E. Ambrosi

539 total citations
19 papers, 179 citations indexed

About

E. Ambrosi is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Biomedical Engineering. According to data from OpenAlex, E. Ambrosi has authored 19 papers receiving a total of 179 indexed citations (citations by other indexed papers that have themselves been cited), including 17 papers in Astronomy and Astrophysics, 4 papers in Nuclear and High Energy Physics and 4 papers in Biomedical Engineering. Recurrent topics in E. Ambrosi's work include Astrophysical Phenomena and Observations (14 papers), Pulsars and Gravitational Waves Research (6 papers) and Gamma-ray bursts and supernovae (4 papers). E. Ambrosi is often cited by papers focused on Astrophysical Phenomena and Observations (14 papers), Pulsars and Gravitational Waves Research (6 papers) and Gamma-ray bursts and supernovae (4 papers). E. Ambrosi collaborates with scholars based in Italy, United Kingdom and Spain. E. Ambrosi's co-authors include L. Zampieri, A. D’Aí, Fabio Pintore, C. Pinto, M. Del Santo, D. J. Walton, T. P. Roberts, Peter Kosec, Matthew Middleton and Roberto Soria and has published in prestigious journals such as Monthly Notices of the Royal Astronomical Society, Astronomy and Astrophysics and Annals of Surgical Oncology.

In The Last Decade

E. Ambrosi

16 papers receiving 168 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
E. Ambrosi Italy 9 148 49 22 22 19 19 179
Congzhan Liu China 7 101 0.7× 45 0.9× 17 0.8× 11 0.5× 9 0.5× 26 144
S Zhang China 9 78 0.5× 28 0.6× 20 0.9× 53 2.4× 1 0.1× 21 187
J. Y. Liao China 8 131 0.9× 54 1.1× 21 1.0× 17 0.8× 3 0.2× 37 175
Alicia Rouco Escorial Netherlands 8 205 1.4× 45 0.9× 60 2.7× 18 0.8× 4 0.2× 14 208
Ryota Tomaru Japan 11 231 1.6× 95 1.9× 24 1.1× 45 2.0× 3 0.2× 13 258
F. D’Amico Brazil 9 154 1.0× 84 1.7× 45 2.0× 17 0.8× 5 0.3× 35 210
Weimin Yuan China 7 93 0.6× 74 1.5× 6 0.3× 17 0.8× 7 0.4× 29 153
Nagomi Uchida Japan 7 55 0.4× 45 0.9× 5 0.2× 2 0.1× 20 1.1× 20 104
S. Yang Norway 7 103 0.7× 31 0.6× 27 1.2× 6 0.3× 20 1.1× 11 145
L. Moser Germany 11 294 2.0× 66 1.3× 12 0.5× 18 0.8× 2 0.1× 25 331

Countries citing papers authored by E. Ambrosi

Since Specialization
Citations

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

Fields of papers citing papers by E. Ambrosi

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of E. Ambrosi

This figure shows the co-authorship network connecting the top 25 collaborators of E. Ambrosi. A scholar is included among the top collaborators of E. Ambrosi 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 E. Ambrosi. E. Ambrosi is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

