Associate researcher in the astronomy department of UCB, between 2000 and 2002,[1] he has since continued his scientific collaboration with researchers from several American institutes (UCB, UCLA,[2]University of Washington,[3]STScl.[4]) on various topics concerning globular clusters.
From 2007 to July 15, 2011, he was an astronomer in the instrumental division of the Baltimore Space Telescope Science Institute. He shares his work between scientific activities and functional tasks for the institute and for the Hubble Space Telescope Observatory (calibration, user support, maintenance missions and support of the institute in general).[9]
Luigi R. Bedin, principal investigator of major HST programs[11] is also leader of several observation projects for the world's main installations : HST, ESO/VLT,[12]LBT and the James Webb Space Telescope (JWST).[13][14]
He discovered, with his team, an isolated dwarf spheroidal galaxy as old as the universe hidden in NGC 6752. The discovery is published in international media in 2019. The galaxy bears his name : Bedin I.[17]
Research in astrometry and photometry from space with HST is enriched with JWST : calibration and instrumentation, extrasolar planets, clusters of globules.[20]
He is co-author of a study on intermediate black holes with the discovery of a homogeneous dark mass of around 800 M☉ corresponding to an intermediate mass black hole at the center of the cluster closest to Earth, the globular cluster Messier 4.[21]
In 2024, from JWST imaging of the nearest globular clusters, it detected excess infrared emission among white dwarfs in NGC 6397, a potential indication of destroyed ancient planetary systems and possible insights into the properties of the dense hydrogen atmosphere of these white dwarfs.[22]
Tribute
2018 : The dwarf galaxy Bedin I discovered with his team.[24]
^"Program Information". STScI.edu. Retrieved 2022-01-12. HST Programs With PI Last Name Similar To: bedin = 16653 - Luigi Bedin astrometric signature of a Second Planet in Proxima 15884 - Luigi Bedin Confirmation of an Astrometrically Detected Exoplanet Candidate Orbiting the closest Brown Dwarfs 15491 - Luigi Bedin The end of the White Dwarf Cooling Sequence of NGC 6752 15096 - Luigi Bedin The end of the White Dwarf Cooling Sequence of NGC 6752 14662 - Luigi Bedin The end of the White Dwarf Cooling Sequences of Omega Centauri 14330 - Luigi Bedin Astrometric search for Planets in the closest Brown Dwarf Binary system Luhman 16AB 14118 - Luigi Bedin The end of the White Dwarf Cooling Sequences of Omega Centauri 13748 - Luigi Bedin Astrometric search for Planets in the closest Brown Dwarf Binary system Luhman 16AB 12911 - Luigi Bedin A search for binaries with massive companions in the core of the closest globular cluster M4 12669 - Luigi Bedin Exploring the Bottom End of the White Dwarf Cooling Sequence in the Open Cluster NGC6819 11688 - Luigi Bedin Exploring the Bottom End of the White Dwarf Cooling Sequence in the Open Cluster NGC6819 10500 - Luigi Bedin Exploring the Bottom End of the White Dwarf Cooling Sequence in the Galactic Open Cluster NGC2158 10146 - Luigi Bedin Solving the problem of the White Dwarf Cooling Sequence End in M4: an efficent approach
^Galliani, Marco (2017-06-01). "Due nane brune per Hubble". MEDIA INAF (in Italian). Retrieved 2022-01-15. L'extraordinaire proximité de ce système en fait un laboratoire idéal pour étudier les propriétés des naines brunes, en particulier leurs atmosphères, l'évolution de leur température de surface, la nature binaire du système lui-même, et la présence éventuelle d'exoplanètes autour d'elles. Précisément sur ce dernier point Luigi Bedin, astronome de l'Institut national d'astrophysique (INAF) à l'Observatoire astronomique de Padoue, a récemment obtenu l'opportunité d'observer le système Luhman 16 avec le télescope spatial Hubble.
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