¶. Marchegiani

3.4k total citations
39 papers, 689 citations indexed

About

¶. Marchegiani is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Instrumentation. According to data from OpenAlex, ¶. Marchegiani has authored 39 papers receiving a total of 689 indexed citations (citations by other indexed papers that have themselves been cited), including 34 papers in Astronomy and Astrophysics, 33 papers in Nuclear and High Energy Physics and 4 papers in Instrumentation. Recurrent topics in ¶. Marchegiani's work include Astrophysics and Cosmic Phenomena (29 papers), Galaxies: Formation, Evolution, Phenomena (28 papers) and Dark Matter and Cosmic Phenomena (15 papers) ¶. Marchegiani is often cited by papers focused on Astrophysics and Cosmic Phenomena (29 papers), Galaxies: Formation, Evolution, Phenomena (28 papers) and Dark Matter and Cosmic Phenomena (15 papers) ¶. Marchegiani collaborates with scholars based in Italy, South Africa and United States ¶. Marchegiani's co-authors include S. Colafrancesco, P. Giommi, M. Perri, C. Leto, S. Piranomonte, A. Maselli, E. Massaro, S. Sclavi, G. C. Perola and Geoff Beck and has published in prestigious journals such as SHILAP Revista de lepidopterología, Scientific Reports and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

¶. Marchegiani

36 papers receiving 666 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
¶. Marchegiani Italy 13 638 581 25 11 8 39 689
L. Ostorero Italy 12 471 0.7× 420 0.7× 14 0.6× 10 0.9× 8 1.0× 27 501
Eileen T. Meyer United States 16 775 1.2× 647 1.1× 45 1.8× 5 0.5× 16 2.0× 55 819
J. Tammi Finland 11 477 0.7× 487 0.8× 14 0.6× 8 0.7× 13 1.6× 34 535
S. Piranomonte Italy 13 1.1k 1.8× 762 1.3× 52 2.1× 14 1.3× 7 0.9× 61 1.2k
Jan Hamann Germany 12 583 0.9× 599 1.0× 14 0.6× 6 0.5× 11 1.4× 20 766
Peter W. A. Roming United States 14 823 1.3× 276 0.5× 68 2.7× 12 1.1× 9 1.1× 42 839
Ritaban Chatterjee United States 11 623 1.0× 597 1.0× 8 0.3× 5 0.5× 14 1.8× 30 690
L. Costamante Italy 15 1.1k 1.7× 1.2k 2.1× 10 0.4× 5 0.5× 8 1.0× 38 1.2k
J. Dennett-Thorpe Netherlands 12 779 1.2× 647 1.1× 26 1.0× 4 0.4× 9 1.1× 18 798
D. M. Worrall United Kingdom 14 537 0.8× 379 0.7× 22 0.9× 8 0.7× 6 0.8× 23 552

