Zobrazeno 1 - 10
of 112
pro vyhledávání: '"Marconcini, C."'
Autor:
Marconcini, C., D'Eugenio, F., Maiolino, R., Arribas, S., Bunker, A., Carniani, S., Charlot, S., Perna, M., Del Pino, B. Rodríguez, Übler, H., Pérez-González, P. G., Willott, C. J., Böker, T., Cresci, G., Curti, M., Lamperti, I., Scholtz, J., Parlanti, E., Venturi, G.
We present JWST/NIRSpec integral field spectroscopic (IFS) observations of the \Lyalpha emitter CR7 at z ~ 6.6, observed as part of the GA-NIFS program. Using low-resolution PRISM (R ~ 100) data, we confirm a bright \Lyalpha emitter, and a diffuse \L
Externí odkaz:
http://arxiv.org/abs/2411.08627
Autor:
Scholtz, J., Curti, M., D'Eugenio, F., Übler, H., Maiolino, R., Marconcini, C., Smit, R., Perna, M., Witstok, J., Arribas, S., Böker, T., Bunker, A. J., Carniani, S., Charlot, S., Cresci, G., Pérez-González, P. G., Lamperti, I., Del Pino, B. Rodríguez, Parlanti, E., Venturi, G.
We present deep JWST/NIRSpec integral-field spectroscopy (IFS) and ALMA [CII]$\lambda$158$\mu$m observations of COS-3018, a star-forming galaxy at z$\sim$6.85, as part of the GA-NIFS programme. Both G395H (R$\sim$ 2700) and PRISM (R$\sim$ 100) NIRSpe
Externí odkaz:
http://arxiv.org/abs/2411.07695
Autor:
Ulivi, L., Perna, M., Lamperti, I., Arribas, S., Cresci, G., Marconcini, C., Del Pino, B. Rodríguez, Boeker, T., Bunker, A. J., Ceci, M., Charlot, S., Eugenio, F. D, Fahrion, K., Maiolino, R., Marconi, A., Pereira-Santaella, M.
The study of starburst and active galactic nuclei (AGN) feedback is crucial for understanding the regulation of star formation and the evolution of galaxies across cosmic time. Arp 220, the closest ultraluminous infrared galaxy (ULIRG), is in an adva
Externí odkaz:
http://arxiv.org/abs/2407.08505
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.
Publikováno v:
A&A 689, A78 (2024)
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
MOKA3D: An innovative approach to 3D gas kinematic modelling. I. Application to AGN ionized outflows
Autor:
Marconcini, C., Marconi, A., Cresci, G., Venturi, G., Ulivi, L., Mannucci, F., Belfiore, F., Tozzi, G., Ginolfi, M., Marasco, A., Carniani, S., Amiri, A., Di Teodoro, E., Scialpi, M., Tomicic, N., Mingozzi, M., Brazzini, M., Moreschini, B.
Publikováno v:
A&A 677, A58 (2023)
Studying the feedback process of Active Galactic Nuclei (AGN) requires characterising multiple kinematical components, such as rotating gas and stellar disks, outflows, inflows, and jets. To compare the observed properties with theoretical prediction
Externí odkaz:
http://arxiv.org/abs/2307.01854
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.
Publikováno v:
A&A 690, A57 (2024)
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:
Mannucci, F., Scialpi, M., Ciurlo, A., Yeh, S., Marconcini, C., Tozzi, G., Cresci, G., Marconi, A., Amiri, A., Belfiore, F., Carniani, S., Cicone, C., Nardini, E., Pancino, E., Rubinur, K., Severgnini, P., Ulivi, L., Venturi, G., Vignali, C., Volonteri, M., Pinna, E., Rossi, F., Puglisi, A., Agapito, G., Plantet, C., Ghose, E., Carbonaro, L., Xompero, M., Grani, P., Esposito, S., Power, J., Ramon, J. C. Guerra, Lefebvre, M., Cavallaro, A., Davies, R., Riccardi, A., Macintosh, M., Taylor, W., Dolci, M., Baruffolo, A., Feuchtgruber, H., Kravchenko, K., Rau, C., Sturm, E., Wiezorrek, E., Dallilar, Y., Kenworthy, M.
The Gaia-Multi-Peak (GMP) technique can be used to identify large numbers of dual or lensed AGN candidates at sub-arcsec separation, allowing us to study both multiple SMBHs in the same galaxy and rare, compact lensed systems. The observed samples ca
Externí odkaz:
http://arxiv.org/abs/2305.07396
Autor:
Ciurlo, A., Mannucci, F., Yeh, S., Amiri, A., Carniani, S., Cicone, C., Cresci, G., Khatun, R., Lusso, E., Marasco, A., Marconcini, C., Marconi, A., Nardini, E., Pancino, E., Rosati, P., Severgnini, P., Scialpi, M., Tozzi, G., Venturi, G., Vignali, C., Volonteri, M.
Publikováno v:
A&A 671, L4 (2023)
The existence of multiple active galactic nuclei (AGN) at small projected distances on the sky is due to either the presence of multiple, in-spiraling SMBHs, or to gravitational lensing of a single AGN. Both phenomena allow us to address important as
Externí odkaz:
http://arxiv.org/abs/2301.03091
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