This map shows the geographic impact of L. Monaco'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 L. Monaco with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites L. Monaco more than expected).
This network shows the impact of papers produced by L. Monaco. 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 L. Monaco. The network helps show where L. Monaco may publish in the future.
Co-authorship network of co-authors of L. Monaco
This figure shows the co-authorship network connecting the top 25 collaborators of L. Monaco.
A scholar is included among the top collaborators of L. Monaco 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 L. Monaco. L. Monaco 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.
Andrade, Acácio A., et al.. (2024). The galaxy cluster AC114. Astronomy and Astrophysics. 686. A81–A81.1 indexed citations
2.
Bonifacio, P., E. Caffau, L. Monaco, et al.. (2024). High-speed stars. Astronomy and Astrophysics. 684. A91–A91.5 indexed citations
Bonifacio, P., L. Monaco, Stefania Salvadori, et al.. (2021). TOPoS. Astronomy and Astrophysics. 651. A79–A79.33 indexed citations
7.
Boffin, H. M. J., David Jones, R. Wesson, et al.. (2018). When nature tries to trick us An eclipsing eccentric close binary superposed on the central star of the planetary nebula M 3-2. UCL Discovery (University College London).5 indexed citations
8.
Molaro, P., L. Monaco, M. Barbieri, S. Zaggia, & C. Lovis. (2015). Simultaneous HARPS and HARPS-N Observations of the Earth Transit of 2014 as Seen from Jupiter: Detection of an Inverse Rossiter-McLaughlin Effect. Msngr. 161. 20–23.1 indexed citations
Gilmore, G., S. E. Koposov, John E. Norris, et al.. (2013). Boötes-I, Segue 1, the Orphan Stream and CEMP-no Stars: Extreme Systems Quantifying Feedback and Chemical Evolution in the Oldest and Smallest Galaxies. Msngr. 151. 25–28.1 indexed citations
13.
Molaro, P., L. Monaco, M. Barbieri, & S. Zaggia. (2013). HARPS Observations of the 2012 Transit of Venus. The Messenger. 153. 22–24.1 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
Monaco, L., P. Bonifacio, L. Sbordone, S. Villanova, & E. Pancino. (2010). The lithium content of ω Centauri - new clues to the cosmological Li problem from old stars in external galaxies. MPG.PuRe (Max Planck Society).21 indexed citations
18.
Saviane, I., V. Piirola, S. Bagnulo, et al.. (2007). Circular Polarimetry Now Offered at EFOSC2. Open Repository and Bibliography (University of Liège). 129. 14–17.2 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.