Zobrazeno 1 - 10
of 85
pro vyhledávání: '"D'Amato, Q."'
Autor:
Pozzi, F., Calura, F., D'Amato, Q., Gavarente, M., Bethermin, M., Boquien, M., Casasola, V., Cimatti, A., Cochrane, R., Dessauges-Zavadsky, M., Enia, A., Esposito, F., Faisst, A. L., Gilli, R., Ginolfi, M., Gobat, R., Gruppioni, C., Hayward, C. C., Ibar, E., Koekemoer, A. M., Lemaux, B. C., Magdis, G. E., Molina, J., Talia, M., Vallini, L., Vergani, D., Zamorani, G.
Publikováno v:
A&A 686, A187 (2024)
Measurements of the size of dust continuum emission are an important tool for constraining the spatial extent of star formation and hence the build-up of stellar mass. Compact dust emission has generally been observed at Cosmic Noon (z~2-3). However,
Externí odkaz:
http://arxiv.org/abs/2403.13490
Autor:
Ulivi, L., Venturi, G., Cresci, G., Marconi, A., Marconcini, C., Amiri, A., Belfiore, F., Bertola, E., Carniani, S., Amato, Q. D, Di Teodoro, E., Ginolfi, M., Girdhar, A., Harrison, C., Maiolino, R., Mannucci, F., Mingozzi, M., Perna, M., Scialpi, M., Tomicic, N., Tozzi, G., Treister, E.
Publikováno v:
A&A 685, A122 (2024)
An increasing number of observations and simulations suggests that low-power (<10$^{44}$ erg s$^{-1}$) jets may be a significant channel of feedback produced by active galactic nuclei (AGN), but little is known about their actual effect on their host
Externí odkaz:
http://arxiv.org/abs/2403.01258
Autor:
Marconi, A., Amiri, A., Feltre, A., Belfiore, F., Cresci, G., Curti, M., Mannucci, F., Bertola, E., Brazzini, M., Carniani, S., Cataldi, E., D'Amato, Q., de Rosa, G., Di Teodoro, E., Ginolfi, M., Kumari, N., Marconcini, C., Maiolino, R., Magrini, L., Marasco, A., Mingozzi, M., Moreschini, B., Nagao, T., Oliva, E., Scialpi, M., Tomicic, N., Tozzi, G., Ulivi, L., Venturi, G.
We present HOMERUN (Highly Optimized Multi-cloud Emission-line Ratios Using photo-ionizatioN), a new approach to modelling emission lines from photoionized gas that can simultaneously reproduce all observed line intensities from a wide range of ioniz
Externí odkaz:
http://arxiv.org/abs/2401.13028
Autor:
Scialpi, M., Mannucci, F., Marconcini, C., Venturi, G., Pancino, E., Marconi, A., Cresci, G., Belfiore, F., Amiri, A., Bertola, E., Carniani, S., Cicone, C., Ciurlo, A., D'Amato, Q., Ginolfi, M., Lusso, E., Marasco, A., Nardini, E., Rubinur, K., Severgnini, P., Tozzi, G., Ulivi, L., Vignali, C., Volonteri, M.
The novel Gaia Multi Peak (GMP) technique has proven to be able to successfully select dual and lensed AGN candidates at sub-arcsec separations. Both populations are important because dual AGN represent one of the central, still largely untested, pre
Externí odkaz:
http://arxiv.org/abs/2305.11850
Autor:
Perrotta, F., Giulietti, M., Massardi, M., Gandolfi, G., Ronconi, T., Zanchettin, M. V., D'Amato, Q., Behiri., M., Torsello, M., Gabrielli, F., Boco, L., Galluzzi, V., Lapi, A.
We report ALMA high-resolution observations of water emission lines $p-{\rm{H_2O}} (2_{02}-1_{11}$), $o-{\rm{H_2O}} (3_{21}-3_{12})$, $p-{\rm{H_2O}} (4_{22}-4_{13})$, in the strongly lensed galaxy HATLASJ113526.2-01460 at redshift z $\sim$ 3.1. From
Externí odkaz:
http://arxiv.org/abs/2304.08563
Autor:
Brienza, M., Gilli, R., Prandoni, I., D'Amato, Q., Rajpurohit, K., Calura, F., Chiaberge, M., Comastri, A., Iwasawa, K., Lanzuisi, G., Liuzzo, E., Marchesi, S., Mignoli, M., Miley, G., Norman, C., Peca, A., Raciti, M., Shimwell, T., Tozzi, P., Vignali, C., Vitello, F., Vito, F.
In the nearby universe jets from AGN are observed to have a dramatic impact on their surrounding extragalactic environment. Their effect at the `cosmic noon' (z>1.5), the epoch when star formation and AGN activity peak, is instead much less constrain
Externí odkaz:
http://arxiv.org/abs/2302.11977
Autor:
D'Amato, Q., Prandoni, I., Gilli, R., Vignali, C., Massardi, M., Liuzzo, E., Jagannathan, P., Brienza, M., Paladino, R., Mignoli, M., Marchesi, S., Peca, A., Chiaberge, M., Mazzolari, G., Norman, C.
Publikováno v:
A&A 668, A133 (2022)
We present deep L-Band observations of the equatorial field centered on the z=6.3 SDSS QSO, reaching a 1 sigma sensitivity of ~2.5 uJy at the center of the field. We extracted a catalog of 1489 radio sources down to a flux density of ~12.5 uJy (5 sig
Externí odkaz:
http://arxiv.org/abs/2210.15595
Autor:
Giulietti, M., Lapi, A., Massardi, M., Behiri, M., Torsello, M., D'Amato, Q., Ronconi, T., Perrotta, F., Bressan, A.
We present high-resolution ($\lesssim0.1$arcsec) ALMA observations of the strongly-lensed galaxy HATLASJ113526.2-01460 at redshift $z\sim3.1$ discovered in the Gama 12$^{\rm th}$ field of the Herschel-ATLAS survey. The gravitationally lensed system i
Externí odkaz:
http://arxiv.org/abs/2207.00466
Autor:
Gilli, R., Norman, C., Calura, F., Vito, F., Decarli, R., Marchesi, S., Iwasawa, K., Comastri, A., Lanzuisi, G., Pozzi, F., D'Amato, Q., Vignali, C., Brusa, M., Mignoli, M., Cox, P.
Publikováno v:
A&A 666, A17 (2022)
We combine results from deep ALMA observations of massive ($M_*>10^{10}\;M_{\odot}$) galaxies at different redshifts to show that the column density of their inter stellar medium (ISM) rapidly increases towards early cosmic epochs. Our analysis inclu
Externí odkaz:
http://arxiv.org/abs/2206.03508
Autor:
Enia, A., Talia, M., Pozzi, F., Cimatti, A., Delvecchio, I., Zamorani, G., D'Amato, Q., Bisigello, L., Gruppioni, C., Rodighiero, G., Calura, F., Dallacasa, D., Giulietti, M., Barchiesi, L., Behiri, M., Romano, M.
The Star Formation Rate Density (SFRD) history of the Universe is well constrained up to redshift $z \sim 2$. At earlier cosmic epochs, the picture has been largely inferred from UV-selected galaxies (e.g. Lyman-break galaxies, LBGs). However, LBGs'
Externí odkaz:
http://arxiv.org/abs/2202.00019