This map shows the geographic impact of F. Paresce'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 F. Paresce with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites F. Paresce more than expected).
This network shows the impact of papers produced by F. Paresce. 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 F. Paresce. The network helps show where F. Paresce may publish in the future.
Co-authorship network of co-authors of F. Paresce
This figure shows the co-authorship network connecting the top 25 collaborators of F. Paresce.
A scholar is included among the top collaborators of F. Paresce 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 F. Paresce. F. Paresce 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.
Wittkowski, M., F. Paresce, O. Chesneau, et al.. (2005). Recent Astrophysical Results from the VLTI. Max Planck Institute for Plasma Physics. 119. 36–42.
Marchi, Guido De & F. Paresce. (1995). Low mass stars in globular clusters. II. The mass function of M15.. A&A. 304. 202.1 indexed citations
4.
Paresce, F., Mario Livio, W. Hack, & K. T. Korista. (1995). The structure and evolution of the Nova V1974 Cygni shell from HST observations.. 299. 823.3 indexed citations
5.
Bianchi, L., H. C. Ford, R. C. Bohlin, F. Paresce, & Guido De Marchi. (1995). HST imaging of the planetary nebula K 648 in M 15.. 301. 537.1 indexed citations
Prangé, R., G. E. Ballester, Walter M. Harris, et al.. (1994). Comparison of IUE and HST diagnostic of the Jovian aurorae. Open Repository and Bibliography (University of Liège). 26.2 indexed citations
10.
Petro, L., et al.. (1994). Improved Dark-Sky Restrictions for HST Observations. American Astronomical Society Meeting Abstracts. 185.
11.
Deharveng, J. M., R. Albrecht, C. Barbieri, et al.. (1994). The massive star content of the blue dwarf galaxy IZw 36 from Faint Object Camera observations. A&A. 288. 413–424.1 indexed citations
12.
Marchi, Guido De & F. Paresce. (1994). Faint blue stars in the core of NGC 6397. 281(1).2 indexed citations
Paresce, F., P. Sartoretti, V. Dols, & Jean‐Claude Gérard. (1992). High Resolution Near UV Observations of Jupiter's Satellite Io with HST. Open Repository and Bibliography (University of Liège).1 indexed citations
16.
Burgarella, D., et al.. (1992). R Aquarii : an attempt at a unified model.. 262(1). 83–96.1 indexed citations
Firmani, C., L. Gutiérrez, Elena Baraza, et al.. (1984). High dispersion spectrophotometry with the MEPSICRON photon counter. 134(2). 251–257.10 indexed citations
20.
Paresce, F.. (1977). Compact sources of EUV radiation. NASA Technical Reports Server (NASA). 3. 55–80.1 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.