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.
Grids of stellar models with rotation
20111.1k citationsSylvia Ekström, C. Georgy et al.Astronomy and Astrophysicsprofile →
This map shows the geographic impact of A. Granada'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 A. Granada with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites A. Granada more than expected).
This network shows the impact of papers produced by A. Granada. 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 A. Granada. The network helps show where A. Granada may publish in the future.
Co-authorship network of co-authors of A. Granada
This figure shows the co-authorship network connecting the top 25 collaborators of A. Granada.
A scholar is included among the top collaborators of A. Granada 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 A. Granada. A. Granada is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Ekström, Sylvia, G. Meynet, C. Georgy, & A. Granada. (2018). Stellar rotation and its importance in the interpretation of stellar populations in MCs. Memorie della Societa Astronomica Italiana. 89. 50.1 indexed citations
8.
Jones, C. E., et al.. (2017). Omega -slow solutions and Be star disks. Americanae (AECID Library).8 indexed citations
Georgy, C., Sylvia Ekström, A. Granada, et al.. (2013). Populations of rotating stars. Astronomy and Astrophysics. 553. A24–A24.192 indexed citations
13.
Granada, A., Sylvia Ekström, C. Georgy, et al.. (2013). Populations of rotating stars. Astronomy and Astrophysics. 553. A25–A25.65 indexed citations
14.
Georgy, C., Sylvia Ekström, P. Eggenberger, et al.. (2013). Grids of stellar models with rotation. Astronomy and Astrophysics. 558. A103–A103.252 indexed citations
15.
Song, Hanfeng, et al.. (2013). Close-binary evolution. Astronomy and Astrophysics. 556. A100–A100.41 indexed citations
Ekström, Sylvia, C. Georgy, P. Eggenberger, et al.. (2011). Grids of stellar models with rotation. Astronomy and Astrophysics. 537. A146–A146.1116 indexed citations breakdown →
Granada, A., M. L. Arias, L. S. Cidale, & R. E. Mennickent. (2010). K- and L-band spectroscopy of Be stars. Proceedings of the International Astronomical Union. 6(S272). 392–393.2 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.