R. Middei

2.0k total citations
41 papers, 503 citations indexed

About

R. Middei is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Atomic and Molecular Physics, and Optics. According to data from OpenAlex, R. Middei has authored 41 papers receiving a total of 503 indexed citations (citations by other indexed papers that have themselves been cited), including 36 papers in Astronomy and Astrophysics, 20 papers in Nuclear and High Energy Physics and 2 papers in Atomic and Molecular Physics, and Optics. Recurrent topics in R. Middei's work include Astrophysical Phenomena and Observations (34 papers), Galaxies: Formation, Evolution, Phenomena (25 papers) and Astrophysics and Cosmic Phenomena (19 papers). R. Middei is often cited by papers focused on Astrophysical Phenomena and Observations (34 papers), Galaxies: Formation, Evolution, Phenomena (25 papers) and Astrophysics and Cosmic Phenomena (19 papers). R. Middei collaborates with scholars based in Italy, United States and France. R. Middei's co-authors include S. Bianchi, F. Vagnetti, F. Ursini, G. Matt, Andrea Marinucci, M. Paolillo, Pierre-Olivier Petrucci, A. Tortosa, F. La Franca and Roberto Serafinelli 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

R. Middei

37 papers receiving 444 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
R. Middei Italy 14 478 230 25 24 17 41 503
A. Tortosa Italy 13 469 1.0× 212 0.9× 16 0.6× 29 1.2× 23 1.4× 25 474
S. Paltani Switzerland 11 367 0.8× 165 0.7× 12 0.5× 24 1.0× 21 1.2× 18 380
E. Behar United Kingdom 12 349 0.7× 145 0.6× 22 0.9× 31 1.3× 14 0.8× 19 362
J. M. Gelbord United States 12 488 1.0× 270 1.2× 27 1.1× 27 1.1× 5 0.3× 47 508
F. Ursini Italy 19 804 1.7× 375 1.6× 22 0.9× 46 1.9× 57 3.4× 55 817
P. Pietrini Italy 7 315 0.7× 149 0.6× 18 0.7× 18 0.8× 8 0.5× 18 319
Ken Pounds United Kingdom 5 443 0.9× 245 1.1× 14 0.6× 21 0.9× 17 1.0× 14 460
Ž. Bošnjak France 13 564 1.2× 312 1.4× 21 0.8× 16 0.7× 9 0.5× 32 606
Mihoko Yukita United States 15 615 1.3× 215 0.9× 69 2.8× 19 0.8× 25 1.5× 25 630

Countries citing papers authored by R. Middei

Since Specialization
Citations

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

Fields of papers citing papers by R. Middei

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of R. Middei

This figure shows the co-authorship network connecting the top 25 collaborators of R. Middei. A scholar is included among the top collaborators of R. Middei 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 R. Middei. R. Middei 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.
2.
Antonelli, L. A., Francesco Tombesi, A. Lamastra, et al.. (2024). Unveiling the periodic variability patterns of the X-ray emission from the blazar PG 1553+113. Astronomy and Astrophysics. 686. A300–A300.
3.
Ursini, F., G. Matt, D. R. Ballantyne, et al.. (2024). The origin of the soft excess in the luminous quasar HE 1029-1401. Astronomy and Astrophysics. 688. A189–A189. 2 indexed citations
4.
Serafinelli, Roberto, Alessandra De Rosa, A. Tortosa, et al.. (2024). Investigating the interplay between the coronal properties and the hard X-ray variability of active galactic nuclei with NuSTAR. Astronomy and Astrophysics. 690. A145–A145. 8 indexed citations
5.
Laurenti, Marco, Francesco Tombesi, F. Vagnetti, et al.. (2024). Investigating the nuclear properties of highly accreting active galactic nuclei with XMM-Newton. Astronomy and Astrophysics. 689. A337–A337. 3 indexed citations
6.
Ballantyne, D. R., S. Bianchi, B. Czerny, et al.. (2024). Unveiling energy pathways in AGN accretion flows with the warm corona model for the soft excess. Monthly Notices of the Royal Astronomical Society. 530(2). 1603–1623. 16 indexed citations
7.
Jin, Chichuan, Elisabeta Lusso, M. J. Ward, Chris Done, & R. Middei. (2023). Wavelength dependences of the optical/UV and X-ray luminosity correlations of quasars. Monthly Notices of the Royal Astronomical Society. 527(1). 356–373. 9 indexed citations
8.
Middei, R., Pierre-Olivier Petrucci, S. Bianchi, et al.. (2023). Tracking the spectral properties of ESO 511-G030 across different epochs. Astronomy and Astrophysics. 672. A101–A101. 4 indexed citations
9.
Luminari, A., Andrea Marinucci, S. Bianchi, et al.. (2023). The Lively Accretion Disk in NGC 2992. III. Tentative Evidence of Rapid Ultrafast Outflow Variability. The Astrophysical Journal. 950(2). 160–160. 6 indexed citations
10.
Piconcelli, E., L. Zappacosta, Francesco Tombesi, et al.. (2022). X-ray spectroscopic survey of highly accreting AGN. Archivio istituzionale della ricerca (Alma Mater Studiorum Università di Bologna). 26 indexed citations
11.
Matzeu, G. A., Maggie Lieu, M. Costa, et al.. (2022). A new emulated Monte Carlo radiative transfer disc-wind model: X-Ray Accretion Disc-wind Emulator – xrade. Monthly Notices of the Royal Astronomical Society. 515(4). 6172–6190. 9 indexed citations
12.
Middei, R., G. A. Matzeu, S. Bianchi, et al.. (2021). X-ray emission of Seyfert 2 galaxy MCG-01-24-12. Springer Link (Chiba Institute of Technology). 5 indexed citations
13.
Luminari, A., et al.. (2021). Location and energetics of the ultra-fast outflow in PG 1448+273. Springer Link (Chiba Institute of Technology). 14 indexed citations
14.
Matzeu, G. A., E. Nardini, M. L. Parker, et al.. (2020). The first broad-band X-ray view of the narrow-line Seyfert 1 Ton S180. Monthly Notices of the Royal Astronomical Society. 497(2). 2352–2370. 19 indexed citations
15.
Bianchi, S., Robert Antonucci, A. Capetti, et al.. (2019). HST unveils a compact mildly relativistic broad-line region in the candidate true type 2 NGC 3147. Monthly Notices of the Royal Astronomical Society Letters. 488(1). L1–L5. 29 indexed citations
16.
Middei, R., S. Bianchi, Andrea Marinucci, et al.. (2019). Relations between phenomenological and physical parameters in the hot coronae of AGNs computed with the MoCA code. Astronomy and Astrophysics. 630. A131–A131. 26 indexed citations
17.
Mao, Junjie, M. Mehdipour, J. S. Kaastra, et al.. (2019). Photoionized emission and absorption features in the high-resolution X-ray spectra of NGC 3783. Astronomy and Astrophysics. 621. A99–A99. 26 indexed citations
18.
Branduardi‐Raymont, G., M. Mehdipour, K. L. Page, et al.. (2019). Multi-wavelength campaign on NGC 7469. Astronomy and Astrophysics. 633. A62–A62. 10 indexed citations
19.
Middei, R., S. Bianchi, M. Cappi, et al.. (2018). Multi-wavelength campaign on NCG 7469. Astronomy and Astrophysics. 615. A163–A163. 25 indexed citations
20.
Vagnetti, F., et al.. (2016). Ensemble X-ray variability of active galactic nuclei. Astronomy and Astrophysics. 593. A55–A55. 39 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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