Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies
if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the
same subfield and year (this is the minimum needed to enter the top 1%, not the average
within it), or reaches the top citation threshold in at least one of its specific research
topics.
Evolutionary tracks and isochrones for low- and intermediate-mass stars: From 0.15 to 7 $M_{\odot}$, and from $Z=0.0004$ to 0.03
20001.7k citationsL. Girardi, A. Bressan et al.profile →
Theoretical isochrones in several photometric systems
2002775 citationsL. Girardi, G. Bertelli et al.Astronomy and Astrophysicsprofile →
Theoretical isochrones in several photometric systems I. Johnson-Cousins-Glass, HST/WFPC2, HST/NICMOS, Washington, and ESO Imaging Survey filter sets
2002663 citationsL. Girardi, G. Bertelli et al.profile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
hero ref
This map shows the geographic impact of C. Chiosi'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 C. Chiosi with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites C. Chiosi more than expected).
This network shows the impact of papers produced by C. Chiosi. 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 C. Chiosi. The network helps show where C. Chiosi may publish in the future.
Co-authorship network of co-authors of C. Chiosi
This figure shows the co-authorship network connecting the top 25 collaborators of C. Chiosi.
A scholar is included among the top collaborators of C. Chiosi 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 C. Chiosi. C. Chiosi is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Girardi, L., A. Bressan, G. Bertelli, & C. Chiosi. (2000). VizieR Online Data Catalog: Low-mass stars evolutionary tracks & isochrones (Girardi+, 2000).3 indexed citations
12.
Buson, L. M., F. Bertola, Michele Cappellari, et al.. (2000). Ultraviolet Imaging of the Galaxy Cluster CL 0939+4713 (Abell 851) at z=0.41*. The Astrophysical Journal. 531(2). 684–692.8 indexed citations
13.
Longhetti, M., A. Bressan, C. Chiosi, & R. Rampazzo. (2000). Star formation history of early-type galaxies in low density environments. IV. What do we learn from nuclear line-strength indices?. A&A. 353. 917–929.3 indexed citations
14.
Marigo, Paola, A. Bressan, & C. Chiosi. (1996). The formation of carbon stars: indication from TP-AGB analytical modelling.. MmSAI. 67. 713–728.1 indexed citations
15.
Bressan, A., et al.. (1994). Theoretical isochrones from models with new radiative opacities. Astronomy & Astrophysics Supplement Series. 106(2). 275–302.35 indexed citations
16.
Carraro, G., et al.. (1993). Two intermediate age open clusters: NGC 752 and NGC 3680.. Research Padua Archive (University of Padua). 101(2). 381–392.
17.
Bertelli, G., A. Bressan, C. Chiosi, et al.. (1993). Evolutionary sequences of stellar models with semiconvection and convective overshoot. I Z=0.008. Astronomy & Astrophysics Supplement Series. 97(4). 851–871.5 indexed citations
18.
Aparicio, A., et al.. (1991). CCD UBVR photometry of two old open clusters: King 11 and Be42. Comparison with theoretical models. Astronomy & Astrophysics Supplement Series. 88(1). 155–175.1 indexed citations
19.
Chiosi, C., Stanford E. Woosley, B. Hauck, et al.. (1986). Nucleosynthesis and chemical evolution : sixteenth advanced course of the Swiss Society of Astronomy and Astrophysics.21 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.