This map shows the geographic impact of D. Alloin'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 D. Alloin with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites D. Alloin more than expected).
This network shows the impact of papers produced by D. Alloin. 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 D. Alloin. The network helps show where D. Alloin may publish in the future.
Co-authorship network of co-authors of D. Alloin
This figure shows the co-authorship network connecting the top 25 collaborators of D. Alloin.
A scholar is included among the top collaborators of D. Alloin 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 D. Alloin. D. Alloin is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Lidman, C. & D. Alloin. (2005). The Cool Universe: Observing Cosmic Dawn. ASPC. 344.18 indexed citations
6.
Alloin, D.. (2004). Physics of Active Galactic Nuclei at all Scales. Msngr. 115. 46–46.3 indexed citations
7.
Hau, G. K. T. & D. Alloin. (2003). Cosmology and Fundamental Physics. The Messenger. 114. 50–50.26 indexed citations
8.
Courbin, F., G. Letawe, Pierre Magain, et al.. (2002). Spectroscopy of quasar host galaxies at the VLT: stellar populations and dynamics down to the central kiloparsec. Open Repository and Bibliography (University of Liège).
9.
Alloin, D., B. Altieri, M. N. Bremer, et al.. (2001). The XMM large scale structure survey and its multi-λ follow-up. Explore Bristol Research. 105. 32–36.5 indexed citations
10.
Bonatto, C., E. Bica, M. G. Pastoriza, & D. Alloin. (2000). Star formation in distant starburst galaxies. Lume (Universidade Federal do Rio Grande do Sul). 355. 99–112.
11.
Barvainis, Richard, Philip R. Maloney, Robert Antonucci, & D. Alloin. (1996). New Molecular Observations and Modelling of the Cloverleaf Quasar. Bulletin of the American Astronomical Society. 189(4). 1302.
12.
Salamanca, I., et al.. (1994). Sources of uncertainty in the relative scaling of spectroscopic data. Astronomy & Astrophysics Supplement Series. 103(1). 121–128.
13.
Rigaut, François, M. Combes, C. Dougados, et al.. (1992). Astrophysical Results with COME-ON. European Southern Observatory Conference and Workshop Proceedings. 42. 479.1 indexed citations
14.
Schmidt, A. A., E. Bica, & D. Alloin. (1990). Disentangling age and metallicity effects in the blueish nuclear population of M 33, NGC 278 and NGC 404.. Monthly Notices of the Royal Astronomical Society. 243(4). 620–628.15 indexed citations
15.
Alloin, D. & E. Bica. (1990). New routes in the analysis of composite stellar populations. 21. 182–186.1 indexed citations
16.
Bica, E. & D. Alloin. (1986). A grid of star cluster properties for stellar population synthesis. Astronomy & Astrophysics Supplement Series. 66(2). 171–179.2 indexed citations
17.
Bica, E. & D. Alloin. (1986). A base of star clusters for stellar population synthesis.. Lume (Universidade Federal do Rio Grande do Sul). 162(1). 21–31.5 indexed citations
18.
Alloin, D., M. G. Edmunds, P. O. Lindblad, & B. E. J. Pagel. (1981). The mild abundance gradient of NGC 1365.. 101. 377–384.1 indexed citations
19.
Alloin, D. & G. Tenorio‐Tagle. (1979). Observational tests for H II region models - A 'champagne party'. The Messenger. 18. 12.1 indexed citations
20.
Alloin, D., et al.. (1975). On the Number of Planetary Nebulae in Our Galaxy. Bulletin of the American Astronomical Society. 7. 399.1 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.