M. Hendry

19.2k total citations · 1 hit paper
56 papers, 932 citations indexed

About

M. Hendry is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics. According to data from OpenAlex, M. Hendry has authored 56 papers receiving a total of 932 indexed citations (citations by other indexed papers that have themselves been cited), including 51 papers in Astronomy and Astrophysics, 10 papers in Instrumentation and 8 papers in Nuclear and High Energy Physics. Recurrent topics in M. Hendry's work include Pulsars and Gravitational Waves Research (23 papers), Gamma-ray bursts and supernovae (23 papers) and Cosmology and Gravitation Theories (16 papers). M. Hendry is often cited by papers focused on Pulsars and Gravitational Waves Research (23 papers), Gamma-ray bursts and supernovae (23 papers) and Cosmology and Gravitation Theories (16 papers). M. Hendry collaborates with scholars based in United Kingdom, United States and Mexico. M. Hendry's co-authors include R. P. Fender, Celia Escamilla‐Rivera, Mariusz P. Da̧browski, Konstantinos F. Dialektopoulos, Jurgen Mifsud, Viktor Gakis, Sebastián Bahamonde, Gabriel Farrugia, Jackson Levi Said and Eleonora Di Valentino and has published in prestigious journals such as Journal of the American Statistical Association, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

M. Hendry

50 papers receiving 886 citations

Hit Papers

Teleparallel gravity: from theory to cosmology 2022 2026 2023 2024 2022 100 200 300

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
M. Hendry United Kingdom 15 885 443 78 62 47 56 932
Cyril Pitrou France 21 1.3k 1.5× 687 1.6× 146 1.9× 79 1.3× 31 0.7× 52 1.4k
Mauro Pieroni Switzerland 18 908 1.0× 436 1.0× 172 2.2× 43 0.7× 18 0.4× 34 980
Suvodip Mukherjee India 17 1.1k 1.3× 277 0.6× 98 1.3× 22 0.4× 38 0.8× 66 1.2k
Kaze W. K. Wong United States 17 1.0k 1.2× 374 0.8× 69 0.9× 43 0.7× 23 0.5× 33 1.1k
C. Burigana Italy 16 1.1k 1.3× 610 1.4× 64 0.8× 105 1.7× 60 1.3× 92 1.2k
A. Torres-Forné Spain 16 691 0.8× 224 0.5× 72 0.9× 50 0.8× 13 0.3× 34 777
P. Väisänen South Africa 16 1.3k 1.4× 392 0.9× 49 0.6× 32 0.5× 246 5.2× 89 1.3k
Michael Kesden United States 25 1.9k 2.2× 646 1.5× 80 1.0× 45 0.7× 55 1.2× 46 2.0k
A. J. Banday Germany 17 1.1k 1.2× 536 1.2× 97 1.2× 79 1.3× 66 1.4× 27 1.1k
Joshua A. Faber United States 19 1.3k 1.4× 349 0.8× 50 0.6× 20 0.3× 39 0.8× 28 1.4k

Countries citing papers authored by M. Hendry

Since Specialization
Citations

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

Fields of papers citing papers by M. Hendry

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of M. Hendry

This figure shows the co-authorship network connecting the top 25 collaborators of M. Hendry. A scholar is included among the top collaborators of M. Hendry 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 M. Hendry. M. Hendry 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.
Seo, E. G., et al.. (2025). Residual Test to Search for Microlensing Signatures in Strongly Lensed Gravitational Wave Signals. The Astrophysical Journal. 988(2). 159–159.
2.
Congedo, G., et al.. (2024). Impact of weak lensing on bright standard siren analyses. Physical review. D. 110(2).
3.
Stachurski, F., C. Messenger, & M. Hendry. (2024). Cosmological inference using gravitational waves and normalizing flows. Physical review. D. 109(12). 5 indexed citations
4.
Saha, Surojit, M. J. Williams, L. E. H. Datrier, et al.. (2024). Rapid Generation of Kilonova Light Curves Using Conditional Variational Autoencoder. The Astrophysical Journal. 961(2). 165–165. 2 indexed citations
5.
Seo, E. G., Tjonnie G. F. Li, & M. Hendry. (2024). Inferring Properties of Dark Galactic Halos Using Strongly Lensed Gravitational Waves. The Astrophysical Journal. 966(1). 107–107. 4 indexed citations
6.
Wright, M., Justin Janquart, & M. Hendry. (2023). Determination of Lens Mass Density Profile from Strongly Lensed Gravitational-wave Signals. The Astrophysical Journal. 959(2). 70–70. 3 indexed citations
7.
Hendry, M., et al.. (2023). Reducing the impact of weak-lensing errors on gravitational-wave standard sirens. Monthly Notices of the Royal Astronomical Society. 522(3). 4059–4077. 8 indexed citations
9.
Escamilla‐Rivera, Celia, et al.. (2022). Neural networks and standard cosmography with newly calibrated high redshift GRB observations. Journal of Cosmology and Astroparticle Physics. 2022(4). 16–16. 11 indexed citations
10.
Bahamonde, Sebastián, Konstantinos F. Dialektopoulos, Celia Escamilla‐Rivera, et al.. (2022). Teleparallel gravity: from theory to cosmology. Reports on Progress in Physics. 86(2). 26901–26901. 318 indexed citations breakdown →
11.
Lamb, Gavin P., F. J. Hayes, A. K. H. Kong, et al.. (2021). Inclination Estimates from Off-Axis GRB Afterglow Modelling. Universe. 7(9). 329–329. 13 indexed citations
12.
Tong, Hui, et al.. (2021). Following up the afterglow: strategy for X-ray observation triggered by gravitational wave events. Research in Astronomy and Astrophysics. 21(12). 308–308. 5 indexed citations
13.
Teodoro, L. F. A., et al.. (2010). Completeness - II. A signal-to-noise ratio approach for completeness estimators applied to galaxy magnitude-redshift surveys. Monthly Notices of the Royal Astronomical Society. no–no. 1 indexed citations
14.
Cavaglià, M., M. Hendry, D. R. Ingram, et al.. (2008). Gravitational-wave Astronomy: Opening a New Window on the Universe for Students, Educators and the Public. Max Planck Digital Library. 400. 328–332. 1 indexed citations
15.
Hendry, M., et al.. (2006). Gamma Ray Bursts: Cosmic Rulers for the High-Redshift Universe?. 4 indexed citations
16.
Kanbur, Shashi M., Chow‐Choong Ngeow, S. Nikolaev, N. R. Tanvir, & M. Hendry. (2003). The extra-galactic Cepheid distance scale from LMC and Galactic period-luminosity relations. Springer Link (Chiba Institute of Technology). 35 indexed citations
17.
Ignace, Richard, et al.. (2003). Microlensing of circumstellar envelopes. Astronomy and Astrophysics. 401(1). 339–346. 2 indexed citations
18.
Hannah, I. G., L. Fletcher, & M. Hendry. (2002). Chaotic dynamics and collisionless reconnection at an X-type neutral point. 1. 295–298. 1 indexed citations
19.
Hendry, M., et al.. (2002). Gravitational microlensing as a test of stellar model atmospheres. Astronomy and Astrophysics. 388(1). L1–L4. 7 indexed citations
20.
Da̧browski, Mariusz P. & M. Hendry. (1997). Non-Uniform Pressure Universes: The Hubble Diagram of Type Ia Supernovae and the Age of the Universe. arXiv (Cornell University). 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.

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