This map shows the geographic impact of L. Padrielli'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. Padrielli with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites L. Padrielli more than expected).
This network shows the impact of papers produced by L. Padrielli. 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. Padrielli. The network helps show where L. Padrielli may publish in the future.
Co-authorship network of co-authors of L. Padrielli
This figure shows the co-authorship network connecting the top 25 collaborators of L. Padrielli.
A scholar is included among the top collaborators of L. Padrielli 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. Padrielli. L. Padrielli is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Bortolotti, C., G. Grueff, A. Maccaferri, et al.. (1995). Detection of the 22-GHz line of water during and after the SL-9/Jupiter event.. 52. 261–266.3 indexed citations
4.
Bondi, M., et al.. (1994). One-year modulation in the flux density time series of low frequency variables.. A&A. 287. 390–402.
5.
Mantovani, F., W. Junor, R. Fanti, L. Padrielli, & D. J. Saikia. (1994). Gaseous cocoons around compact steep spectrum sources.. Bulletin of the Astronomical Society of India. 23. 534–66.
Padrielli, L., M. F. Aller, H. D. Aller, et al.. (1987). Multifrequency observations of low frequency variable sources: a statistical analysis. Astronomy & Astrophysics Supplement Series. 67(1). 63–86.
Marscher, Alan P., J. J. Broderick, N. Bartel, L. Padrielli, & J. D. Romney. (1985). 18 cm VLBI Observations of the Quasar NRAO 140 During and After a Low-Frequency Outburst. Bulletin of the American Astronomical Society. 17. 608.
11.
Fanti, C., R. Fanti, L. Feretti, et al.. (1983). WSRT radio observations at 1.4 GHz of 32 Abell clusters of distance class 3 and 4.. Leiden Repository (Leiden University). 51. 179–194.1 indexed citations
12.
Fanti, C., R. Fanti, L. Feretti, et al.. (1982). Radio and optical observations of 9 nearby Abell Clusters: A 262, A 347, A 569, A 779, A 1213, A 1228, A 2162, A 2666.. A&A. 105. 200–218.1 indexed citations
13.
Fanti, R., L. Padrielli, & M. Salvati. (1982). Variable Radio Sources. Symposium - International Astronomical Union. 97. 317–324.1 indexed citations
14.
Fanti, C., et al.. (1981). Low frequency variable sources 5 year monitoring program at 408 MHZ.. Astronomy & Astrophysics Supplement Series. 45. 61–78.4 indexed citations
15.
Padrielli, L., et al.. (1981). Compact and extended structure in B2 radio sources of intermediate strength. Leiden Repository (Leiden University). 46. 473–481.1 indexed citations
16.
Fanti, R., L. Feretti, G. Giovannini, & L. Padrielli. (1979). Radio spectral properties of B2 quasars.. 73. 40–45.
17.
Lari, C., et al.. (1975). Statistical properties of radio sources of intermediate strength. Leiden Repository (Leiden University). 40. 91–118.4 indexed citations
18.
Fanti, C., et al.. (1974). B2 catalogue of radio sources: fourth part. 18. 147–156.1 indexed citations
Fanti, C., E. Gandolfi, G. Grueff, et al.. (1970). A catalogue of 3235 radio sources at 408 MHz. Astronomy & Astrophysics Supplement Series. 1(3). 281.5 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.