This map shows the geographic impact of G. Marconi'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 G. Marconi with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites G. Marconi more than expected).
This network shows the impact of papers produced by G. Marconi. 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 G. Marconi. The network helps show where G. Marconi may publish in the future.
Co-authorship network of co-authors of G. Marconi
This figure shows the co-authorship network connecting the top 25 collaborators of G. Marconi.
A scholar is included among the top collaborators of G. Marconi 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 G. Marconi. G. Marconi 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.
Mignani, R., R. Paladino, B. Rudak, et al.. (2017). The First Detection of a Pulsar with ALMA. The Astrophysical Journal Letters. 851(1). L10–L10.10 indexed citations
2.
Humphreys, E. M. L., A. D. Biggs, K. Immer, et al.. (2017). ALMA Band 5 Science Verification. The Messenger. 167. 7–10.1 indexed citations
3.
Momany, Y., S. Ortolani, E. V. Held, et al.. (2015). V, J, H and K imaging of the metal rich globular cluster NGC 6528 : reddening, metallicity, and distance based on cleaned colour-magnitude diagrams. Americanae (AECID Library).4 indexed citations
Monaco, L., S. Villanova, P. Bonifacio, et al.. (2011). Lithium and sodium in the globular cluster M4. A Main Sequence star with Li compatible with the cosmological value: nature or nurture?. arXiv (Cornell University).1 indexed citations
Giuffrida, G., L. Sbordone, S. Zaggia, et al.. (2010). A Wide-angle VIMOS Survey of the Sagittarius Dwarf Spheroidal Galaxy. Cineca Institutional Research Information System (Tor Vergata University). 141. 29–31.
10.
Israel, G. L., N. Rea, E. Rol, et al.. (2009). ESO-VLT discovery of the variable nIR counterpart to the AXP 1E1547.0-5408. UvA-DARE (University of Amsterdam). 1909. 1.3 indexed citations
Sbordone, L., P. Bonifacio, G. Marconi, & R. Buonanno. (2004). Chemical abundances in Terzan 7. MmSAI. 75. 396.1 indexed citations
16.
Gallart, Carme, R. Zinn, F. Pont, et al.. (2002). Using color-magnitude diagrams and spectroscopy to derive star formation histories: VLT observations of Fornax. The Messenger. 108. 16–20.1 indexed citations
Baade, D., T. R. Bedding, C. M. Carollo, et al.. (1993). Remote Observing with the NTT and EMMI/SUSI: a First Assessment. The Messenger. 72. 13–14.1 indexed citations
20.
Tosi, M., P. Focardi, L. Greggio, & G. Marconi. (1989). Star formation in dwarf irregular galaxies.. Msngr. 57. 57–60.2 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.