G. Henri

20.1k total citations
40 papers, 772 citations indexed

About

G. Henri is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Electrical and Electronic Engineering. According to data from OpenAlex, G. Henri has authored 40 papers receiving a total of 772 indexed citations (citations by other indexed papers that have themselves been cited), including 36 papers in Astronomy and Astrophysics, 27 papers in Nuclear and High Energy Physics and 4 papers in Electrical and Electronic Engineering. Recurrent topics in G. Henri's work include Astrophysical Phenomena and Observations (30 papers), Astrophysics and Cosmic Phenomena (26 papers) and Pulsars and Gravitational Waves Research (13 papers). G. Henri is often cited by papers focused on Astrophysical Phenomena and Observations (30 papers), Astrophysics and Cosmic Phenomena (26 papers) and Pulsars and Gravitational Waves Research (13 papers). G. Henri collaborates with scholars based in France, Italy and United States. G. Henri's co-authors include G. Dubus, Benoît Cerutti, Pierre-Olivier Petrucci, Jonathan Ferreira, J. Malzac, G. Pelletier, L. Saugé, R. Bélmont, Guy Pelletier and S. Corbel and has published in prestigious journals such as The Journal of Chemical Physics, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

G. Henri

36 papers receiving 740 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. Henri France 19 700 409 76 72 46 40 772
F. Yusef‐Zadeh United States 20 1.1k 1.5× 503 1.2× 44 0.6× 70 1.0× 36 0.8× 41 1.1k
Jonathan Ferreira France 23 1.7k 2.4× 339 0.8× 58 0.8× 118 1.6× 147 3.2× 63 1.7k
Masayoshi Nobukawa Japan 15 492 0.7× 344 0.8× 25 0.3× 20 0.3× 14 0.3× 45 517
A. M. Dumont France 14 471 0.7× 172 0.4× 67 0.9× 53 0.7× 29 0.6× 43 544
R. M. Hjellming United States 15 602 0.9× 274 0.7× 20 0.3× 44 0.6× 15 0.3× 38 638
W. W. Tian China 16 654 0.9× 478 1.2× 23 0.3× 10 0.1× 21 0.5× 53 699
T. Viehmann Germany 12 565 0.8× 168 0.4× 24 0.3× 56 0.8× 9 0.2× 20 582
P. Varnière France 18 861 1.2× 195 0.5× 18 0.2× 29 0.4× 150 3.3× 40 895
Z. Abraham Brazil 13 515 0.7× 318 0.8× 23 0.3× 9 0.1× 27 0.6× 68 546
Christopher W. Mauche United States 15 599 0.9× 179 0.4× 27 0.4× 23 0.3× 6 0.1× 45 618

