F. Acero

8.1k total citations
41 papers, 556 citations indexed

About

F. Acero is a scholar working on Nuclear and High Energy Physics, Astronomy and Astrophysics and Computer Vision and Pattern Recognition. According to data from OpenAlex, F. Acero has authored 41 papers receiving a total of 556 indexed citations (citations by other indexed papers that have themselves been cited), including 38 papers in Nuclear and High Energy Physics, 37 papers in Astronomy and Astrophysics and 3 papers in Computer Vision and Pattern Recognition. Recurrent topics in F. Acero's work include Astrophysics and Cosmic Phenomena (37 papers), Gamma-ray bursts and supernovae (30 papers) and Astrophysical Phenomena and Observations (13 papers). F. Acero is often cited by papers focused on Astrophysics and Cosmic Phenomena (37 papers), Gamma-ray bursts and supernovae (30 papers) and Astrophysical Phenomena and Observations (13 papers). F. Acero collaborates with scholars based in France, United States and Japan. F. Acero's co-authors include M. Ackermann, J. Ballet, A. Decourchelle, M. Lemoine‐Goumard, R. Lallement, V. Kharchenko, Dimitra Koutroumpa, M. Renaud, G. Dubner and B. Condon and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and IEEE Transactions on Image Processing.

In The Last Decade

F. Acero

36 papers receiving 540 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
F. Acero France 13 498 477 7 7 7 41 556
D. Bastieri Italy 10 280 0.6× 315 0.7× 5 0.7× 13 1.9× 8 1.1× 61 345
Nayantara Gupta India 12 332 0.7× 416 0.9× 6 0.9× 2 0.3× 2 0.3× 52 462
Gwenael Giacinti Germany 13 511 1.0× 650 1.4× 2 0.3× 2 0.3× 4 0.6× 52 688
Romain Hascoët France 11 450 0.9× 194 0.4× 4 0.6× 4 0.6× 4 0.6× 18 453
D. Svinkin Russia 11 374 0.8× 134 0.3× 5 0.7× 9 1.3× 4 0.6× 47 385
F. D’Ammando Italy 18 826 1.7× 781 1.6× 10 1.4× 2 0.3× 12 1.7× 89 859
C. Casadio Spain 10 411 0.8× 407 0.9× 7 1.0× 15 2.1× 27 437
S. Kiehlmann United States 10 304 0.6× 290 0.6× 7 1.0× 1 0.1× 12 1.7× 32 343
Jun Fang China 12 422 0.8× 408 0.9× 9 1.3× 8 1.1× 56 458
I. S. Troitsky Russia 6 256 0.5× 269 0.6× 7 1.0× 15 2.1× 13 287

Countries citing papers authored by F. Acero

Since Specialization
Citations

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

Fields of papers citing papers by F. Acero

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of F. Acero

This figure shows the co-authorship network connecting the top 25 collaborators of F. Acero. A scholar is included among the top collaborators of F. Acero 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 F. Acero. F. Acero 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.
Bobin, J., et al.. (2025). Best of both worlds: Fusing hyperspectral data from two generations of spectro-imagers for X-ray astrophysics. Astronomy and Astrophysics. 694. A34–A34.
2.
Zhang, Shuo, T. Ergin, Naomi Tsuji, et al.. (2025). Discovery of a Pulsar Wind Nebula Candidate Associated with the Galactic PeVatron 1LHAASO J0343+5254u. The Astrophysical Journal. 983(1). 21–21. 1 indexed citations
3.
Lemoine-Goumard, M., et al.. (2024). Hadronic particle acceleration in the supernova remnant SN 1006 as traced by Fermi-LAT observations. Astronomy and Astrophysics. 693. A193–A193.
4.
Acero, F., et al.. (2024). Bayesian insights into the Tycho supernova remnant: A detailed mapping of ejecta properties. Astronomy and Astrophysics. 693. A234–A234. 2 indexed citations
5.
Bobin, J., et al.. (2024). SUSHI: An algorithm for source separation of hyperspectral images with non-stationary spectral variation. Astronomy and Astrophysics. 686. A259–A259. 1 indexed citations
6.
Williams, Brian J., et al.. (2024). Mapping thermal emission in the synchrotron-dominated supernova remnants G330.2+1.0, 3C58, and RX J1713.7-3946. Astronomy and Astrophysics. 683. A197–A197. 1 indexed citations
7.
Rosillo, M. Nievas, F. Acero, M. Vázquez Acosta, et al.. (2024). Unified multiwavelength data analysis workflow with gammapy. Astronomy and Astrophysics. 693. A287–A287.
8.
Williams, Brian J., et al.. (2023). The X-ray synchrotron rims in Cassiopeia A narrow with energy. Astronomy and Astrophysics. 672. A57–A57. 5 indexed citations
9.
Castro, Daniel, Joseph D. Gelfand, M. Kerr, et al.. (2023). Fermi-LAT Gamma-Ray Emission Discovered from the Composite Supernova Remnant B0453-685 in the Large Magellanic Cloud. The Astrophysical Journal. 945(1). 4–4. 3 indexed citations
10.
Tutone, Antonio, J. Ballet, F. Acero, A. D’Aí, & G. Cusumano. (2021). Multiple accelerated particle populations in the Cygnus Loop with Fermi-LAT. Astronomy and Astrophysics. 656. A139–A139. 9 indexed citations
11.
Li, Jiangtao, J. Ballet, M. Miceli, et al.. (2018). Spatially Resolved Broadband Synchrotron Emission from the Nonthermal Limbs of SN1006. The Astrophysical Journal. 864(1). 85–85. 13 indexed citations
12.
Devin, J., F. Acero, J. Ballet, & Julia Schmid. (2018). Disentangling hadronic from leptonic emission in the composite SNR G326.3−1.8. Astronomy and Astrophysics. 617. A5–A5. 4 indexed citations
13.
Acero, F., Satoru Katsuda, J. Ballet, & Robert Petre. (2016). Measurement of the X-ray proper motion in the south-east rim of RX J1713.7−3946. Astronomy and Astrophysics. 597. A106–A106. 10 indexed citations
14.
Katsuda, Satoru, F. Acero, Nozomu Tominaga, et al.. (2015). EVIDENCE FOR THERMAL X-RAY LINE EMISSION FROM THE SYNCHROTRON-DOMINATED SUPERNOVA REMNANT RX J1713.7-3946. The Astrophysical Journal. 814(1). 29–29. 22 indexed citations
15.
Miceli, M., F. Acero, G. Dubner, et al.. (2014). Shock-Cloud Interaction and Particle Acceleration in the Southwestern Limb of SN 1006. CONICET Digital (CONICET). 21 indexed citations
16.
Sushch, I., S. Ohm, R. Terrier, et al.. (2011). An Extended X-ray PWN Counterpart to the VHE Gamma-ray Source HESS J1303-631. 57.
17.
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
18.
Kosack, K., R. C. G. Chaves, & F. Acero. (2011). HESS J1852-000: A Very High Energy Gamma-ray source near Supernova Remnant Kes~78. International Cosmic Ray Conference. 7. 76–78.
19.
Acero, F., J. Ballet, A. Decourchelle, et al.. (2008). A joint spectro-imaging analysis of the XMM-Newton and HESS observations of the supernova remnant RX J1713.7-3946. Conicet. 43 indexed citations
20.
Koutroumpa, Dimitra, F. Acero, R. Lallement, J. Ballet, & V. Kharchenko. (2007). OVII and OVIII line emission in the diffuse soft X-ray background: heliospheric and galactic contributions. Springer Link (Chiba Institute of Technology). 58 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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