Zobrazeno 1 - 10
of 97
pro vyhledávání: '"Duras F."'
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:
Travascio, A., Bongiorno, A., Tozzi, P., Fassbender, R., De Gasperin, F., Cardone, V. F., Zappacosta, L., Vietri, G., Merlin, E., Bischetti, M., Piconcelli, E., Duras, F., Fiore, F., Menci, N., Mazzotta, P., Nastasi, A.
Undisturbed galaxy clusters are characterized by a massive and large elliptical galaxy at their center, i.e. the Brightest Cluster Galaxy (BCG). How these central galaxies form is still debated. According to most models, a typical epoch for their ass
Externí odkaz:
http://arxiv.org/abs/2008.11132
Autor:
Zappacosta, L., Piconcelli, E., Giustini, M., Vietri, G., Duras, F., Miniutti, G., Bischetti, M., Bongiorno, A., Brusa, M., Chiaberge, M., Comastri, A., Feruglio, C., Luminari, A., Marconi, A., Ricci, C., Vignali, C., Fiore, F.
Publikováno v:
A&A 635, L5 (2020)
Hyperluminous quasars ($L_{\rm bol}\gtrsim 10^{47}$ erg s$^{-1}$) are ideal laboratories to study the interaction and impact of extreme radiative field and the most powerful winds in the AGN nuclear regions. They typically exhibit low coronal X-ray l
Externí odkaz:
http://arxiv.org/abs/2002.00957
Autor:
Duras, F., Bongiorno, A., Ricci, F., Piconcelli, E., Shankar, F., Lusso, E., Bianchi, S., Fiore, F., Maiolino, R., Marconi, A., Onori, F., Sani, E., Schneider, R., Vignali, C., La Franca, F.
Publikováno v:
A&A 636, A73 (2020)
The AGN bolometric correction is a key element to understand BH demographics and compute accurate BH accretion histories from AGN luminosities. However, current estimates still differ from each other by up to a factor of two to three, and rely on ext
Externí odkaz:
http://arxiv.org/abs/2001.09984
Autor:
Yang, Guang, Boquien, M., Buat, V., Burgarella, D., Ciesla, L., Duras, F., Stalevski, M., Brandt, W. N., Papovich, C.
Publikováno v:
Monthly Notices of the Royal Astronomical Society, Volume 491, Issue 1, January 2020, Pages 740-757
CIGALE is a powerful multiwavelength spectral energy distribution (SED) fitting code for extragalactic studies. However, the current version of CIGALE is not able to fit X-ray data, which often provide unique insights into AGN intrinsic power. We dev
Externí odkaz:
http://arxiv.org/abs/2001.08263
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:
Bruni, G., Piconcelli, E., Misawa, T., Zappacosta, L., Saturni, F. G., Vietri, G., Vignali, C., Bongiorno, A., Duras, F., Feruglio, C., Tombesi, F., Fiore, F.
The WISSH quasars project aims at studying the nuclear and host galaxy properties of the most luminous quasars ($L_{bol}>10^{47}$ erg/s, $1.8
Externí odkaz:
http://arxiv.org/abs/1908.09673
The hyperluminous Compton-thick $z\sim2$ quasar nucleus of the hot DOG W1835+4355 observed by NuSTAR
Autor:
Zappacosta, L., Piconcelli, E., Duras, F., Vignali, C., Valiante, R., Bianchi, S., Bongiorno, A., Fiore, F., Feruglio, C., Lanzuisi, G., Maiolino, R., Mathur, S., Miniutti, G., Ricci, C.
Publikováno v:
A&A 618, A28 (2018)
We present a 155ks NuSTAR observation of the $z\sim2$ hot dust-obscured galaxy (hot DOG) W1835+4355. We extracted spectra from the two NuSTAR detectors and analyzed them jointly with the archival XMM PN and MOS spectra. We performed a spectroscopic a
Externí odkaz:
http://arxiv.org/abs/1807.06022
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:
Vietri, G., Piconcelli, E., Bischetti, M., Duras, F., Martocchia, S., Bongiorno, A., Marconi, A., Zappacosta, L., Bisogni, S., Bruni, G., Brusa, M., Comastri, A., Cresci, G., Feruglio, C., Giallongo, E., La Franca, F., Mainieri, V., Mannucci, F., Ricci, F., Sani, E., Testa, V., Tombesi, F., Vignali, C., Fiore, F.
Publikováno v:
A&A 617, A81 (2018)
We have undertaken a multi-band observing program aimed at obtaining a complete census of winds in a sample of WISE/SDSS selected hyper-luminous (WISSH) QSOs at z~2-4. We have analyzed the rest-frame optical (LBT/LUCI and VLT/SINFONI) and UV (SDSS) s
Externí odkaz:
http://arxiv.org/abs/1802.03423