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.
Magnetism, rotation, and nonthermal emission in cool stars
2022102 citationsA. Reiners, I. Ribas et al.Astronomy and Astrophysicsprofile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
hero ref
This map shows the geographic impact of P. J. Amado'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 P. J. Amado with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites P. J. Amado more than expected).
This network shows the impact of papers produced by P. J. Amado. 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 P. J. Amado. The network helps show where P. J. Amado may publish in the future.
Co-authorship network of co-authors of P. J. Amado
This figure shows the co-authorship network connecting the top 25 collaborators of P. J. Amado.
A scholar is included among the top collaborators of P. J. Amado 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 P. J. Amado. P. J. Amado is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Cifuentes, C., J. A. Caballero, P. J. Amado, et al.. (2024). CARMENES input catalogue of M dwarfs. Astronomy and Astrophysics. 693. A228–A228.4 indexed citations
Cortés‐Contreras, M., J. A. Caballero, V. J. S. Béjar, et al.. (2015). Preparation of the CARMENES Input Catalogue: Multiplicity of M dwarfs from Tenths of Arcseconds to Hundreds of Arcminutes. 18. 805–810.
15.
Amado, P. J., A. Quirrenbach, J. A. Caballero, et al.. (2013). CARMENES: A radial-velocity survey for terrestrial planets in the habitable zones of M dwarfs. A historical overview. Max Planck Institute for Plasma Physics. 842–847.1 indexed citations
16.
Caballero, J. A., M. Cortés‐Contreras, F. J. Alonso-Floriano, et al.. (2013). CARMENES. III. CARMENCITA, the input catalogue. 645–645.
17.
Alonso-Floriano, F. J., D. Montes, J. A. Caballero, et al.. (2013). CARMENES. IV. Preliminary low-resolution spectroscopic characterisation. Max Planck Institute for Plasma Physics. 431–431.1 indexed citations
18.
Caballero, J. A., M. Cortés‐Contreras, F. J. Alonso-Floriano, et al.. (2013). CARMENES at PPVI. CARMENCITA Herbs and Spices to Help you Prepare a Genuine Target Sample.
19.
Amado, P. J., et al.. (2001). Monitoring of spotted RS CVn and BY Dra type stars. I. Simultaneous optical and infrared photometry. 31(1). 13–25.2 indexed citations
20.
Amado, P. J.. (1997). Physical properties of starspots. Observatory. 118. 247–248.1 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.