indexed citations
12.
Nelemans, G., R. Voss, Silvia Toonen, et al.. (2013). Population synthesis of ultracompact X-ray binaries in the Galactic bulge. Springer Link (Chiba Institute of Technology). 21 indexed citations
13.
Bours, M. C. P., Silvia Toonen, & G. Nelemans. (2013). Single degenerate supernova type Ia progenitors : Studying the influence of different mass retention efficiencies. Data Archiving and Networked Services (DANS). 34 indexed citations
14.
Voss, R. & G. Nelemans. (2012). Type Ia supernovae in globular clusters: observational upper limits. Springer Link (Chiba Institute of Technology). 5 indexed citations
15.
Nelemans, G., et al.. (2012). The evolution of ultracompact X-ray binaries. Springer Link (Chiba Institute of Technology). 27 indexed citations
16.
Voss, R., et al.. (2012). Long-term luminosity behavior of 14 ultracompact X-ray binaries. Springer Link (Chiba Institute of Technology). 14 indexed citations
17.
Nelemans, G., et al.. (2012). Formation of the planet around the millisecond pulsar J1719–1438. Springer Link (Chiba Institute of Technology). 23 indexed citations
18.
Hu, Haili, M.‐A. Dupret, C. Aerts, et al.. (2008). A seismic approach to testing different formation channels of subdwarf B stars. Springer Link (Chiba Institute of Technology). 17 indexed citations
19.
Lasota, J. P., G. Nelemans, G. Dubus, et al.. (2006). . UvA-DARE (University of Amsterdam). 34 indexed citations
20.
Nelemans, G.. (2006). \nUltracompact binary stars. Radboud Repository (Radboud University). 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.

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