Y. A. Gallant

18.5k total citations
39 papers, 1.1k citations indexed

About

Y. A. Gallant is a scholar working on Nuclear and High Energy Physics, Astronomy and Astrophysics and Statistical and Nonlinear Physics. According to data from OpenAlex, Y. A. Gallant has authored 39 papers receiving a total of 1.1k indexed citations (citations by other indexed papers that have themselves been cited), including 30 papers in Nuclear and High Energy Physics, 29 papers in Astronomy and Astrophysics and 2 papers in Statistical and Nonlinear Physics. Recurrent topics in Y. A. Gallant's work include Astrophysics and Cosmic Phenomena (28 papers), Gamma-ray bursts and supernovae (21 papers) and Pulsars and Gravitational Waves Research (13 papers). Y. A. Gallant is often cited by papers focused on Astrophysics and Cosmic Phenomena (28 papers), Gamma-ray bursts and supernovae (21 papers) and Pulsars and Gravitational Waves Research (13 papers). Y. A. Gallant collaborates with scholars based in France, Germany and United States. Y. A. Gallant's co-authors include A. Achterberg, J. G. Kirk, J. Ballet, Alexandre Marcowith, E. van der Swaluw, E. Parizot, G. Tóth, Olaf Skjæraasen, G. Dubus and M. Renaud and has published in prestigious journals such as Monthly Notices of the Royal Astronomical Society, Astronomy and Astrophysics and The Astrophysical Journal Letters.

In The Last Decade

Y. A. Gallant

35 papers receiving 1.0k citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
Y. A. Gallant France 15 953 886 20 20 15 39 1.1k
E. Giacani Argentina 18 1.0k 1.1× 900 1.0× 16 0.8× 23 1.1× 12 0.8× 49 1.1k
R. Bandiera Italy 21 839 0.9× 573 0.6× 30 1.5× 27 1.4× 8 0.5× 60 871
Joseph D. Gelfand United States 16 912 1.0× 647 0.7× 31 1.6× 53 2.6× 14 0.9× 58 1.0k
Y. C. Lin United States 17 705 0.7× 666 0.8× 19 0.9× 26 1.3× 14 0.9× 50 815
D. K. Milne Australia 17 734 0.8× 536 0.6× 26 1.3× 21 1.1× 14 0.9× 72 758
D. Khangulyan Japan 21 1.2k 1.2× 952 1.1× 11 0.6× 67 3.4× 19 1.3× 54 1.3k
Antonella Fruscione United States 11 755 0.8× 373 0.4× 13 0.7× 38 1.9× 50 3.3× 34 792
Daniel Patnaude United States 17 700 0.7× 472 0.5× 30 1.5× 32 1.6× 29 1.9× 50 718
D. A. Grabelsky United States 16 794 0.8× 412 0.5× 11 0.6× 36 1.8× 26 1.7× 43 854
Anthony H. Minter United States 10 440 0.5× 195 0.2× 11 0.6× 16 0.8× 21 1.4× 23 461

Countries citing papers authored by Y. A. Gallant

Since Specialization
Citations

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

Fields of papers citing papers by Y. A. Gallant

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by Y. A. Gallant. 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 Y. A. Gallant. The network helps show where Y. A. Gallant may publish in the future.

