C. Maceroni

1.1k total citations
43 papers, 427 citations indexed

About

C. Maceroni is a scholar working on Astronomy and Astrophysics, Instrumentation and Computational Mechanics. According to data from OpenAlex, C. Maceroni has authored 43 papers receiving a total of 427 indexed citations (citations by other indexed papers that have themselves been cited), including 36 papers in Astronomy and Astrophysics, 21 papers in Instrumentation and 5 papers in Computational Mechanics. Recurrent topics in C. Maceroni's work include Stellar, planetary, and galactic studies (34 papers), Astronomy and Astrophysical Research (21 papers) and Astro and Planetary Science (17 papers). C. Maceroni is often cited by papers focused on Stellar, planetary, and galactic studies (34 papers), Astronomy and Astrophysical Research (21 papers) and Astro and Planetary Science (17 papers). C. Maceroni collaborates with scholars based in Italy, Belgium and Spain. C. Maceroni's co-authors include J. Montalbán, K. Pavlovski, C. Aerts, L. Milano, G. Russo, M. Rainer, J. Southworth, D. Gandolfi, P. Degroote and F. D’Antona and has published in prestigious journals such as SHILAP Revista de lepidopterología, Monthly Notices of the Royal Astronomical Society and Astronomy and Astrophysics.

In The Last Decade

C. Maceroni

41 papers receiving 404 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
C. Maceroni Italy 11 417 184 40 14 13 43 427
S. Štefl Germany 14 533 1.3× 113 0.6× 24 0.6× 9 0.6× 16 1.2× 29 547
P. B. Etzel United States 10 443 1.1× 194 1.1× 33 0.8× 4 0.3× 12 0.9× 42 457
M. Grosso Argentina 12 565 1.4× 203 1.1× 40 1.0× 21 1.5× 13 1.0× 23 576
T. Szeifert Germany 12 436 1.0× 113 0.6× 30 0.8× 19 1.4× 11 0.8× 30 451
A. F. J. Moffat Canada 12 345 0.8× 87 0.5× 42 1.1× 12 0.9× 6 0.5× 34 355
A. M. Hubert France 14 792 1.9× 290 1.6× 87 2.2× 9 0.6× 15 1.2× 57 806
C. D. Scarfe Canada 9 345 0.8× 149 0.8× 53 1.3× 7 0.5× 9 0.7× 64 364
Kh. F. Khaliullin Russia 12 400 1.0× 124 0.7× 29 0.7× 11 0.8× 9 0.7× 40 412
F. Thévenin France 5 389 0.9× 188 1.0× 21 0.5× 25 1.8× 6 0.5× 7 402
V. P. Goranskij Russia 11 316 0.8× 65 0.4× 45 1.1× 24 1.7× 18 1.4× 58 327

Countries citing papers authored by C. Maceroni

Since Specialization
Citations

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

Fields of papers citing papers by C. Maceroni

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of C. Maceroni

This figure shows the co-authorship network connecting the top 25 collaborators of C. Maceroni. A scholar is included among the top collaborators of C. Maceroni 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 C. Maceroni. C. Maceroni 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.
Muraveva, T., G. Clementini, C. Maceroni, et al.. (2014). Eclipsing binary stars in the Large Magellanic Cloud: results from the EROS-2, OGLE and VMC surveys★. Monthly Notices of the Royal Astronomical Society. 443(1). 432–445. 15 indexed citations
2.
Maceroni, C., H. Lehmann, R. da Silva, et al.. (2014). KIC 3858884: a hybridδScuti pulsator in a highly eccentric eclipsing binary. Astronomy and Astrophysics. 563. A59–A59. 38 indexed citations
3.
Aerts, C., K. Pavlovski, C. Maceroni, et al.. (2013). KIC 11285625: A double-lined spectroscopic binary with aγDoradus pulsator discovered fromKeplerspace photometry. Astronomy and Astrophysics. 556. A56–A56. 37 indexed citations
4.
Maceroni, C., J. Montalbán, D. Gandolfi, K. Pavlovski, & M. Rainer. (2013). CoRoT 102918586: aγDoradus pulsator in a short-period eccentric eclipsing binary. Astronomy and Astrophysics. 552. A60–A60. 30 indexed citations
5.
Maceroni, C., D. Gandolfi, J. Montalbán, & C. Aerts. (2011). The Impact of CoRoT and Kepler on Eclipsing Binary Science. Proceedings of the International Astronomical Union. 7(S282). 41–46. 1 indexed citations
6.
Maceroni, C., J. Montalbán, Elisa Michel, et al.. (2009). HD 174884: a strongly eccentric, short-period early-type binary system discovered by CoRoT. Astronomy and Astrophysics. 508(3). 1375–1389. 45 indexed citations
7.
Vilhu, O. & C. Maceroni. (2006). Surface Imaging of Late-Type Contact Binaries II: Hα Emission in AE Phe and YY Eri. Proceedings of the International Astronomical Union. 2(S240). 719–723.
8.
D’Antona, F., D. Cardini, M. P. Di Mauro, et al.. (2005). 85 Peg A: what age for a low-metallicity solar-like star?. Monthly Notices of the Royal Astronomical Society. 363(3). 847–856. 11 indexed citations
9.
Maceroni, C., et al.. (2004). The shortest period M dwarf eclipsing system BW3 V38. Springer Link (Chiba Institute of Technology). 50 indexed citations
10.
Maceroni, C. & J. Montalbán. (2004). The shortest period M dwarf eclipsing system BW3 V38. Astronomy and Astrophysics. 426(2). 577–585. 36 indexed citations
11.
Maceroni, C., et al.. (2002). Lithium during the AGB evolution in young open clusters of the LargeMagellanic Cloud. Astronomy and Astrophysics. 395(1). 179–187. 4 indexed citations
12.
Clementini, G., M. Tosi, A. Bragaglia, R. Merighi, & C. Maceroni. (1995). New pulsational properties of eight 'anomalous' RR Lyrae variables. Monthly Notices of the Royal Astronomical Society. 275(4). 929–943. 4 indexed citations
13.
Maceroni, C., et al.. (1994). Surface imaging of late-type contact binaries I: AE Phoenicis and YY Eridani. 288. 529. 5 indexed citations
14.
Maceroni, C., et al.. (1991). The galactic cluster NGC 188 : W Ursae Majoris contact binaries as a clue to two separate burst of star formation. 248(2). 430–434. 3 indexed citations
15.
Maceroni, C., et al.. (1990). Magnetic cycles in solar-type single and close binary stars.. 237(2). 395–401. 1 indexed citations
16.
Maceroni, C.. (1986). Light-curve solution of contact binaries and the uniqueness of derived mass ratios: V523 Cas. 170(1). 43–47. 1 indexed citations
17.
Maceroni, C., L. Milano, & G. Russo. (1985). General properties of W Ursae Majoris systems. Monthly Notices of the Royal Astronomical Society. 217(4). 843–866. 15 indexed citations
18.
Russo, G., et al.. (1982). Determination of parameters of W UMa system. II : TW Cet, S Ant, U Peg, ER Ori.. Astronomy & Astrophysics Supplement Series. 47. 211–216. 3 indexed citations
19.
Maceroni, C., L. Milano, & G. Russo. (1982). Determination of parameters of W UMa systems. III : CC Com, YY Eri, V502 OPH and TY Pup.. Astronomy & Astrophysics Supplement Series. 49. 123–128. 1 indexed citations
20.
Maceroni, C., M. Salvati, & F. Pacini. (1974). On the expansion of supernova shells. Astrophysics and Space Science. 28(1). 205–212. 2 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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