- Research Grants
Research Supported by FAPESP assembles referential information of scholarships and research grants from various research modalities, awarded by FAPESP.
Concerning projects carried out in research institutions abroad, FAPESP encourages granted researchers to develop collaborative research with renowned partner organizations from other countries, such as the institution abroad .
The display board "FAPESP Support in Numbers" presents the number of ongoing or concluded scholarships and research grants, awarded by the Foundation, in cooperation with the institution abroad Centro de Estudios de Física del Cosmos de Aragón (CEFCA). In the center of the page, you will see some information on those awarded scholarships and research grants.
Use the "Refine results" list of options to filter information on awarded research in cooperation with the research institution abroad Centro de Estudios de Física del Cosmos de Aragón (CEFCA) and to get results that are more specific for your search, according to the following parameters: type of Research Grants, modalities of Scholarships, Field of Knowledge and Start Date.
The Maps and Graphs show the geographical distribution of FAPESP sponsorship in the State of São Paulo and the historical sequence of funded research, by year, of the ongoing projects from the cooperation with the research institution abroad Centro de Estudios de Física del Cosmos de Aragón (CEFCA).
IAG-USP is part of the Brazilian-Spanish collaboration JPAS (Javalambre Physics of the Accelerating Universe Astrophysical Survey), a photometric sky survey of 8000 square degrees of the sky done in 59 filters. The designs of the J-PAS camera and filter system allow mapping not only the positions and colors of hundreds of millions of galaxies in the sky, but to study their clustering pr...
The J-PAS (Javalambre-Physics of the Accelerated Universe Astrophysical Survey; Benítez, N., Dupke, et al. 2014) represents the largest and most accurate photometric redshift survey ever undertaken. This project, leaded by Brazilian and Spanish institutions, is considered one of the few "new generation" photometric survey (Stage-IV). Although the main scientific case is to carry out an ...
Quasars are the brightest non-transient objects in the Universe. They trace some of the heaviest halos, and are abundant at high redshifts, since their luminosity function peaks around $z~2$. These two facts imply that quasars (AGNs, in a more general sense) have a huge potential to help us map the web of structures of the Universe on its largest scales. This potential has not yet been ...
(Only some records are available in English at this moment)
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