Co-authorship network of co-authors of Y. A. Gallant

This figure shows the co-authorship network connecting the top 25 collaborators of Y. A. Gallant. A scholar is included among the top collaborators of Y. A. Gallant 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 Y. A. Gallant. Y. A. Gallant 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.
Gallant, Y. A., R. Bandiera, N. Bucciantini, & Elena Amato. (2017). Constraining pulsar birth properties with supernova X-ray observations. Proceedings of the International Astronomical Union. 12(S331). 63–68. 1 indexed citations
2.
Acero, F., Y. A. Gallant, J. Ballet, M. Renaud, & R. Terrier. (2013). A new nearby pulsar wind nebula overlapping the RX J0852.0−4622 supernova remnant. Astronomy and Astrophysics. 551. A7–A7. 19 indexed citations
3.
Zajczyk, A., Y. A. Gallant, Patrick Slane, et al.. (2012). Infrared imaging and polarimetric observations of the pulsar wind nebula in SNR G21.5-0.9. Astronomy and Astrophysics. 542. A12–A12. 17 indexed citations
4.
Wilhelmi, E. de Oña, B. Rudak, J. A. Barrio, et al.. (2012). Prospects for observations of pulsars and pulsar wind nebulae with CTA. Astroparticle Physics. 43. 287–300. 20 indexed citations
5.
Acero, F., Y. A. Gallant, R. Terrier, M. Renaud, & J. Ballet. (2011). A new nearby PWN overlapping the Vela Jr SNR. MmSAI. 82. 752. 1 indexed citations
6.
Feinstein, F., A. Fiaßon, Y. A. Gallant, et al.. (2009). What do supernova remnants interacting with molecular clouds reveal?. AIP conference proceedings. 54–62. 7 indexed citations
7.
Fiaßon, A., K. Kosack, J. L. Skilton, et al.. (2008). Probing cosmic ray acceleration through molecular clouds in the vicinity of supernova remnant with H.E.S.S.. AIP conference proceedings. 361–363. 2 indexed citations
8.
Gallant, Y. A., S. Carrigan, A. Djannati-Ataï, et al.. (2008). VHE γ-ray emitting pulsar wind nebulae discovered by H.E.S.S.. AIP conference proceedings. 983. 195–199. 6 indexed citations
9.
Hinton, J. A., S. Funk, S. Carrigan, et al.. (2007). Discovery of an X-ray nebula around PSR J1718-3825 and implications for the nature of the γ-ray source HESS J1718–385. Astronomy and Astrophysics. 476(3). L25–L28. 6 indexed citations
10.
Ter–Antonyan, S., et al.. (2007). Rigidity-dependent cosmic ray energy spectra in the knee region obtained with the GAMMA experiment. Astroparticle Physics. 28(2). 169–181. 17 indexed citations
11.
Bocchino, F., R. Bandiera, & Y. A. Gallant. (2007). XMM-Newton survey of non-thermal shell candidates: Preliminary results on DA 530. Advances in Space Research. 41(3). 407–410. 3 indexed citations
12.
Parizot, E., Alexandre Marcowith, J. Ballet, & Y. A. Gallant. (2006). Observational constraints on energetic particle diffusion in young supernovae remnants: amplified magnetic field and maximum energy. Astronomy and Astrophysics. 453(2). 387–395. 135 indexed citations
13.
Ter–Antonyan, S., et al.. (2005). All-particle primary energy spectrum in the knee region. ICRC. 6. 105.
14.
Swaluw, E. van der, A. Achterberg, Y. A. Gallant, T. P. Downes, & Rony Keppens. (2003). Interaction of high-velocity pulsars with supernova remnant shells. Springer Link (Chiba Institute of Technology). 35 indexed citations
15.
Kirk, J. G., Olaf Skjæraasen, & Y. A. Gallant. (2002). Pulsed radiation from neutron star winds. Astronomy and Astrophysics. 388(2). L29–L32. 48 indexed citations
16.
Swaluw, E. van der, A. Achterberg, Y. A. Gallant, & G. Tóth. (2001). Pulsar wind nebulae in supernova remnants. Astronomy and Astrophysics. 380(1). 309–317. 104 indexed citations
17.
Gallant, Y. A. & R. J. Tuffs. (1999). Infrared observations of plerionic supernovae remnants: high-energy astrophysics with ISO. ESASP. 427. 313. 2 indexed citations
18.
Swaluw, E. van der, A. Achterberg, & Y. A. Gallant. (1998). Hydrodynamical simulations of pulsar wind nebulae in supernova remnants. Memorie della Societa Astronomica Italiana. 69. 1017. 4 indexed citations
19.
Gallant, Y. A. & R. J. Tuffs. (1998). Infrared Observations of Plerions With ISO. MmSAI. 69. 237–970. 5 indexed citations
20.
Duffy, P., J. G. Kirk, Y. A. Gallant, & R. O. Dendy. (1995). Anomalous transport and particle acceleration at shocks. CERN Bulletin. 302. 6 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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