CANTALUPO, SEBASTIANO
CANTALUPO, SEBASTIANO
DIPARTIMENTO DI FISICA "GIUSEPPE OCCHIALINI"
A deep X-ray look to the most obscured quasar at z ∼ 3.6 and its environment
2026 Villani, I; Zappacosta, L; Piconcelli, E; Ginolfi, M; Ricci, F; La Franca, F; Arrigoni-Battaia, F; Bongiorno, A; Cantalupo, S; Carniani, S; Civano, F; Comastri, A; Fiore, F; Maiolino, R; Pentericci, L; Ricci, C; Schneider, R; Valiante, R; Vignali, C; Vito, F
MUSEQuBES: the column density, covering fraction, mass, and environmental dependence of cool Hi gas around low-redshift galaxies
2026 Dutta, S; Muzahid, S; Schaye, J; Johnson, S; Bouche, N; Augustin, R; Cantalupo, S; Chen, H; Wendt, M
A giant disk galaxy two billion years after the Big Bang
2025 Wang, W; Cantalupo, S; Pensabene, A; Galbiati, M; Travascio, A; Steidel, C; Maseda, M; Pezzulli, G; De Beer, S; Fossati, M; Fumagalli, M; Gallego, S; Lazeyras, T; Mackenzie, R; Matthee, J; Nanayakkara, T; Quadri, G
ALMA survey of a massive node of the Cosmic Web at z a 3: II. A dynamically cold and massive disk galaxy in the proximity of a hyper-luminous quasar
2025 Pensabene, A; Cantalupo, S; Wang, W; Bacchini, C; Fraternali, F; Bischetti, M; Cicone, C; Decarli, R; Pezzulli, G; Galbiati, M; Lazeyras, T; Ledos, N; Quadri, G; Travascio, A
Connecting the growth of galaxies to the large-scale environment in a massive node of the Cosmic Web at z ∼ 3
2025 Galbiati, M; Cantalupo, S; Steidel, C; Pensabene, A; Travascio, A; Wang, W; Fossati, M; Fumagalli, M; Rudie, G; Fresco, A; Lazeyras, T; Ledos, N; Quadri, G
Cosmic Himalayas: The Highest Quasar Density Peak Identified in a 10,000 deg2 Sky with Spatial Discrepancies between Galaxies, Quasars, and IGM H i
2025 Liang, Y; Ouchi, M; Sun, D; Kashikawa, N; Cai, Z; Cantalupo, S; Nagamine, K; Yajima, H; Kirihara, T; Zhang, H; Li, M; Shimakawa, R; Fan, X; Ito, K; Tanaka, M; Harikane, Y; Prochaska, J; Travascio, A; Wang, W; Elvis, M; Fabbiano, G; Arita, J; Onoue, M; Silverman, J; Shi, D; An, F; Izumi, T; Shimasaku, K; Uchiyama, H; Zhu, C
HI Properties of Field Galaxies at z ≈ 0.2–0.6: Insights into Declining Cosmic Star Formation
2025 Depalma, D; Gupta, N; Chen, H; Simcoe, R; Balashev, S; Boettcher, E; Cantalupo, S; Chen, M; Combes, F; Faucher-Giguere, C; Johnson, S; Klockner, H; Krogager, J; I-Hsiu Li, J; Lopez, S; Noterdaeme, P; Petitjean, P; Qu, Z; Rudie, G; Schaye, J; Zahedy, F
High-definition imaging of a filamentary connection between a close quasar pair at z = 3
2025 Tornotti, D; Fumagalli, M; Fossati, M; Benitez-Llambay, A; Izquierdo-Villalba, D; Travascio, A; Arrigoni Battaia, F; Cantalupo, S; Beckett, A; Bonoli, S; Dayal, P; D'Odorico, V; Dutta, R; Lusso, E; Peroux, C; Rafelski, M; Revalski, M; Spinoso, D; Swinbank, M
MUSEQuBES: Connecting H i Absorption with Lyα Emitters at z ≈ 3.3
2025 Banerjee, E; Muzahid, S; Schaye, J; Blaizot, J; Bouche, N; Cantalupo, S; Johnson, S; Matthee, J; Verhamme, A
MUSEQuBES: The Kinematics of O vi-bearing Gas in and around Low-redshift Galaxies
2025 Dutta, S; Muzahid, S; Schaye, J; Cantalupo, S; Chen, H; Johnson, S
MUSEQuBES: Unveiling Cosmic Web Filaments at z ≈ 3.6 through Dual Absorption and Emission Line Analysis
2025 Banerjee, E; Muzahid, S; Schaye, J; Cantalupo, S; Johnson, S
The Morphology and Kinematics of a Giant, Symmetric Nebula around a Radio-loud Quasar 3C 57: Extended Rotating Gas or Biconical Outflows?
