All verified mentions of this organization in source documents.
The INAF study was published in the Journal of Geophysical Research: Planets.
The INAF team implemented an approach to separate spectral signals associated with iron-rich clays from those associated with magnesium-rich clays.
The INAF study is based on nearly 1,500 observations acquired by the CRISM (Compact Reconnaissance Imaging Spectrometer for Mars) instrument on NASA’s Mars Reconnaissance Orbiter.
INAF is a lead participant in the development of Ma_MISS (Mars Multispectral Imager for Subsurface Studies), a spectrometer designed to analyze subsurface Martian rocks and soils and reconstruct their geological and environmental history.
Dario Barghini, an INAF researcher from Turin, stated that their cameras in Castellana Grotte and Lecce did not register any bolide the evening of January 10, 2026, after 6:00 PM.
The study led by INAF astrophysicist Sara Mulas produced and analyzed 450 solar maps in K-band from 2018 to 2023.
The INAF radio telescopes can dedicate only a fraction of their time to solar observations, leading to the development of methods for continuous data collection.
Innovations developed at INAF include methods to observe the Sun with large antennas, which were previously considered unfeasible.
The Grueff Radio Telescope and the Sardinia Radio Telescope are two large INAF radio telescopes adapted for high-frequency observations of the Sun.
The SunDish project, established and coordinated by INAF researcher Alberto Pellizzoni, aims to observe the Sun at high radio frequencies, currently from 18 to 26 GHz.
The SunDish project demonstrated the ability to predict solar flares with a high level of success by observing the Sun at high radio frequencies using the INAF's radio telescopes.
The Istituto Nazionale di Astrofisica (INAF) and the University of Palermo collaborated to improve the understanding of young star evolution and star formation mechanisms in the Milky Way.
Marco Tarantino, a PhD student in statistics at the University of Palermo, collaborated with Loredana Prisinzano's team at INAF on the project.
The neural network developed at the University of Palermo in collaboration with INAF overcomes limitations of previous methods by processing hundreds of millions of stars cataloged with only photometric data.
A study by the National Institute for Astrophysics (INAF) provided significant evidence linking high-energy neutrinos to a specific class of supermassive black holes known as Flat-Spectrum Radio Quasars (FSRQ).
The National Institute of Astrophysics (INAF) led a team that revealed the presence of an invisible molecular flow in the young stellar system HH46 using the James Webb Space Telescope.
Maria Gabriella Navarro, a post-doc at INAF, stated that the observations confirmed that HH46 IRS is a binary system with stars separated by approximately 90 times the distance from the Earth to the Sun.
Francesca Onori from Inaf d'Abruzzo emphasizes the effectiveness of a multi-band observational strategy in studying transients.
The symposium was organized in collaboration with the National Laboratory of Astrophysics (LNA) and the National Institute of Astrophysics (INAF).
Sergio Campana, a researcher at the National Institute for Astrophysics (INAF), contributed to identifying the precise position of the transient in the X-ray band using Swift.