CANTALUPO SEBASTIANO
Publications
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
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
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
Liang, Y., Ouchi, M., Sun, D., Kashikawa, N., Cai, Z., Cantalupo, S., et al. (2025). Cosmic Himalayas: The Highest Quasar Density Peak Identified in a 10,000 deg2 Sky with Spatial Discrepancies between Galaxies, Quasars, and IGM H i. THE ASTROPHYSICAL JOURNAL, 986(1) [10.3847/1538-4357/adc1bb]. Detail
Depalma, D., Gupta, N., Chen, H., Simcoe, R., Balashev, S., Boettcher, E., et al. (2025). HI Properties of Field Galaxies at z ≈ 0.2–0.6: Insights into Declining Cosmic Star Formation. THE ASTROPHYSICAL JOURNAL LETTERS, 993(1) [10.3847/2041-8213/ae0d8b]. Detail