2025 Liu, Z; Johnson, S; Li, J; Epinat, B; Rudie, G; Monreal-Ibero, A; Cantalupo, S; Qu, Z; Chen, M; Kollatschny, W; Muzahid, S; Zahedy, F; Kesler, E; Mishra, N
The MUSE Ultra Deep Field (MUDF): VII. Probing high-redshift gas structures in the surroundings of ALMA-identified massive dusty galaxies
2025 Pensabene, A; Galbiati, M; Fumagalli, M; Fossati, M; Smail, I; Rafelski, M; Revalski, M; Arrigoni-Battaia, F; Beckett, A; Cantalupo, S; Dutta, R; Lusso, E; Lazeyras, T; Quadri, G; Tornotti, D
The properties of X-ray-selected active galactic nuclei in protoclusters pinpointed by enormous Lyman alpha nebulae
2025 Traina, A; Vito, F; Arrigoni-Battaia, F; Chen, C; Vignali, C; Prochaska, X; Cantalupo, S; Pensabene, A; Tozzi, P; Travascio, A; Gilli, R; Isla Llave, M; Marchesi, S; Mazzolari, G
X-ray view of a massive node of the Cosmic Web at z ∼ 3 I. An exceptional overdensity of rapidly accreting supermassive black holes
2025 Travascio, A; Cantalupo, S; Tozzi, P; Vito, F; Pezzulli, G; Paggi, A; Elvis, M; Fabbiano, G; Fiore, F; Fossati, M; Fresco, A; Fumagalli, M; Galbiati, M; Lazeyras, T; Ledos, N; Pannella, M; Pensabene, A; Quadri, G; Wang, W
ALMA survey of a massive node of the Cosmic Web at z ∼ 3: I. Discovery of a large overdensity of CO emitters
2024 Pensabene, A; Cantalupo, S; Cicone, C; Decarli, R; Galbiati, M; Ginolfi, M; de Beer, S; Fossati, M; Fumagalli, M; Lazeyras, T; Pezzulli, G; Travascio, A; Wang, W; Matthee, J; Maseda, M
An Ensemble Study of Turbulence in Extended QSO Nebulae at z ≈ 0.5-1
2024 Chen, M; Chen, H; Rauch, M; Qu, Z; Johnson, S; Schaye, J; Rudie, G; Li, J; Liu, Z; Zahedy, F; Cantalupo, S; Boettcher, E
Atacama Large Aperture Submillimeter Telescope (AtLAST) science: The hidden circumgalactic medium
2024 Lee, M; Schimek, A; Cicone, C; Andreani, P; Popping, G; Sommovigo, L; Appleton, P; Bischetti, M; Cantalupo, S; Chen, C; Dannerbauer, H; De Breuck, C; Di Mascolo, L; Emonts, B; Hatziminaoglou, E; Pensabene, A; Rizzo, F; Rybak, M; Shen, S; Lundgren, A; Booth, M; Klaassen, P; Mroczkowski, T; Cordiner, M; Johnstone, D; van Kampen, E; Liu, D; Maccarone, T; Saintonge, A; Smith, M; Thelen, A; Wedemeyer, S
Discovery of Optically Emitting Circumgalactic Nebulae around the Majority of UV-luminous Quasars at Intermediate Redshift
2024 Johnson, S; Liu, Z; Li, J; Schaye, J; Greene, J; Cantalupo, S; Rudie, G; Qu, Z; Chen, H; Rafelski, M; Muzahid, S; Chen, M; Contini, T; Kollatschny, W; Mishra, N; Petitjean, P; Rauch, M; Zahedy, F
MAMMOTH-Subaru. II. Diverse Populations of Circumgalactic Lyα Nebulae at Cosmic Noon
2024 Li, M; Zhang, H; Cai, Z; Liang, Y; Kashikawa, N; Ma, K; Fan, X; Prochaska, J; Emonts, B; Wang, X; Wu, Y; Zhang, S; Li, Q; Johnson, S; Yue, M; Arrigoni Battaia, F; Cantalupo, S; Hennawi, J; Kikuta, S; Ning, Y; Ouchi, M; Shimakawa, R; Wang, B; Wang, W; Zheng, Z; Zheng, Z