19 of 19 papers shown
1.
Sokolova-Lapa, E., A. D’Aí, E. Ambrosi, et al.. (2025). How the spin-phase variability of cyclotron lines shapes the pulsed fraction spectra: Insights from 4U 1538–52. Astronomy and Astrophysics. 700. A70–A70.
2.
Pintore, Fabio, C. Pinto, G. A. Rodríguez Castillo, et al.. (2025). A new pulsating neutron star in the ultraluminous X-ray source NGC 4559 X7?. Astronomy and Astrophysics. 695. A238–A238. 4 indexed citations
3.
D’Aí, A., C. Ferrigno, E. Ambrosi, et al.. (2025). Energy-resolved pulse profile changes in V 0332+53: Indications of wings in the cyclotron absorption line profile. Astronomy and Astrophysics. 694. A316–A316. 1 indexed citations
4.
Paiano, S., Fabio Pintore, T. D. Russell, et al.. (2025). Search for the multi-wavelength counterparts to extragalactic unassociated Fermi γ-ray sources. Astronomy and Astrophysics. 694. A176–A176. 1 indexed citations
5.
Parola, V. La, M. Capalbi, M. Perri, et al.. (2024). Tracking the long-term timing accuracy of the X-Ray Telescope on board the Neil Gehrels Swift Observatory. Astronomy and Astrophysics. 692. A234–A234.
6.
Ferrigno, C., A. D’Aí, & E. Ambrosi. (2023). Energy-resolved pulse profiles of accreting pulsars: Diagnostic tools for spectral features. Astronomy and Astrophysics. 677. A103–A103. 9 indexed citations
7.
Marino, A., T. D. Russell, M. Del Santo, et al.. (2023). The accretion/ejection link in the neutron star X-ray binary 4U 1820-30 I: a boundary layer-jet coupling?. Monthly Notices of the Royal Astronomical Society. 525(2). 2366–2379. 8 indexed citations
8.
Ambrosi, E., et al.. (2022). Disc precession to explain the superorbital modulation of LMC X-4: results from the Swift monitoring campaign. Monthly Notices of the Royal Astronomical Society. 512(3). 3422–3435. 3 indexed citations
9.
Sathyaprakash, Rajath, T. P. Roberts, Fabien Grisé, et al.. (2022). A multi-wavelength view of distinct accretion regimes in the pulsating ultraluminous X-ray source NGC 1313 X-2. Monthly Notices of the Royal Astronomical Society. 511(4). 5346–5362. 10 indexed citations
10.
Pinto, C., Fabio Pintore, E. Ambrosi, et al.. (2022). A transient ultraluminous X-ray source in NGC 55. Monthly Notices of the Royal Astronomical Society. 515(4). 4669–4674. 2 indexed citations
11.
Wolter, A., Fabio Pintore, C. Pinto, et al.. (2022). Investigating the nature of the ultraluminous X-ray sources in the galaxy NGC 925. Monthly Notices of the Royal Astronomical Society. 512(2). 1814–1828. 6 indexed citations
12.
Pintore, Fabio, S. Motta, C. Pinto, et al.. (2021). The rare X-ray flaring activity of the ultraluminous X-ray source NGC 4559 X7. Monthly Notices of the Royal Astronomical Society. 504(1). 551–564. 12 indexed citations
13.
Pinto, C., Roberto Soria, D. J. Walton, et al.. (2021). XMM-Newton campaign on the ultraluminous X-ray source NGC 247 ULX-1: outflows. Monthly Notices of the Royal Astronomical Society. 505(4). 5058–5074. 40 indexed citations
14.
Alston, William, C. Pinto, D. Barret, et al.. (2021). Quasi-periodic dipping in the ultraluminous X-ray source, NGC 247 ULX-1. Monthly Notices of the Royal Astronomical Society. 505(3). 3722–3729. 17 indexed citations
15.
D’Aí, A., C. Pinto, M. Del Santo, et al.. (2021). The Chameleon on the branches: spectral state transition and dips in NGC 247 ULX-1. Monthly Notices of the Royal Astronomical Society. 507(4). 5567–5579. 12 indexed citations
16.
Sakamoto, T., E. Ambrosi, S. D. Barthelmy, et al.. (2019). GRB 190719C: Swift-BAT refined analysis. GRB Coordinates Network. 25125. 1. 4 indexed citations
17.
Pintore, Fabio, A. Belfiore, G. Novara, et al.. (2018). A new ultraluminous X-ray source in the galaxy NGC 5907. Monthly Notices of the Royal Astronomical Society Letters. 477(1). L90–L95. 16 indexed citations
18.
Ambrosi, E. & L. Zampieri. (2018). Modelling optical emission of Ultra-luminous X-ray Sources accreting above the Eddington limit. Monthly Notices of the Royal Astronomical Society. 12 indexed citations
19.
Zanoni, Andrea, Giuseppe Verlato, Simone Giacopuzzi, et al.. (2016). ypN0: Does It Matter How You Get There? Nodal Downstaging in Esophageal Cancer. Annals of Surgical Oncology. 23(S5). 998–1004. 22 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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