Countries citing papers authored by ¶. Marchegiani

Since Specialization
Citations

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

Fields of papers citing papers by ¶. Marchegiani

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of ¶. Marchegiani

This figure shows the co-authorship network connecting the top 25 collaborators of ¶. Marchegiani. A scholar is included among the top collaborators of ¶. Marchegiani 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 ¶. Marchegiani. ¶. Marchegiani 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.
Vacca, V., F. Govoni, M. Murgia, et al.. (2024). Filaments in and between galaxy clusters at low and mid-frequency with the SKA. Astronomy and Astrophysics. 691. A334–A334. 2 indexed citations
2.
Marchegiani, ¶.. (2022). Sunyaev Zel’dovich effect in galaxy clusters cavities: Thermal or non-thermal origin?. SHILAP Revista de lepidopterología.
3.
Datta, Abhirup, S. Colafrancesco, ¶. Marchegiani, et al.. (2017). Relativistic inverse Compton scattering of photons from the early universe. Scientific Reports. 7(1). 16918–16918. 7 indexed citations
4.
Colafrancesco, S., et al.. (2016). Probing the physics and history of cosmic reionization with the Sunyaev-Zel’dovich effect. Springer Link (Chiba Institute of Technology). 2 indexed citations
5.
Massaro, E., A. Maselli, C. Leto, et al.. (2016). VizieR Online Data Catalog: The Roma BZCAT - 5th edition (Massaro+, 2015). 1 indexed citations
6.
Colafrancesco, S. & ¶. Marchegiani. (2014). Probing photon decay with the Sunyaev-Zel’dovich effect. Astronomy and Astrophysics. 562. L2–L2. 4 indexed citations
7.
Colafrancesco, S., ¶. Marchegiani, P. de Bernardis, & S. Masi. (2012). A multi-frequency study of the SZE in giant radio galaxies. Astronomy and Astrophysics. 550. A92–A92. 7 indexed citations
8.
Colafrancesco, S., Richard Lieu, ¶. Marchegiani, et al.. (2011). Dark matter interpretation of the origin of non-thermal phenomena in galaxy clusters. Springer Link (Chiba Institute of Technology). 4 indexed citations
9.
Colafrancesco, S. & ¶. Marchegiani. (2011). The energetics of giant radio galaxy lobes from inverse Compton\n scattering observations. Springer Link (Chiba Institute of Technology). 14 indexed citations
10.
Bernardis, P. de, S. Colafrancesco, G. D’Alessandro, et al.. (2011). Low-resolution spectroscopy of the Sunyaev-Zel’dovich effect and estimates of cluster parameters. Astronomy and Astrophysics. 538. A86–A86. 17 indexed citations
11.
Colafrancesco, S., ¶. Marchegiani, & R. Buonanno. (2011). Untangling the atmosphere of the Bullet cluster with Sunyaev-Zel’dovich effect observations. Astronomy and Astrophysics. 527. L1–L1. 16 indexed citations
12.
Colafrancesco, S., ¶. Marchegiani, & P. Giommi. (2010). Disentangling the gamma-ray emission of NGC 1275 and that of the Perseus cluster. Springer Link (Chiba Institute of Technology). 12 indexed citations
13.
Colafrancesco, S. & ¶. Marchegiani. (2010). On the ability of the spectroscopic Sunyaev-Zeldovich effect measurements to determine\nthe temperature structure of galaxy clusters. Springer Link (Chiba Institute of Technology). 11 indexed citations
14.
Colafrancesco, S. & ¶. Marchegiani. (2009). On the inverse Compton scattering interpretation of the hard X-ray excesses in galaxy clusters: the case of Ophiuchus. Springer Link (Chiba Institute of Technology). 12 indexed citations
15.
Massaro, E., P. Giommi, C. Leto, et al.. (2008). Roma-BZCAT: a multifrequency catalogue of blazars. Astronomy and Astrophysics. 495(2). 691–696. 203 indexed citations
16.
Colafrancesco, S. & ¶. Marchegiani. (2008). Warming rays in cluster cool cores. Astronomy and Astrophysics. 484(1). 51–65. 14 indexed citations
17.
Giommi, P., S. Colafrancesco, S. Cutini, et al.. (2008). AGILE and Swift simultaneous observations of the blazar S50716+714 during the bright flare of October 2007. Astronomy and Astrophysics. 487(3). L49–L52. 11 indexed citations
18.
Marchegiani, ¶., G. C. Perola, & S. Colafrancesco. (2007). Testing the cosmic ray content in galaxy clusters. Astronomy and Astrophysics. 465(1). 41–49. 10 indexed citations
19.
Colafrancesco, S., ¶. Marchegiani, & G. C. Perola. (2005). Where does the hard X-ray diffuse emission in clusters of galaxies come from?. Astronomy and Astrophysics. 443(1). 1–10. 16 indexed citations
20.
Colafrancesco, S., et al.. (2002). The non-thermal Sunyaev–Zel'dovich effect in clusters of galaxies. Springer Link (Chiba Institute of Technology). 44 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.

Explore authors with similar magnitude of impact

Breakdown of academic impact, for papers by L. Ostorero Breakdown of academic impact, for papers by Eileen T. Meyer Breakdown of academic impact, for papers by J. Tammi Breakdown of academic impact, for papers by S. Piranomonte Breakdown of academic impact, for papers by Jan Hamann Breakdown of academic impact, for papers by Peter W. A. Roming Breakdown of academic impact, for papers by Ritaban Chatterjee Breakdown of academic impact, for papers by L. Costamante Breakdown of academic impact, for papers by J. Dennett-Thorpe Breakdown of academic impact, for papers by D. M. Worrall
Rankless by CCL
2026