R. Abuter, Fatmé Allouche, C. Bailet, M. Benisty, Anthony Berdeu, Jean-Philippe Berger, P. Berio, Azzurra Bigioli, Christopher Blanchard, O. Boebion, H. Bonnet, G. Bourdarot, P. Bourget, W. Brandner, J. Brulé, P. Burgos, M. Carbillet, C. Correia, B. Courtney Barrer, Stéphane Curaba, R. Davies, D. Defrère, A. Delboulbé, F. Delplancke, R. Dembet, A. Drescher, Nicolás Dubost, A. Eckart, C. Édouard, F. Eisenhauer, Luis Esteras Otal, M Fabricius, H. Feuchtgruber, P. Fédou, G. Finger, N. M. Förster Schreiber, R. Frahm, E. García, P. Garcia, R. García López, R. Genzel, J. P. Gil, S. Gillessen, T. Gomes, F. Gonté, V. Gopinath, C. Gouvret, J. Graf, P. Guajardo, S. Guieu, W. Hackenberg, M. Hartl, X. Haubois, F. Haußmann, T. Henning, Pascale Hibon, S. Hönig, M. Horrobin, M. Houllé, N. Hubin, Ihsan Ibn Taïeb, L. Jochum, L. Jocou, A. Jost, J. Kammerer, L. Karl, A. Kaufer, Petra Kern, P. Kervella, J. Kolb, H. Korhonen, L. Kreidberg, P. W. Krempl, S. Lacour, S. Lagarde, Olivier Lai, V. Lapeyrère, R. Laugier, Vítor Leal, J.-B. Le Bouquin, J. Leftley, P. Léna, B. Lopez, D. Lutz, Y. Magnard, F. Mang, A. Marcotto, D. Maurel, A. Mérand, F. Millour, M. Montargès, N. More, Nuno Morujão, T. Moulin, H. Nowacki, Mathias Nowak, S. Oberti, T. Ott, L. Pallanca, F. Patru
GRAVITY+ improves by orders of magnitude the sensitivity, sky-coverage, and contrast of the Very Large Telescope Interferometer (VLTI). A central part of this project is the development of Gravity Plus Adaptive Optics (GPAO), a dedicated high-order and laser-guide star adaptive optics (AO) system for VLTI. GPAO consists of four state-of-the-art AO systems that equip all 8 m class Unit Telescopes (UTs) for the wavefront correction of the VLTI instruments. It offers both visible and infrared natural guide star (NGS) and laser guide star (LGS) operations. The paper presents the design, operations, and performances of GPAO. We illustrate the improvement brought by GPAO with interferometric observations obtained during the commissioning of the NGS mode at the end of 2024. These science results include the first optical interferometry observations of a redshift z ~ 4 quasar, the spectroscopy of a cool brown-dwarf with magnitude K ~ 21.0, the first observations of a Class I young star with GRAVITY, and the first sub-micro arcsecond differential astrometry in the optical. Together with the entire GRAVITY+ project, the implementation of GPAO is a true paradigm shift for observing the optical Universe at very high angular resolution.