M. Fabrizio

31.5k total citations
25 papers, 524 citations indexed

About

M. Fabrizio is a scholar working on Astronomy and Astrophysics, Instrumentation and Computational Mechanics. According to data from OpenAlex, M. Fabrizio has authored 25 papers receiving a total of 524 indexed citations (citations by other indexed papers that have themselves been cited), including 23 papers in Astronomy and Astrophysics, 13 papers in Instrumentation and 4 papers in Computational Mechanics. Recurrent topics in M. Fabrizio's work include Stellar, planetary, and galactic studies (23 papers), Astronomy and Astrophysical Research (13 papers) and Astrophysics and Star Formation Studies (9 papers). M. Fabrizio is often cited by papers focused on Stellar, planetary, and galactic studies (23 papers), Astronomy and Astrophysical Research (13 papers) and Astrophysics and Star Formation Studies (9 papers). M. Fabrizio collaborates with scholars based in Italy, France and Spain. M. Fabrizio's co-authors include S. Marinoni, G. Bono, P. M. Marrese, G. Altavilla, B. Lemasle, M. Romaniello, K. Genovali, F. Primas, R. Buonanno and Noriyuki Matsunaga 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

M. Fabrizio

24 papers receiving 492 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
M. Fabrizio Italy 15 508 240 39 34 15 25 524
C. E. Martínez-Vázquez Spain 15 520 1.0× 282 1.2× 26 0.7× 36 1.1× 17 1.1× 37 543
G. Tautvaišienė Lithuania 15 640 1.3× 292 1.2× 58 1.5× 28 0.8× 13 0.9× 56 668
H. E. Delgado Spain 3 531 1.0× 238 1.0× 19 0.5× 37 1.1× 10 0.7× 3 547
H. M. Tabernero Spain 14 459 0.9× 245 1.0× 39 1.0× 28 0.8× 16 1.1× 34 468
George C. Angelou Germany 14 530 1.0× 287 1.2× 36 0.9× 25 0.7× 14 0.9× 27 538
F. Jiménez-Esteban Spain 14 559 1.1× 270 1.1× 18 0.5× 45 1.3× 9 0.6× 36 586
G. Maciejewski Poland 13 567 1.1× 281 1.2× 33 0.8× 22 0.6× 9 0.6× 43 576
G. Guiglion Germany 12 464 0.9× 206 0.9× 39 1.0× 21 0.6× 12 0.8× 27 495
Hsiang-Chih Hwang United States 15 515 1.0× 176 0.7× 48 1.2× 15 0.4× 21 1.4× 33 542
P. Klagyivik Hungary 11 483 1.0× 178 0.7× 31 0.8× 43 1.3× 10 0.7× 30 494

