This map shows the geographic impact of A. Milani'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 A. Milani with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites A. Milani more than expected).
This network shows the impact of papers produced by A. Milani. 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 A. Milani. The network helps show where A. Milani may publish in the future.
Co-authorship network of co-authors of A. Milani
This figure shows the co-authorship network connecting the top 25 collaborators of A. Milani.
A scholar is included among the top collaborators of A. Milani 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 A. Milani. A. Milani is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Schettino, Giulia, et al.. (2016). The radio science experiment with BepiColombo mission to Mercury .. Research Padua Archive (University of Padua). 87(1). 24–29.4 indexed citations
5.
Munari, U., et al.. (2013). After a post-maximum plateau Nova Del 2013 has begun a normal decline. The astronomer's telegram. 5304. 1.1 indexed citations
6.
Munari, U., et al.. (2013). Spectroscopy of the very fast Nova Del 2013, already declining past maximum brightness. ATel. 5297. 1.1 indexed citations
7.
Chesley, Steven R., M. C. Nolan, Davide Farnocchia, et al.. (2012). The Trajectory Dynamics of Near-Earth Asteroid 101955 (1999 RQ36). 1667. 6470.4 indexed citations
Munari, U., A. Milani, P. Valisa, & E. Semkov. (2010). Spectroscopic confirmation of HBC 722 as a new FU Orionis star in NGC 7000. ATel. 2808. 1.5 indexed citations
11.
Valsecchi, G. B., A. Milani, A. Rossi, & Giacomo Tommei. (2006). The SRT, Near-Earth objects, and space debris. 10. 186–191.3 indexed citations
12.
Milani, A., et al.. (2000). Direct solar radiation pressure on the orbits of small near-Earth asteroids: observable effects?. A&A. 362. 746–755.15 indexed citations
13.
Chesley, Steven R. & A. Milani. (2000). An Automatic Earth-Asteroid Collision Monitoring System. 31.5 indexed citations
14.
Chesley, Steven R. & A. Milani. (1999). NEODyS: an online information system for near-Earth objects. DPS. 31(4). 1117–106.1 indexed citations
15.
Knežević, Zoran & A. Milani. (1995). An analytical perturbation theory for the low lunar polar orbiter.. 49. 19–39.3 indexed citations
16.
Knežević, Zoran & A. Milani. (1992). Proper Elements for 20, 000 Asteroids. 24.1 indexed citations
17.
Zappalà, V., A. Cellino, P. Farinella, & A. Milani. (1992). Asteroid Families: Extension to Unnumbered Multi-Opposition Asteroids. 24.9 indexed citations
18.
Milani, A.. (1992). Proper Elements for Trojan Asteroids. 24.1 indexed citations
19.
Barlier, F., M. Carpino, P. Farinella, et al.. (1986). Non-gravitational perturbations on the semimajor axis of LAGEOS.. Annales Geophysicae. 4. 193–210.24 indexed citations
20.
Anselmo, Luciano, P. Farinella, A. Milani, & A. M. Nobili. (1981). Modelling of orbital perturbations due to radiation pressure for high earth satellites.. ESASP. 160. 47–52.1 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.