This map shows the geographic impact of V. Mangano'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 V. Mangano with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites V. Mangano more than expected).
This network shows the impact of papers produced by V. Mangano. 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 V. Mangano. The network helps show where V. Mangano may publish in the future.
Co-authorship network of co-authors of V. Mangano
This figure shows the co-authorship network connecting the top 25 collaborators of V. Mangano.
A scholar is included among the top collaborators of V. Mangano 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 V. Mangano. V. Mangano is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Romano, P., V. Mangano, L. Ducci, et al.. (2013). From hours to years: Swift's revolutionary view of SFXTs .. MmSAI. 84. 602.1 indexed citations
4.
Chester, M. M., J. R. Cummings, N. Gehrels, et al.. (2013). GRB 130831A: Swift detection of a burst with an optical counterpart.. GRB Coordinates Network. 15139. 1.2 indexed citations
5.
Kennea, J. A., M. Linares, H. A. Krimm, et al.. (2013). MAXI J1828-249: Swift UV counterpart and XRT spectral fit. The astronomer's telegram. 5479. 1.1 indexed citations
6.
Romano, P., V. Mangano, S. Vercellone, et al.. (2012). Swift-X-Ray Telescope Monitoring of the Candidate Supergiant Fast X-ray Transient IGR J16418-4532. NASA STI Repository (National Aeronautics and Space Administration).12 indexed citations
7.
Kennea, J. A., E. A. Hoversten, M. H. Siegel, et al.. (2011). MAXI J1836-194: Swift localization and optical counterpart. ATel. 3613. 1.3 indexed citations
8.
Kennea, J. A., H. A. Krimm, V. Mangano, et al.. (2010). MAXI J1659-152: Swift localization and monitoring. ATel. 2877. 1.2 indexed citations
9.
Mangano, V., et al.. (2010). GRB 100119A: Swift detection of a burst.. GRB Coordinates Network. 10348. 1.3 indexed citations
10.
Sbarufatti, B. & V. Mangano. (2008). GRB 080710: Swift XRT position.. GRB Coordinates Network. 7195. 1.1 indexed citations
11.
Mangano, V., A. Parsons, T. Sakamoto, et al.. (2008). Swift Observation of GRB 080603B.. 144. 1–4.1 indexed citations
12.
Sidoli, L., P. Romano, V. Mangano, et al.. (2008). A new outburst from the Supergiant Fast X-ray Transient IGRJ17544-2619 caught by Swift. The astronomer's telegram. 1454. 1.1 indexed citations
13.
Sbarufatti, B., A. Parsons, T. Sakamoto, et al.. (2008). Swift Observation of GRB 080605.. 142. 1–4.1 indexed citations
14.
Romano, P., V. Mangano, S. Mereghetti, et al.. (2007). Bright Outburst from IGRJ11215-5952 observed with Swift/XRT at apastron. The astronomer's telegram. 1151. 1.1 indexed citations
15.
Mineo, T., V. Mangano, G. Cusumano, & B. Sbarufatti. (2006). GRB061025: Swift XRT position.. GRB Coordinates Network. 5753. 1.1 indexed citations
16.
Parola, V. La, V. Mangano, Bing Zhang, et al.. (2006). The short GRB 051210 observed by Swift. CERN Bulletin. 121(12). 1505–1506.1 indexed citations
17.
Angelini, L., S. D. Barthelmy, A. Cucchiara, et al.. (2005). GRB050904: Swift-BAT detection of a probable burst.. GCN. 3910. 1.1 indexed citations
Rea, N., G. L. Israel, V. Testa, et al.. (2004). Correlated X-ray and IR decaying flux from the Anomalous X-ray Pulsar XTE J1810-197. ATel. 284. 1.1 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.