Zobrazeno 1 - 10
of 583
pro vyhledávání: '"Travascio, A"'
Autor:
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.
A direct link between large-scale environment and galaxy properties is very well established in the local universe. However, very little is known about the role of the environment for galaxy growth before the peak of the cosmic star formation history
Externí odkaz:
http://arxiv.org/abs/2410.03822
Autor:
Travascio, A., Cantalupo, S., Tozzi, P., Vito, F., Paggi, A., Pezzulli, G., 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.
Exploring SMBH population in protoclusters offers valuable insights into how environment affects SMBH growth. However, research on AGN within these areas is still limited by the small number of protoclusters known at high redshift and by the availabi
Externí odkaz:
http://arxiv.org/abs/2410.03933
Autor:
Wang, Weichen, Cantalupo, Sebastiano, Pensabene, Antonio, Galbiati, Marta, Travascio, Andrea, Steidel, Charles C., Maseda, Michael V., Pezzulli, Gabriele, de Beer, Stephanie, Fossati, Matteo, Fumagalli, Michele, Gallego, Sofia G., Lazeyras, Titouan, Mackenzie, Ruari, Matthee, Jorryt, Nanayakkara, Themiya, Quadri, Giada
Observational studies showed that galaxy disks are already in place in the first few billion years of the universe. The early disks detected so far, with typical half-light radii of 3 kiloparsecs at stellar masses around 10^11 M_sun for redshift z~3,
Externí odkaz:
http://arxiv.org/abs/2409.17956
Autor:
Tornotti, Davide, Fumagalli, Michele, Fossati, Matteo, Benitez-Llambay, Alejandro, Izquierdo-Villalba, David, Travascio, Andrea, Battaia, Fabrizio Arrigoni, Cantalupo, Sebastiano, Beckett, Alexander, Bonoli, Silvia, Dayal, Pratika, D'Odorico, Valentina, Dutta, Rajeshwari, Lusso, Elisabeta, Peroux, Celine, Rafelski, Marc, Revalski, Mitchell, Spinoso, Daniele, Swinbank, Mark
Filaments connecting halos are a long-standing prediction of cold dark matter theories. We present a novel detection of the cosmic web emission connecting two massive quasar-host galaxies at cosmic noon in the MUSE Ultra Deep Field (MUDF) using unpre
Externí odkaz:
http://arxiv.org/abs/2406.17035
Autor:
Liang, Yongming, Ouchi, Masami, Sun, Dongsheng, Kashikawa, Nobunari, Cai, Zheng, Cantalupo, Sebastiano, Nagamine, Kentaro, Yajima, Hidenobu, Kirihara, Takanobu, Zhang, Haibin, Li, Mingyu, Shimakawa, Rhythm, Fan, Xiaohui, Ito, Kei, Tanaka, Masayuki, Harikane, Yuichi, Prochaska, J. Xavier, Travascio, Andrea, Wang, Weichen, Elvis, Martin, Fabbiano, Giuseppina, Arita, Junya, Onoue, Masafusa, Silverman, John D., Shi, Dongdong, An, FangXia, Izumi, Takuma, Shimasaku, Kazuhiro, Uchiyama, Hisakazu, Zhu, Chenghao
We report the identification of a quasar overdensity in the BOSSJ0210 field, dubbed Cosmic Himalayas, consisting of 11 quasars at $z=2.16-2.20$, the densest overdensity of quasars ($17\sigma$) in the $\sim$10,000 deg$^2$ of the Sloan Digital Sky Surv
Externí odkaz:
http://arxiv.org/abs/2404.15963
Autor:
Travascio, A., Piconcelli, E., Bischetti, M., Cresci, G., Feruglio, C., Perna, M., Vietri, G., Carniani, S., Cantalupo, S., Cicone, C., Ginolfi, M., Venturi, G., Zubovas, K., Bongiorno, A., Brusa, M., Luminari, A., Mainieri, V., Marconi, A., Menci, N., Nardini, E., Pensabene, A., Almeida, C. Ramos, Tombesi, F., Vignali, C., Zappacosta, L., Fiore, F.
Publikováno v:
A&A 686, A250 (2024)
PDS 456 is the most luminous RQQ at z<0.3 and can be regarded as a local counterpart of the powerful QSOs shining at Cosmic Noon. It hosts a strong nuclear X-ray ultra-fast outflow, and a massive and clumpy CO(3-2) molecular outflow extending up to 5
Externí odkaz:
http://arxiv.org/abs/2403.18043
Autor:
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. V.
Sub-mm surveys toward overdense regions in the early Universe are essential to uncover the obscured star-formation and the cold gas content of assembling galaxies within massive dark matter halos. In this work, we present deep ALMA mosaic observation
Externí odkaz:
http://arxiv.org/abs/2401.04765
Autor:
de Beer, Stephanie, Cantalupo, Sebastiano, Travascio, Andrea, Pezzulli, Gabriele, Galbiati, Marta, Fossati, Matteo, Fumagalli, Michele, Lazeyras, Titouan, Pensabene, Antonio, Theuns, Tom, Wang, Weichen
Ly$\alpha$ nebulae ubiquitously found around z>2 quasars can supply unique constraints on the properties of the Circumgalactic Medium, such as its density distribution, provided the quasar halo mass is known. We present a new method to constrain quas
Externí odkaz:
http://arxiv.org/abs/2309.01506
Autor:
Zanchettin, Maria Vittoria, Feruglio, Chiara, Massardi, Marcella, Lapi, Andrea, Bischetti, Manuela, Cantalupo, Sebastiano, Fiore, Fabrizio, Bongiorno, Angela, Malizia, Angela, Marinucci, Andrea, Molina, Manuela, Piconcelli, Enrico, Tombesi, Francesco, Travascio, Andrea, Tozzi, Giulia, Tripodi, Roberta
Publikováno v:
A&A 679, A88 (2023)
We present an analysis of the gas kinematics in NGC 2992, based on VLT/MUSE, ALMA and VLA data, aimed at characterising the disk, the wind and their interplay in the cold molecular and warm ionised phases. CO(2-1) and H$\rm \alpha~$ arise from a mult
Externí odkaz:
http://arxiv.org/abs/2308.04108
Publikováno v:
Frontiers in Bioengineering and Biotechnology, Vol 12 (2024)
Externí odkaz:
https://doaj.org/article/03be4c9d164e458c94fb0bddb2804f2a
