Zobrazeno 1 - 10
of 10 333
pro vyhledávání: '"A. Bertola"'
Autor:
Bertola, E., Circosta, C., Ginolfi, M., Mainieri, V., Vignali, C., Rivera, G. Calistro, Ward, S. R., Lopez, I. E., Pensabene, A., Alexander, D. M., Bischetti, M., Brusa, M., Cappi, M., Comastri, A., Contursi, A., Cicone, C., Cresci, G., Dadina, M., D'Amato, Q., Feltre, A., Harrison, C. M., Kakkad, D., Lamperti, I., Lanzuisi, G., Mannucci, F., Marconi, A., Perna, M., Piconcelli, E., Puglisi, A., Ricci, F., Scholtz, J., Tozzi, G., Vietri, G., Zamorani, G., Zappacosta, L.
The energy released by AGN has the potential to heat or remove the gas of the ISM, thus likely impacting the cold molecular gas reservoir of host galaxies at first, with star formation following on longer timescales. Previous works on high-z galaxies
Externí odkaz:
http://arxiv.org/abs/2408.16821
Autor:
Bertola, Marco
We detail a numerical algorithm and related code to construct rational quadratic differentials on the Riemann sphere that satisfy the Boutroux condition. These differentials, in special cases, provide solutions of (generalized) Chebotarov problem as
Externí odkaz:
http://arxiv.org/abs/2408.15234
Autor:
Tozzi, G., Cresci, G., Perna, M., Mainieri, V., Mannucci, F., Marconi, A., Kakkad, D., Marasco, A., Brusa, M., Bertola, E., Bischetti, M., Carniani, S., Cicone, C., Circosta, C., Fiore, F., Feruglio, C., Harrison, C. M., Lamperti, I., Netzer, H., Piconcelli, E., Puglisi, A., Scholtz, J., Vietri, G., Vignali, C., Zamorani, G.
We present spatially resolved VLT/SINFONI spectroscopy with adaptive optics of type-2 active galactic nuclei (AGN) from the SINFONI Survey for Unveiling the Physics and Effect of Radiative feedback (SUPER), which targeted X-ray bright ($L_{2-10 keV}\
Externí odkaz:
http://arxiv.org/abs/2407.04099
Autor:
Lanzuisi, G., Matzeu, G., Baldini, P., Bertola, E., Comastri, A., Tombesi, F., Luminari, A., Braito, V., Reeves, J., Chartas, G., Bianchi, S., Brusa, M., Cresci, G., Nardini, E., Piconcelli, E., Zappacosta, L., Serafinelli, R., Gaspari, M., Gilli, R., Cappi, M., Dadina, M., Perna, M., Vignali, C., Veilleux, S.
IRASF11119 is an ultra-luminous IR galaxy with post-merger morphology, hosting a type-1 QSO at z=0.189. Its 2013 Suzaku spectrum shows a prominent Ultra Fast Outflow (UFO) absorption feature (v_out~0.25c). In 2021, we obtained the first XMM-Newton lo
Externí odkaz:
http://arxiv.org/abs/2406.12057
Autor:
Lamperti, Isabella, Arribas, Santiago, Perna, Michele, Del Pino, Bruno Rodríguez, Circosta, Chiara, Pérez-González, Pablo G., Bunker, Andrew J., Carniani, Stefano, Charlot, Stéphane, D'Eugenio, Francesco, Maiolino, Roberto, Übler, Hannah, Willott, Chris J., Bertola, Elena, Böker, Torsten, Cresci, Giovanni, Curti, Mirko, Jones, Gareth C., Kumari, Nimisha, Parlanti, Eleonora, Scholtz, Jan, Venturi, Giacomo
We present JWST NIRSpec observations in IFS mode of the galaxy GS5001 at redshift z=3.47, the brightest member of a candidate protocluster in the GOODS-S field. The data cover a field of view (FoV) of 4''$\times$4'' (~$30\times30$~kpc$^2$) and were o
Externí odkaz:
http://arxiv.org/abs/2406.10348
Autor:
Scholtz, Jan, D'Eugenio, Francesco, Maiolino, Roberto, Pérez-González, Pablo G., Circosta, Chiara, Tacchella, Sandro, Williams, Christina C., Alberts, Stacey, Arribas, Santiago, Baker, William M., Bertola, Elena, Bunker, Andrew J., Carniani, Stefano, Charlot, Stephane, Cresci, Giovanni, Jones, Gareth C., Kumari, Nimisha, Lamperti, Isabella, Looser, Tobias J., Del Pino, Bruno Rodríguez, Robertson, Brant, Parlanti, Eleonora, Perna, Michele, Übler, Hannah, Venturi, Giacomo, Witstok, Joris
JWST is discovering increasing numbers of quiescent galaxies 1--2 billion years after the Big Bang, whose redshift, high mass, and old stellar ages indicate that their formation and quenching were surprisingly rapid. This fast-paced evolution seems t
Externí odkaz:
http://arxiv.org/abs/2405.19401
Autor:
Maiolino, Roberto, Risaliti, Guido, Signorini, Matilde, Trefoloni, Bartolomeo, Juodzbalis, Ignas, Scholtz, Jan, Uebler, Hannah, D'Eugenio, Francesco, Carniani, Stefano, Fabian, Andy, Ji, Xihan, Mazzolari, Giovanni, Bertola, Elena, Brusa, Marcella, Bunker, Andrew J., Charlot, Stephane, Comastri, Andrea, Cresci, Giovanni, DeCoursey, Christa Noel, Egami, Eiichi, Fiore, Fabrizio, Gilli, Roberto, Perna, Michele, Tacchella, Sandro, Venturi, Giacomo
We investigate the X-ray properties of a large sample of 71 broad line and narrow line AGN at 2
Externí odkaz:
http://arxiv.org/abs/2405.00504
Autor:
López, I. E., Yang, G., Mountrichas, G., Brusa, M., Alexander, D. M., Baldi, R. D., Bertola, E., Bonoli, S., Comastri, A., Shankar, F., Acharya, N., Tetilla, A. V. Alonso, Lapi, A., Laloux, B., López, X. López, Rodríguez, I. Muñoz, Musiimenta, B., Clavijo, N. Osorio, Sala, L., Sengupta, D.
The spectral energy distribution (SED) of low-luminosity active galactic nuclei (LLAGN) presents unique challenges due to their comparable radiation output to their host galaxies and complex accretion dynamics. We introduce a novel module within the
Externí odkaz:
http://arxiv.org/abs/2404.16938
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:
Baldini, P., Lanzuisi, G., Brusa, M., Merloni, A., Gkimisi, K., Perna, M., Lopez, I. E., Bertola, E., Igo, Z., Waddell, S., Musiimenta, B., Aydar, C., Arcodia, R., Matzeu, G. A., Luminari, A., Buchner, J., Vignali, C., Dadina, M., Comastri, A., Cresci, G., Marchesi, S., Gilli, R., Tombesi, F., Serafinelli, R.
Publikováno v:
A&A 686, A217 (2024)
Powerful outflows from active galactic nuclei (AGN) can significantly impact the gas reservoirs of their host galaxies. However, it is still unclear how these outflows can propagate from the very central regions of galaxies to their outskirts, and wh
Externí odkaz:
http://arxiv.org/abs/2402.16966