Countries citing papers authored by G. Henri

Since Specialization
Citations

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

Fields of papers citing papers by G. Henri

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

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

This figure shows the co-authorship network connecting the top 25 collaborators of G. Henri. A scholar is included among the top collaborators of G. Henri 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. Henri. G. Henri 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.
Petrucci, Pierre-Olivier, V. Piétu, Ehud Behar, et al.. (2023). Simultaneous millimetric and X-ray intraday variability in the radio-quiet AGN MCG+08-11-11. Astronomy and Astrophysics. 678. L4–L4. 6 indexed citations
2.
Ferreira, Jonathan, Pierre-Olivier Petrucci, Juan Rodríguez, et al.. (2022). Are low-frequency quasi-periodic oscillations in accretion flows the disk response to jet instability?. Astronomy and Astrophysics. 660. A66–A66. 13 indexed citations
3.
Petrucci, Pierre-Olivier, S. Bianchi, G. Ponti, et al.. (2021). Expected evolution of disk wind properties along an X-ray binary outburst. Astronomy and Astrophysics. 649. A128–A128. 9 indexed citations
4.
Ferreira, Jonathan, M. Clavel, Pierre-Olivier Petrucci, et al.. (2019). A unified accretion-ejection paradigm for black hole X-ray binaries. Astronomy and Astrophysics. 626. A115–A115. 39 indexed citations
5.
Ferreira, Jonathan, Pierre-Olivier Petrucci, G. Henri, et al.. (2018). A unified accretion-ejection paradigm for black hole X-ray binaries. Astronomy and Astrophysics. 615. A57–A57. 33 indexed citations
6.
Vuillaume, Thomas, et al.. (2018). A stratified jet model for AGN emission in the two-flow paradigm. Astronomy and Astrophysics. 620. A41–A41. 2 indexed citations
7.
Chakravorty, Susmita, Pierre-Olivier Petrucci, Jonathan Ferreira, et al.. (2016). Absorption lines from magnetically driven winds in X-ray binaries. Astronomy and Astrophysics. 589. A119–A119. 29 indexed citations
8.
Roland, J., et al.. (2015). Structure of the nucleus of 1928+738. Astronomy and Astrophysics. 578. A86–A86. 6 indexed citations
9.
Vuillaume, Thomas, et al.. (2015). Variation of bulk Lorentz factor in AGN jets due to Compton rocket in a complex photon field. Astronomy and Astrophysics. 581. A18–A18. 5 indexed citations
10.
Cerutti, Benoît, G. Dubus, J. Malzac, et al.. (2011). Absorption of high-energy gamma rays in Cygnus X-3. Springer Link (Chiba Institute of Technology). 21 indexed citations
11.
Petrucci, Pierre-Olivier, J. Ferreira, G. Henri, J. Malzac, & C. Foellmi. (2010). Relevance of jet emitting disc physics to microquasars: application to Cygnus X-1. Astronomy and Astrophysics. 522. A38–A38. 23 indexed citations
12.
Dubus, G., Benoît Cerutti, & G. Henri. (2010). Relativistic Doppler-boosted emission in gamma-ray binaries. Astronomy and Astrophysics. 516. A18–A18. 50 indexed citations
13.
Cerutti, Benoît, G. Dubus, & G. Henri. (2009). One-dimensional pair cascade emission in gamma-ray binaries. Astronomy and Astrophysics. 507(3). 1217–1224. 6 indexed citations
14.
Cerutti, Benoît, G. Dubus, & G. Henri. (2008). Spectral signature of a free pulsar wind in the gamma-raybinaries LS 5039 and LSI +61°303. Astronomy and Astrophysics. 488(1). 37–46. 19 indexed citations
15.
Dubus, G., Benoît Cerutti, & G. Henri. (2007). The modulation of the gamma-ray emission from the binary LS 5039. Astronomy and Astrophysics. 477(3). 691–700. 41 indexed citations
16.
Saugé, L. & G. Henri. (2006). On the dependence of the spectral parameters on the observational conditions in homogeneous time dependent models of the TeV blazars. Astronomy and Astrophysics. 454(1). L1–L4. 2 indexed citations
17.
Ferreira, Jonathan, Pierre-Olivier Petrucci, G. Henri, L. Saugé, & G. Pelletier. (2006). A unified accretion-ejection paradigm for black hole X-ray binaries. Astronomy and Astrophysics. 447(3). 813–825. 101 indexed citations
18.
Hannikainen, Diana, Juan Rodríguez, C. Cabanac, et al.. (2004). Discovery of a newINTEGRALsource: IGR J19140+0951. Astronomy and Astrophysics. 423(2). L17–L20. 11 indexed citations
19.
Petrucci, Pierre-Olivier, G. Henri, L. Maraschi, et al.. (2002). A rapidly variable narrow X-ray iron line in Mkn 841. Astronomy and Astrophysics. 388(1). L5–L8. 35 indexed citations
20.
Petrucci, Pierre-Olivier, G. Henri, & Guy Pelletier. (2001). Pair creation at shocks: \n Application to the high energy emission of compact objects. Springer Link (Chiba Institute of Technology). 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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