Zobrazeno 1 - 10
of 21 146
pro vyhledávání: '"A Puglisi"'
Autor:
Bertola, E., Circosta, C., Ginolfi, M., Mainieri, V., Vignali, C., Rivera, G. Calistro, Ward, S. R., Lopez, I. E., Pensabene, A., Alexander, D. M., Bischetti, M., Brusa, M., Cappi, M., Comastri, A., Contursi, A., Cicone, C., Cresci, G., Dadina, M., D'Amato, Q., Feltre, A., Harrison, C. M., Kakkad, D., Lamperti, I., Lanzuisi, G., Mannucci, F., Marconi, A., Perna, M., Piconcelli, E., Puglisi, A., Ricci, F., Scholtz, J., Tozzi, G., Vietri, G., Zamorani, G., Zappacosta, L.
The energy released by AGN has the potential to heat or remove the gas of the ISM, thus likely impacting the cold molecular gas reservoir of host galaxies at first, with star formation following on longer timescales. Previous works on high-z galaxies
Externí odkaz:
http://arxiv.org/abs/2408.16821
Autor:
Stepney, Matthew, Banerji, Manda, Tang, Shenli, Hewett, Paul C., Temple, Matthew J., Wethers, Clare F., Puglisi, Annagrazia, Molyneux, Stephen J.
We present a deep X-Shooter rest-frame UV to optical spectral analysis of the heavily reddened quasar, ULASJ2315+043 at z=2.566, known to reside in a major-merger host galaxy. The rest-frame optical is best-fit by a dust-reddened quasar E(B-V)_QSO =
Externí odkaz:
http://arxiv.org/abs/2408.10403
Autor:
Amerini, Irene, Barni, Mauro, Battiato, Sebastiano, Bestagini, Paolo, Boato, Giulia, Bonaventura, Tania Sari, Bruni, Vittoria, Caldelli, Roberto, De Natale, Francesco, De Nicola, Rocco, Guarnera, Luca, Mandelli, Sara, Marcialis, Gian Luca, Micheletto, Marco, Montibeller, Andrea, Orru', Giulia, Ortis, Alessandro, Perazzo, Pericle, Puglisi, Giovanni, Salvi, Davide, Tubaro, Stefano, Tonti, Claudia Melis, Villari, Massimo, Vitulano, Domenico
AI-generated synthetic media, also called Deepfakes, have significantly influenced so many domains, from entertainment to cybersecurity. Generative Adversarial Networks (GANs) and Diffusion Models (DMs) are the main frameworks used to create Deepfake
Externí odkaz:
http://arxiv.org/abs/2408.00388
Autor:
Tan, Qing-Hua, Daddi, Emanuele, Magnelli, Benjamin, Correa, Camila A., Bournaud, Frédéric, Adscheid, Sylvia, Zhang, Shao-Bo, Elbaz, David, Gómez-Guijarro, Carlos, Kalita, Boris S., Liu, Daizhong, Liu, Zhaoxuan, Pety, Jérôme, Puglisi, Annagrazia, Schinnerer, Eva, Silverman, John D., Valentino, Francesco
The majority of stars in today's Universe reside within spheroids, which are bulges of spiral galaxies and elliptical galaxies. Their formation is still an unsolved problem. Infrared/submm-bright galaxies at high redshifts have long been suspected to
Externí odkaz:
http://arxiv.org/abs/2407.16578
Autor:
de Xivry, Gilles Orban, Absil, Olivier, De Rosa, Robert J., Bonse, Markus J., Dannert, Felix, Hayoz, Jean, Grani, Paolo, Puglisi, Alfio, Baruffolo, Andrea, Salasnich, Bernardo, Davies, Ric, Glauser, Adrian M., Huby, Elsa, Kenworthy, Matthew, Quanz, Sascha P., Taylor, William, Zins, Gérard
Publikováno v:
Proceedings of the SPIE, Volume 13097, id. 13097-42 (2024)
The Enhanced Resolution Imager and Spectrograph (ERIS) is the new near-infrared instrument at the VLT-UT4. ERIS replaces and extends the observational capabilities formerly provided by SINFONI and NACO: integral field spectroscopy at 1 - 2.5 $\mu$m,
Externí odkaz:
http://arxiv.org/abs/2407.14406
Autor:
Tozzi, G., Cresci, G., Perna, M., Mainieri, V., Mannucci, F., Marconi, A., Kakkad, D., Marasco, A., Brusa, M., Bertola, E., Bischetti, M., Carniani, S., Cicone, C., Circosta, C., Fiore, F., Feruglio, C., Harrison, C. M., Lamperti, I., Netzer, H., Piconcelli, E., Puglisi, A., Scholtz, J., Vietri, G., Vignali, C., Zamorani, G.
We present spatially resolved VLT/SINFONI spectroscopy with adaptive optics of type-2 active galactic nuclei (AGN) from the SINFONI Survey for Unveiling the Physics and Effect of Radiative feedback (SUPER), which targeted X-ray bright ($L_{2-10 keV}\
Externí odkaz:
http://arxiv.org/abs/2407.04099
Autor:
Yao, Jian, Krachmalnicoff, Nicoletta, Foschi, Marianna, Puglisi, Giuseppe, Baccigalupi, Carlo
We present ForSE+, a Python package that produces non-Gaussian diffuse Galactic thermal dust emission maps at arcminute angular scales and that has the capacity to generate random realizations of small scales. This represents an extension of the ForS
Externí odkaz:
http://arxiv.org/abs/2406.14519
Autor:
Fu, Hao, Shankar, Francesco, Ayromlou, Mohammadreza, Koutsouridou, Ioanna, Cattaneo, Andrea, Bertemes, Caroline, Bellstedt, Sabine, Martín-Navarro, Ignacio, Leja, Joel, Allevato, Viola, Bernardi, Mariangela, Boco, Lumen, Dimauro, Paola, Gruppioni, Carlotta, Lapi, Andrea, Menci, Nicola, Rodríguez, Iván Muñoz, Puglisi, Annagrazia, Alonso-Tetilla, Alba V.
In a hierarchical, dark matter-dominated Universe, stellar mass functions (SMFs), galaxy merger rates, star formation histories (SFHs), satellite abundances, and intracluster light, should all be intimately connected observables. However, the systema
Externí odkaz:
http://arxiv.org/abs/2406.07605
Autor:
Puglisi, Lemuel, Rondinella, Alessia, De Meo, Linda, Guarnera, Francesco, Battiato, Sebastiano, Ravì, Daniele
Brain age is a critical measure that reflects the biological ageing process of the brain. The gap between brain age and chronological age, referred to as brain PAD (Predicted Age Difference), has been utilized to investigate neurodegenerative conditi
Externí odkaz:
http://arxiv.org/abs/2406.00365
In this work, we introduce Brain Latent Progression (BrLP), a novel spatiotemporal disease progression model based on latent diffusion. BrLP is designed to predict the evolution of diseases at the individual level on 3D brain MRIs. Existing deep gene
Externí odkaz:
http://arxiv.org/abs/2405.03328