Countries citing papers authored by M. Fabrizio

Since Specialization
Citations

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

Fields of papers citing papers by M. Fabrizio

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of M. Fabrizio

This figure shows the co-authorship network connecting the top 25 collaborators of M. Fabrizio. A scholar is included among the top collaborators of M. Fabrizio 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 M. Fabrizio. M. Fabrizio 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.
Marengo, M., C. E. Martínez-Vázquez, Brian Chaboyer, et al.. (2023). RR Lyrae Mid-infrared Period–Luminosity–Metallicity and Period–Wesenheit–Metallicity Relations Based on Gaia DR3 Parallaxes. The Astrophysical Journal. 945(1). 83–83. 9 indexed citations
2.
Marini, E., F. Dell’Agli, D. Kamath, et al.. (2023). The intense production of silicates during the final AGB phases of intermediate mass stars. Astronomy and Astrophysics. 670. A97–A97. 9 indexed citations
3.
Dall’Ora, M., G. Bono, P. B. Stetson, et al.. (2022). On the dwarf irregular galaxy NGC 6822. I. Young, intermediate, and old stellar populations. arXiv (Cornell University). 6 indexed citations
4.
Prudil, Z., Andreas Koch, B. Lemasle, et al.. (2022). Milky Way archaeology using RR Lyrae and type II Cepheids. Astronomy and Astrophysics. 664. A148–A148. 17 indexed citations
5.
Lemasle, B., V. V. Kovtyukh, Z. Prudil, et al.. (2022). Tracing the Milky Way warp and spiral arms with classical Cepheids. Astronomy and Astrophysics. 668. A40–A40. 29 indexed citations
6.
Chaboyer, Brian, M. Marengo, G. Bono, et al.. (2021). Metallicities from high-resolution spectra of 49 RR Lyrae variables. Monthly Notices of the Royal Astronomical Society. 503(4). 4719–4733. 15 indexed citations
7.
Braga, V. F., G. Bono, G. Fiorentino, et al.. (2020). Separation between RR Lyrae and type II Cepheids and their importance for a distance determination: the case of omega Cen. Astronomy and Astrophysics. 644. A95–A95. 19 indexed citations
8.
Bono, G., V. F. Braga, G. Fiorentino, et al.. (2020). Evolutionary and pulsation properties of Type II Cepheids. Springer Link (Chiba Institute of Technology). 16 indexed citations
9.
Marrese, P. M., S. Marinoni, M. Fabrizio, & G. Altavilla. (2018). Gaia Data Release 2. Astronomy and Astrophysics. 621. A144–A144. 75 indexed citations
10.
Marrese, P. M., S. Marinoni, M. Fabrizio, & G. Giuffrida. (2017). Gaia Data Release 1. Astronomy and Astrophysics. 607. A105–A105. 21 indexed citations
11.
Fabrizio, M., M. Nonino, G. Bono, et al.. (2015). The Carina Project. Astronomy and Astrophysics. 580. A18–A18. 22 indexed citations
12.
Coppola, Giuseppina, M. Marconi, P. B. Stetson, et al.. (2015). THE CARINA PROJECT. IX. ON HYDROGEN AND HELIUM BURNING VARIABLES. The Astrophysical Journal. 814(1). 71–71. 32 indexed citations
13.
Genovali, K., B. Lemasle, G. Bono, et al.. (2014). On the fine structure of the Cepheid metallicity gradient in the Galactic thin disk. Springer Link (Chiba Institute of Technology). 65 indexed citations
14.
Stetson, P. B., M. Marconi, G. Bono, et al.. (2014). The Carina Project. VI. The helium burning variable stars1. 17 indexed citations
15.
Fabrizio, M., Gabriella Raimondo, E. Brocato, et al.. (2014). A bag of tricks: Using proper motions of Galactic stars to identify the Hercules ultra-faint dwarf galaxy members. Astronomy and Astrophysics. 570. A61–A61. 5 indexed citations
16.
Calamida, A., G. Bono, E. P. Lagioia, et al.. (2014). Strömgren and near-infrared photometry of metal-rich bulge globular clusters. Astronomy and Astrophysics. 565. A8–A8. 9 indexed citations
17.
Genovali, K., B. Lemasle, G. Bono, et al.. (2013). On the metallicity distribution of classical Cepheids in the Galactic inner disk. Springer Link (Chiba Institute of Technology). 21 indexed citations
18.
Lemasle, B., P. François, K. Genovali, et al.. (2013). Galactic abundance gradients from Cepheids. Astronomy and Astrophysics. 558. A31–A31. 51 indexed citations
19.
Lemasle, B., P. François, K. Genovali, et al.. (2013). Galactic abundance gradients from Cepheids - α and heavy elements in the outer disk. UvA-DARE (University of Amsterdam). 558. 1–16. 31 indexed citations
20.
Fabrizio, M., M. Nonino, G. Bono, et al.. (2011). The Carina Project. IV. Radial Velocity Distribution1. Publications of the Astronomical Society of the Pacific. 123(902). 384–401. 14 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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