Zobrazeno 1 - 10
of 400
pro vyhledávání: '"Cantalupo, S."'
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:
Jiménez-Andrade, E. F., Cantalupo, S., Magnelli, B., Romano-Díaz, E., Gómez-Guijarro, C., Mackenzie, R., Smolčić, V., Murphy, E., Matthee, J., Toft, S.
Ly$\alpha$ $\lambda$1216 (Ly$\alpha$) emission extending over $\gtrsim\,\rm 10\,kiloparsec\,(kpc)$ around dusty, massive starbursts at $z\gtrsim3$ might represent a short-lived phase in the evolution of present-day, massive quiescent galaxies. To obt
Externí odkaz:
http://arxiv.org/abs/2210.07982
Autor:
Ginolfi, M., Piconcelli, E., Zappacosta, L., Jones, G. C., Pentericci, L., Maiolino, R., Travascio, A., Menci, N., Carniani, S., Rizzo, F., Battaia, F. Arrigoni, Cantalupo, S., De Breuck, C., Graziani, L., Knudsen, K., Laursen, P., Mainieri, V., Schneider, R., Stanley, F., Valiante, R., Verhamme, A.
The phase transition between galaxies and quasars is often identified with the rare population of hyper-luminous, hot dust-obscured galaxies. Galaxy formation models predict these systems to grow via mergers, that can deliver large amounts of gas tow
Externí odkaz:
http://arxiv.org/abs/2208.03248
Autor:
Guaita, L., Aravena, M., Gurung-Lopez, S., Cantalupo, S., Marino, R., Riechers, D., da Cunha, E., Wagg, J., Algera, H. S. B., Dannerbauer, H., Cox, P.
Publikováno v:
A&A 660, A137 (2022)
We study the members of the protocluster around AzTEC3 submillimeter galaxy at z=5.3. We analyzed the data from the MUSE instrument in an area of 1.4x1.4 arcmin^2 around AzTEC3 and derived information on the Lya line in emission. We compared the Lya
Externí odkaz:
http://arxiv.org/abs/2202.03883
Autor:
Brok, J. S. den, Cantalupo, S., Mackenzie, R., Marino, R. A., Pezzulli, G., Matthee, J., Johnson, S. D., Krumpe, M., Urrutia, T., Kollatschny, W.
A prediction of the classic active galactic nuclei (AGN) unification model is the presence of ionisation cones with different orientations depending on the AGN type. Confirmations of this model exist for present times, but it is less clear in the ear
Externí odkaz:
http://arxiv.org/abs/2005.01732
Autor:
Travascio, A., Zappacosta, L., Cantalupo, S., Piconcelli, E., Battaia, F. Arrigoni, Ginolfi, M., Bischetti, M., Vietri, G., Bongiorno, A., D'Odorico, V., Duras, F., Feruglio, C., Vignali, C., Fiore, F.
During the last years, Ly$\alpha$ nebulae have been routinely detected around high-z, radio-quiet quasars (RQQs) thanks to the advent of sensitive integral field spectrographs. Constraining the physical properties of the Ly$\alpha$ nebulae is crucial
Externí odkaz:
http://arxiv.org/abs/2001.07218
Autor:
Umehata, H., Fumagalli, M., Smail, I., Matsuda, Y., Swinbank, A. M., Cantalupo, S., Sykes, C., Ivison, R. J., Steidel, C. C., Shapley, A. E., Vernet, J., Yamada, T., Tamura, Y., Kubo, M., Nakanishi, K., Kajisawa, M., Hatsukade, B., Kohno, K.
Cosmological simulations predict the Universe contains a network of intergalactic gas filaments, within which galaxies form and evolve. However, the faintness of any emission from these filaments has limited tests of this prediction. We report the de
Externí odkaz:
http://arxiv.org/abs/1910.01324
Autor:
Fossati, M., Fumagalli, M., Lofthouse, E. K., D'Odorico, V., Lusso, E., Cantalupo, S., Cooke, R. J., Cristiani, S., Haardt, F., Morris, S. L., Peroux, C., Prichard, L. J., Rafelski, M., Smail, I., Theuns, T.
We present the goals, design, and first results of the MUSE Ultra Deep Field (MUDF) survey, a large programme using the Multi Unit Spectroscopic Explorer (MUSE) instrument at the ESO Very Large Telescope. The MUDF survey is collecting ~ 150 hours on-
Externí odkaz:
http://arxiv.org/abs/1909.04672
Autor:
Marino, R. A., Cantalupo, S., Pezzulli, G., Lilly, S. J., Gallego, S., Mackenzie, R., Matthee, J., Brinchmann, J., Bouché, N., Feltre, A., Muzahid, S., Schroetter, I., Johnson, S. D., Nanayakkara, T.
The well-known quasar SDSS J095253.83+011421.9 (J0952+0114) at z=3.02 has one of the most peculiar spectra discovered so far, showing the presence of narrow Ly$\alpha$ and broad metal emission lines. Although recent studies have suggested that a Prox
Externí odkaz:
http://arxiv.org/abs/1906.06347