This map shows the geographic impact of S. Pascual'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 S. Pascual with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites S. Pascual more than expected).
This network shows the impact of papers produced by S. Pascual. 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 S. Pascual. The network helps show where S. Pascual may publish in the future.
Co-authorship network of co-authors of S. Pascual
This figure shows the co-authorship network connecting the top 25 collaborators of S. Pascual.
A scholar is included among the top collaborators of S. Pascual 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 S. Pascual. S. Pascual is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
García-Vargas, M. L., E. Carrasco, M. Mollá, et al.. (2020). MEGARA-GTC stellar spectral library: I. Monthly Notices of the Royal Astronomical Society. 493(1). 871–898.5 indexed citations
8.
Zamorano, J., Carlos Tapia, S. Pascual, et al.. (2018). Night Sky Brightness monitoring in Spain.. 599–604.1 indexed citations
9.
Tollerud, Erik, S. Pascual, Prasanth B. Nair, et al.. (2017). liberfa/erfa: v1.4.0. Zenodo (CERN European Organization for Nuclear Research).
10.
Zamorano, J., Alejandro Sánchez de Miguel, Carlos Tapia, et al.. (2015). Low-cost photometers and open source software for Light Pollution research. 29. 2254626.5 indexed citations
11.
Castillo-Morales, Á., M. C. Eliche‐Moral, S. Pascual, et al.. (2013). MEGARA control system. LA Referencia (Red Federada de Repositorios Institucionales de Publicaciones Científicas). 42. 123–123.1 indexed citations
12.
Paz, A. Gil de, J. Gallego, Á. Castillo-Morales, et al.. (2013). MEGARA: the future IFU and MOS of the 10.4 M GTC. Redalyc (Universidad Autónoma del Estado de México). 42. 90–92.
13.
Miguel, Alejandro Sánchez de, et al.. (2012). ISS nocturnal images as a scientific tool against Light Pollution: Flux calibration and colors. 916–919.5 indexed citations
14.
Miguel, Alejandro Sánchez de, et al.. (2012). Contaminación Lumínica en España 2012: Light Pollution in Spain 2012. 956–956.1 indexed citations
15.
Caballero, J. A., A. Cabrera‐Lavers, D. García-Álvarez, & S. Pascual. (2012). Stars and brown dwarfs in theσ Orionis cluster. Astronomy and Astrophysics. 546. A59–A59.2 indexed citations
16.
Pascual, S., J. Gallego, N. Cardiel, & M. C. Eliche‐Moral. (2010). PyEmir: Data Reduction Pipeline for EMIR, the GTC Near-IR Multi-Object Spectrograph. ASPC. 434. 353–780.1 indexed citations
Pascual, S., J. Gallego, & N. Cardiel. (2006). Data Reduction Pipeline for EMIR, the Near-IR Multi-Object Spectrograph for GTC. Redalyc (Universidad Autónoma del Estado de México). 29. 142–142.1 indexed citations
19.
Pascual, S., V. Villar, J. Gallego, et al.. (2005). Properties of Hα-selected star-forming galaxies from z ∼ 0.8 to now. 24. 268–269.1 indexed citations
20.
Pascual, S., J. Gallego, Alfonso Aragón‐Salamanca, & J. Zamorano. (2001). Hα emitting galaxies and the star formation rate density at z ≃ 0.24. LA Referencia (Red Federada de Repositorios Institucionales de Publicaciones Científicas).32 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.