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Dark matter is an invisible substance that makes up more than eighty percent of the matter content of the universe. We know of its existence due to its gravitational influence, being a key ingredient to understand everything from the large-scale evolution of the universe to the formation of galaxies like the Milky Way, of which we are part of . However, very little is known about its nature, which constitutes one of the greatest unsolved problems in contemporary physics. The fuzzy dark matter model has recently been studied as a promising candidate. In this model , it is postulated that dark
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Thanks to images obtained by the James Webb Telescope (JWST), an international scientific team in which the Instituto de Astrofísica de Canarias (IAC) participates has been able to verify that galaxies in the early universe are usually flat and elongated, and not round or spiral like the nearest galaxies. International research has found, by analysing high-resolution, infrared images of the JWST, that flattened oval disc and tube-shaped galaxies were much more common when the universe was between 600 million and 6 billion years old. In contrast, the nearest galaxies have clearly defined
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From today the new edition of the monographic magazine Paralajes, produced and edited by the IAC, is available in both digital and paper formats. This volume is on the theme of astronomy in the infrared, radiation outside the range visible to the human eye, very important in the history of the IAC, described in detail in over 170 pages. A major fraction of the energy emitted within the universe is in the infrared, but we cannot detect it except using instruments specially developed to do this. The IAC has been aware of this since its beginning, and has been developing infrared instruments
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