S. Chaty

16.5k total citations · 1 hit paper
103 papers, 2.1k citations indexed

About

S. Chaty is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Computational Mechanics. According to data from OpenAlex, S. Chaty has authored 103 papers receiving a total of 2.1k indexed citations (citations by other indexed papers that have themselves been cited), including 99 papers in Astronomy and Astrophysics, 28 papers in Nuclear and High Energy Physics and 17 papers in Computational Mechanics. Recurrent topics in S. Chaty's work include Astrophysical Phenomena and Observations (91 papers), Pulsars and Gravitational Waves Research (53 papers) and Gamma-ray bursts and supernovae (48 papers). S. Chaty is often cited by papers focused on Astrophysical Phenomena and Observations (91 papers), Pulsars and Gravitational Waves Research (53 papers) and Gamma-ray bursts and supernovae (48 papers). S. Chaty collaborates with scholars based in France, United States and United Kingdom. S. Chaty's co-authors include Farid Rahoui, Juan Rodríguez, C. A. Haswell, C. R. Shrader, R. I. Hynes, Wei Cui, John A. Tomsick, P. Filliatre, M. Krämer and Philipp Podsiadlowski and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Astronomy and Astrophysics.

In The Last Decade

S. Chaty

99 papers receiving 2.0k citations

Hit Papers

Formation of Double Neutron Star Systems 2017 2026 2020 2023 2017 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
S. Chaty France 22 2.1k 720 211 153 118 103 2.1k
Victor Doroshenko Germany 25 1.9k 0.9× 480 0.7× 513 2.4× 112 0.7× 119 1.0× 147 2.0k
C. Ferrigno Switzerland 29 2.3k 1.1× 691 1.0× 566 2.7× 130 0.8× 146 1.2× 170 2.4k
Arash Bahramian United States 22 1.6k 0.8× 385 0.5× 301 1.4× 133 0.9× 54 0.5× 98 1.6k
G. Dubus France 33 2.8k 1.4× 1.3k 1.8× 299 1.4× 214 1.4× 56 0.5× 91 2.9k
Scott C. Noble United States 21 1.5k 0.7× 572 0.8× 102 0.5× 116 0.8× 55 0.5× 41 1.5k
I. R. Tuohy Australia 21 1.5k 0.7× 691 1.0× 169 0.8× 108 0.7× 100 0.8× 93 1.6k
A. P. Smale United States 23 1.6k 0.8× 314 0.4× 483 2.3× 195 1.3× 101 0.9× 110 1.7k
Sudip Bhattacharyya India 19 1.2k 0.6× 346 0.5× 368 1.7× 193 1.3× 42 0.4× 92 1.3k
R. D. Saxton Spain 25 1.8k 0.9× 646 0.9× 90 0.4× 75 0.5× 51 0.4× 88 1.9k
F. A. Córdova United States 19 1.3k 0.6× 360 0.5× 211 1.0× 76 0.5× 78 0.7× 55 1.3k

Countries citing papers authored by S. Chaty

Since Specialization
Citations

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

Fields of papers citing papers by S. Chaty

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of S. Chaty

This figure shows the co-authorship network connecting the top 25 collaborators of S. Chaty. A scholar is included among the top collaborators of S. Chaty 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 S. Chaty. S. Chaty 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.
García, Federico, et al.. (2021). Stellar wind structures in the eclipsing binary system IGR J18027–2016. Springer Link (Chiba Institute of Technology). 2 indexed citations
2.
Nowak, Michael A., A. Paizis, Gaurava K. Jaisawal, et al.. (2019). <i>Chandra</i>-HETGS Characterization of an Outflowing Wind in the Accreting Millisecond Pulsar IGR J17591–2342. Technical University of Denmark, DTU Orbit (Technical University of Denmark, DTU). 8 indexed citations
3.
Keivani, A., Kohta Murase, Μαρία Πετροπούλου, et al.. (2018). A Multimessenger Picture of the Flaring Blazar TXS 0506+056: Implications for High-energy Neutrino Emission and Cosmic-Ray Acceleration. The Astrophysical Journal. 864(1). 84–84. 167 indexed citations
4.
Coleiro, A. & S. Chaty. (2017). VLT/X-Shooter spectrum of the blazar TXS 0506+056 (located inside the IceCube-170922A error box). ATel. 10840. 1. 1 indexed citations
5.
Bozzo, E., V. Bhalerao, John A. Tomsick, et al.. (2016). Multi-wavelength observations of IGR J17544-2619 from quiescence to outburst. Springer Link (Chiba Institute of Technology). 2 indexed citations
6.
Romero, Gustavo E., et al.. (2016). Modeling the polarization of high-energy radiation from accreting black holes : A case study of XTE J1118+480. El Servicio de Difusión de la Creación Intelectual (National University of La Plata). 5 indexed citations
7.
Chernyakova, M., A. A. Abdo, A. Neronov, et al.. (2014). Multi-wavelength observations of the binary system PSR B1259-63/LS 2883 around the 2010-2011 periastron passage. arXiv (Cornell University). 43 indexed citations
8.
Wood, K. S., M. Chernyakova, A. A. Abdo, et al.. (2014). Multi-wavelength Observations of the Binary System PSR B1259-63/LS 2883 Around the 2010-2011 Periastron Passage. 223. 3 indexed citations
9.
Paizis, A., J. Wilms, S. Chaty, et al.. (2011). UNVEILING THE NATURE OF IGR J17177–3656 WITH X-RAY, NEAR-INFRARED, AND RADIO OBSERVATIONS. DSpace@MIT (Massachusetts Institute of Technology). 9 indexed citations
10.
Curran, P. A., et al.. (2011). A search for near infrared counterparts of three pulsar wind nebulae. Springer Link (Chiba Institute of Technology). 2 indexed citations
11.
Chaty, S., et al.. (2009). Infrared identification of IGR J09026-4812 as a Seyfert 1 galaxy. Springer Link (Chiba Institute of Technology). 9 indexed citations
12.
Rodríguez, Juan, et al.. (2009). Swift archival observations of the field around the new INTEGRAL source IGR J19294+1816. ATel. 1998. 1. 1 indexed citations
13.
Rahoui, Farid & S. Chaty. (2008). IGR J18483–0311: a new intermediate supergiant fast X-ray transient. Springer Link (Chiba Institute of Technology). 30 indexed citations
14.
Testa, V., N. Rea, R. Mignani, et al.. (2008). Adaptive optics, near-infrared observations of magnetars. Springer Link (Chiba Institute of Technology). 13 indexed citations
15.
Neronov, A., M. Cadolle Bel, S. E. Shaw, et al.. (2008). Bright flare of Cyg X-1 in hard X-ray band. The astronomer's telegram. 1533. 1.
16.
Chaty, S., et al.. (2007). Discovery of a likely-period of 185 days in AX J1749.1-2733. ATel. 1035. 1. 1 indexed citations
17.
Negueruela, I., David M. Smith, & S. Chaty. (2005). Optical counterpart to IGR J16465-4507. ATel. 429. 1. 2 indexed citations
18.
Negueruela, I., David M. Smith, & S. Chaty. (2005). HD 306414 and IGR J11215-5952. ATel. 470. 1. 2 indexed citations
19.
Cocco, G. Di, L. Foschini, P. Grandi, et al.. (2004). . UvA-DARE (University of Amsterdam). 5 indexed citations
20.
Türler, M., T. J.-L. Courvoisier, S. Chaty, & Y. Fuchs. (2004). Quasar jet emission model applied to the microquasar GRS 1915+105. Springer Link (Chiba Institute of Technology). 11 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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