This map shows the geographic impact of P. Benvenuti'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 P. Benvenuti with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites P. Benvenuti more than expected).
This network shows the impact of papers produced by P. Benvenuti. 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 P. Benvenuti. The network helps show where P. Benvenuti may publish in the future.
Co-authorship network of co-authors of P. Benvenuti
This figure shows the co-authorship network connecting the top 25 collaborators of P. Benvenuti.
A scholar is included among the top collaborators of P. Benvenuti 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 P. Benvenuti. P. Benvenuti 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.
Benvenuti, P., M. T. V. T. Lago, Maria Cunningham, et al.. (2018). IAU volume 14 issue S345 Cover and Front matter. Proceedings of the International Astronomical Union. 14(S345). f1–f19.2 indexed citations
2.
Montmerle, T., P. Benvenuti, J. H. Knapen, et al.. (2015). IAU volume 11 issue S317 Cover and Front matter. Proceedings of the International Astronomical Union. 11(S317). f1–f16.1 indexed citations
Benvenuti, P., et al.. (2003). Astrovirtel - a Precursor of the Virtual Observatory. 25.1 indexed citations
6.
Mulas, G., Giuliano Malloci, & P. Benvenuti. (2003). Testing the “strong” PAHs hypothesis. Astronomy and Astrophysics. 410(2). 639–648.21 indexed citations
7.
Malloci, Giuliano, G. Mulas, & P. Benvenuti. (2003). Testing the “strong” PAHs hypothesis. Astronomy and Astrophysics. 410(2). 623–637.21 indexed citations
8.
Genova, F., P. Benvenuti, R. J. Hanisch, et al.. (2002). International Collaboration for the Virtual Observatory. 200.1 indexed citations
9.
Pierfederici, F., et al.. (2001). ASTROVIRTEL: Accessing Astronomical Archives as Virtual Telescopes. Research Padua Archive (University of Padua). 238. 141.1 indexed citations
10.
Jenniskens, P., I. Porceddu, P. Benvenuti, & F.–X. Désert. (1996). DIFFUSE INTERSTELLAR BANDS : RESOLVED ROTATIONAL BAND STRUCTURE AT 5850 A. 313(2). 649–656.4 indexed citations
11.
Benvenuti, P.. (1995). ESO/ST-ECF Workshop on Calibrating and Understanding HST and ESO Instruments, Garching, Germany, 25-28 April 1995 : proceedings.
Fulle, M., F. Pasian, & P. Benvenuti. (1992). HST observations of the inner coma of Comet Levy 1990c. Annales Geophysicae. 10. 145–149.5 indexed citations
14.
Bennett, K., P. Benvenuti, V. Domingo, et al.. (1983). Report on the scientific satellites of the European Space Agency. NASA STI/Recon Technical Report N. 83. 32831.1 indexed citations
15.
Benvenuti, P.. (1982). An Atlas of UV Spectra of Supernovae. Research Padua Archive (University of Padua). 1046. 438.
16.
Perinotto, M., N. Panagia, & P. Benvenuti. (1980). Physical conditions and abundances of CNO elements in NGC 7027. Research Padua Archive (University of Padua). 85(49). 332–341.2 indexed citations
D’Odorico, S., M. A. Dopita, & P. Benvenuti. (1980). A catalogue of supernova remnant candidates in nearby galaxies.. Research Padua Archive (University of Padua). 40. 67–80.3 indexed citations
19.
Benvenuti, P., et al.. (1974). Spectroscopic Observations of Comet Kohoutek (1973f). NASA Technical Reports Server (NASA). 31. 121.12 indexed citations
20.
Bellettini, G., C. Bemporad, P.L. Braccini, P. Benvenuti, & L. Foà. (1966). A precision detector for high-energy neutral pions. Nuovo cimento della Società italiana di fisica. A, Nuclei, particles and fields. 44(4). 946–965.
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.