CANTALUPO SEBASTIANO

Villani, I., Zappacosta, L., Piconcelli, E., Ginolfi, M., Ricci, F., La Franca, F., et al. (2026). A deep X-ray look to the most obscured quasar at z   ∼  3.6 and its environment. ASTRONOMY & ASTROPHYSICS, 705(January 2026), 1-11 [10.1051/0004-6361/202556627]. Detail

Dutta, S., Muzahid, S., Schaye, J., Johnson, S., Bouche, N., Augustin, R., et al. (2026). MUSEQuBES: the column density, covering fraction, mass, and environmental dependence of cool Hi gas around low-redshift galaxies. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 545(3) [10.1093/mnras/staf2080]. Detail

Tornotti, D., Fumagalli, M., Fossati, M., Benitez-Llambay, A., Izquierdo-Villalba, D., Travascio, A., et al. (2025). High-definition imaging of a filamentary connection between a close quasar pair at z = 3. NATURE ASTRONOMY, 9(4), 577-588 [10.1038/s41550-024-02463-w]. Detail

Galbiati, M., Cantalupo, S., Steidel, C., Pensabene, A., Travascio, A., Wang, W., et al. (2025). Connecting the growth of galaxies to the large-scale environment in a massive node of the Cosmic Web at z ∼ 3. ASTRONOMY & ASTROPHYSICS, 696(April 2025), 1-20 [10.1051/0004-6361/202452493]. Detail

Pensabene, A., Galbiati, M., Fumagalli, M., Fossati, M., Smail, I., Rafelski, M., et al. (2025). The MUSE Ultra Deep Field (MUDF): VII. Probing high-redshift gas structures in the surroundings of ALMA-identified massive dusty galaxies. ASTRONOMY & ASTROPHYSICS, 696(April 2025), 1-14 [10.1051/0004-6361/202452462]. Detail