Zobrazeno 1 - 10
of 324
pro vyhledávání: '"Pappalardo C"'
Autor:
Carvajal, R., Matute, I., Afonso, J., Norris, R. P., Luken, K. J., Sánchez-Sáez, P., Cunha, P. A. C., Humphrey, A., Messias, H., Amarantidis, S., Barbosa, D., Cruz, H. A., Miranda, H., Paulino-Afonso, A., Pappalardo, C.
Publikováno v:
A&A 679, A101 (2023)
We developed and trained a pipeline of three machine learning (ML) models than can predict which sources are more likely to be an AGN and to be detected in specific radio surveys. Also, it can estimate redshift values for predicted radio-detectable A
Externí odkaz:
http://arxiv.org/abs/2309.11652
Autor:
Bischetti, M., Feruglio, C., Piconcelli, E., Duras, F., Pèrez-Torres, M., Herrero, R., Venturi, G., Carniani, S., Bruni, G., Gavignaud, I., Testa, V., Bongiorno, A., Brusa, M., Circosta, C., Cresci, G., D'Odorico, V., Maiolino, R., Marconi, A., Mingozzi, M., Pappalardo, C., Perna, M., Traianou, E., Travascio, A., Vietri, G., Zappacosta, L., Fiore, F.
Publikováno v:
A&A 645, A33 (2021)
Sources at the brightest end of QSO luminosity function during the peak epoch of star formation and black hole accretion (z~2-4, i.e. Cosmic noon) are privileged sites to study the feeding & feedback cycle of massive galaxies. We perform the first sy
Externí odkaz:
http://arxiv.org/abs/2009.01112
Autor:
Maiolino, R., Cirasuolo, M., Afonso, J., Bauer, F. E., Bowler, R., Cucciati, O., Daddi, E., De Lucia, G., Evans, C., Flores, H., Gargiulo, A., Garilli, B., Jablonka, P., Jarvis, M., Kneib, J. -P., Lilly, S., Looser, T., Magliocchetti, M., Man, Z., Mannucci, F., Maurogordato, S., McLure, R. J., Norberg, P., Oesch, P., Oliva, E., Paltani, S., Pappalardo, C., Peng, Y., Pentericci, L., Pozzetti, L., Renzini, A., Rodrigues, M., Royer, F., Serjeant, S., Vanzi, L., Wild, V., Zamorani, G.
Publikováno v:
The Messenger, vol. 180, 2020, p. 24-29
The MOONS instrument possesses an exceptional combination of large multiplexing, high sensitivity, broad simultaneous spectral coverage (from optical to near-infrared bands), large patrol area and high fibre density. These properties provide the unpr
Externí odkaz:
http://arxiv.org/abs/2009.00644
Autor:
Padilla Suarez, E.G., Pugliese, S., Galdiero, E., Guida, M., Libralato, G., Saviano, L., Spampinato, M., Pappalardo, C., Siciliano, A.
Publikováno v:
In Environmental Pollution 15 November 2023 337
Autor:
Dannerbauer, H., van Kampen, E., Afonso, J., Andreani, P., Battaia, F. Arrigoni, Bertoldi, F., Casey, C., Chen, C. -C., Clements, D. L., De Breuck, C., Frye, B., Geach, J., Harrington, K., Hayashi, M., Jin, S., Klaassen, P., Kohno, K., Lehnert, M. D., Matute, I., Mroczkowski, T., Noble, A., Pappalardo, C., Tamura, Y., Zavala, J.
We present the science case for mapping several thousand galaxy (proto)clusters at z=1-10 with a large aperture single dish sub-mm facility, producing a high-redshift counterpart to local large surveys of rich clusters like the well-studied Abell cat
Externí odkaz:
http://arxiv.org/abs/1903.06238
Since the Virgo cluster is the closest galaxy cluster in the northern hemisphere, galaxy interactions can be observed in it with a kpc resolution. The spiral galaxy NGC 4388 underwent a ram pressure stripping event ~200 Myr ago caused by its highly e
Externí odkaz:
http://arxiv.org/abs/1809.03805
Autor:
Bischetti, M., Piconcelli, E., Feruglio, C., Duras, F., Bongiorno, A., Carniani, S., Marconi, A., Pappalardo, C., Schneider, R., Travascio, A., Valiante, R., Vietri, G., Zappacosta, L., Fiore, F.
We present an ALMA high-resolution observation of the 840 um continuum and [CII] line emission in the WISE-SDSS selected hyper-luminous (WISSH) QSO J1015+0020 at z~4.4. Our analysis reveals an exceptional overdensity of [CII]-emitting companions with
Externí odkaz:
http://arxiv.org/abs/1804.06399
Autor:
Donevski, D., Buat, V., Boone, F., Pappalardo, C., Bethermin, M., Schreiber, C., Mazyed, F., Álvarez-Márquez, J., Duivenvoorden, S.
Publikováno v:
A&A 614, A33 (2018)
$\mathit{Herschel}$ extragalactic surveys offer a unique opportunity to efficiently select a significant number of rare and massive dusty objects, and thus gain insight into the prodigious star-forming activity that takes place in the very distant Un
Externí odkaz:
http://arxiv.org/abs/1709.00942
Autor:
Duras, F., Bongiorno, A., Piconcelli, E., Bianchi, S., Pappalardo, C., Valiante, R., Bischetti, M., Feruglio, C., Martocchia, S., Schneider, R., Vietri, G., Vignali, C., Zappacosta, L., La Franca, F., Fiore, F.
Studying the coupling between the energy output produced by the central quasar and the host galaxy is fundamental to fully understand galaxy evolution. Quasar feedback is indeed supposed to dramatically affect the galaxy properties by depositing larg
Externí odkaz:
http://arxiv.org/abs/1706.04214
Autor:
Privatus, P.1,2 (AUTHOR) privatuspius08@gmail.com, Pappalardo, C.3,4 (AUTHOR), Rao, P. V. K.1 (AUTHOR), Mazengo, D. T.1 (AUTHOR)
Publikováno v:
Astrophysics. Sep2023, Vol. 66 Issue 3, p311-323. 13p.