G. Bélanger

2.1k total citations
39 papers, 959 citations indexed

About

G. Bélanger is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Geophysics. According to data from OpenAlex, G. Bélanger has authored 39 papers receiving a total of 959 indexed citations (citations by other indexed papers that have themselves been cited), including 31 papers in Astronomy and Astrophysics, 18 papers in Nuclear and High Energy Physics and 5 papers in Geophysics. Recurrent topics in G. Bélanger's work include Astrophysical Phenomena and Observations (29 papers), Pulsars and Gravitational Waves Research (17 papers) and Astrophysics and Cosmic Phenomena (13 papers). G. Bélanger is often cited by papers focused on Astrophysical Phenomena and Observations (29 papers), Pulsars and Gravitational Waves Research (17 papers) and Astrophysics and Cosmic Phenomena (13 papers). G. Bélanger collaborates with scholars based in France, Spain and United Kingdom. G. Bélanger's co-authors include Sabine Kraml, Béranger Dumont, John F. Gunion, Ulrich Ellwanger, A. Goldwurm, Fulvio Melia, R. Terrier, G. Trap, A. Goldwurm and P. Ferrando 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. Bélanger

35 papers receiving 938 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. Bélanger France 17 820 532 113 82 35 39 959
V. Beckmann Switzerland 21 1.2k 1.4× 631 1.2× 64 0.6× 38 0.5× 26 0.7× 104 1.2k
Robert F. Penna United States 17 1.3k 1.6× 712 1.3× 103 0.9× 96 1.2× 36 1.0× 34 1.3k
Chichuan Jin China 20 1.2k 1.5× 474 0.9× 29 0.3× 69 0.8× 38 1.1× 62 1.3k
Hotaka Shiokawa United States 11 993 1.2× 509 1.0× 49 0.4× 49 0.6× 33 0.9× 13 1.0k
A. Goldwurm France 17 818 1.0× 402 0.8× 104 0.9× 82 1.0× 43 1.2× 46 858
K. Dodds-Eden Germany 12 1.2k 1.4× 311 0.6× 78 0.7× 90 1.1× 81 2.3× 15 1.2k
M. R. Garcia United States 20 1.4k 1.7× 410 0.8× 180 1.6× 177 2.2× 28 0.8× 66 1.4k
L. Heil Netherlands 13 628 0.8× 209 0.4× 109 1.0× 89 1.1× 31 0.9× 13 655
Ziri Younsi United Kingdom 20 1.3k 1.6× 912 1.7× 57 0.5× 30 0.4× 35 1.0× 37 1.4k
D. J. K. Buisson United Kingdom 17 885 1.1× 353 0.7× 76 0.7× 136 1.7× 20 0.6× 51 907

Countries citing papers authored by G. Bélanger

Since Specialization
Citations

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

Fields of papers citing papers by G. Bélanger

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

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

This figure shows the co-authorship network connecting the top 25 collaborators of G. Bélanger. A scholar is included among the top collaborators of G. Bélanger 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. Bélanger. G. Bélanger 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.
Ferrigno, C., E. Kuulkers, V. Savchenko, et al.. (2018). INTEGRAL hard X-ray spectroscopy of AT2018cow: preliminary detection of a cutoff at 40 keV.. ATel. 11788. 1.
2.
Savchenko, V., C. Ferrigno, E. Kuulkers, et al.. (2018). INTEGRAL observations of decaying hard X-ray emission from AT2018cow. The astronomer's telegram. 11843. 1.
3.
Ferrigno, C., et al.. (2015). ANTARES neutrino detection: INTEGRAL upper limit on the hard X-ray counterpart. ATel. 7995. 1.
4.
Ponti, G., M. Morris, R. Terrier, et al.. (2015). TheXMM–Newtonview of the central degrees of the Milky Way. Monthly Notices of the Royal Astronomical Society. 453(1). 172–213. 61 indexed citations
5.
Bélanger, G.. (2013). ON DETECTING TRANSIENT PHENOMENA. The Astrophysical Journal. 773(1). 66–66. 7 indexed citations
6.
Trap, G., A. Goldwurm, K. Dodds-Eden, et al.. (2011). Concurrent X-ray, near-infrared, sub-millimeter, and GeV gamma-ray observations of Sagittarius A*. Springer Link (Chiba Institute of Technology). 31 indexed citations
7.
Nucita, Achille, B. Maiolo, S. Carpano, et al.. (2009). The X-ray eclipse of the dwarf nova HT Cassiopeiae observed by theXMM-Newton satellite: spectral and timing analysis. Astronomy and Astrophysics. 504(3). 973–979. 16 indexed citations
8.
9.
Porquet, D., N. Grosso, P. Predehl, et al.. (2008). X-ray hiccups from Sagittarius A* observed by XMM-Newton. Astronomy and Astrophysics. 488(2). 549–557. 78 indexed citations
10.
Meyer, L., Tuan Do, A. M. Ghez, et al.. (2008). A 600 Minute Near-Infrared Light Curve of Sagittarius A*. The Astrophysical Journal. 688(1). L17–L20. 36 indexed citations
11.
Beckmann, V., S. Soldi, G. Bélanger, et al.. (2007). Cygnus X-3 transition from the ultrasoft to the hard state. Springer Link (Chiba Institute of Technology). 5 indexed citations
12.
Falanga, M., S. Soldi, S. E. Shaw, et al.. (2007). INTEGRAL IBIS/ISGRI hard X-ray detection of the accreting millisecond pulsar XTE J1751-305. ATel. 1046. 1.
13.
Cesare, G. De, R. Walter, A. Bodaghee, et al.. (2006). IGR J17252-3616: an accreting pulsar observed byINTEGRAL andXMM-Newton. Astronomy and Astrophysics. 448(1). 261–270. 22 indexed citations
14.
Yusef‐Zadeh, F., H. Bushouse, C. D. Dowell, et al.. (2006). A Multiwavelength Study of Sgr A*: The Role of Near‐IR Flares in Production of X‐Ray, Soft γ‐Ray, and Submillimeter Emission. The Astrophysical Journal. 644(1). 198–213. 88 indexed citations
15.
Hill, A. B., R. Walter, C. Knigge, et al.. (2005). The 1–50 keV spectral and timing analysis of IGR J18027-2016: an eclipsing, high mass X-ray binary. Astronomy and Astrophysics. 439(1). 255–263. 30 indexed citations
16.
Bassani, L., A. Malizia, J. B. Stephen, et al.. (2004). 17 New Identified INTEGRAL Sources. ATel. 232. 1. 1 indexed citations
17.
Lebrun, F., R. Terrier, A. Bazzano, et al.. (2004). Compact sources as the origin of the soft γ-ray emission of the Milky Way. Nature. 428(6980). 293–296. 32 indexed citations
18.
Terrier, R., F. Lebrun, A. Bazzano, et al.. (2003). In-flight calibration of the ISGRI camera. Springer Link (Chiba Institute of Technology). 19 indexed citations
19.
Rodríguez, Juan, M. Del Santo, F. Lebrun, et al.. (2003). First results from the IBIS/ISGRI data obtained during the Galactic Plane Scan. Astronomy and Astrophysics. 411(1). L373–L376. 5 indexed citations
20.
Bélanger, G., et al.. (1978). Traumatic central retinal vein occlusion.. Munich Personal RePEc Archive (Ludwig Maximilian University of Munich). 10(5). 587–91. 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.

Explore authors with similar magnitude of impact

Rankless by CCL
2026