Fabrizio Fiore
Fabrizio Fiore
Verified email at - Homepage
Cited by
Cited by
Discovery of an X-ray afterglow associated with the γ-ray burst of 28 February 1997
E Costa, F Frontera, J Heise, M Feroci, J In't Zand, F Fiore, MN Cinti, ...
Nature 387 (6635), 783-785, 1997
Massive molecular outflows and evidence for AGN feedback from CO observations
C Cicone, R Maiolino, E Sturm, J Graciá-Carpio, C Feruglio, R Neri, ...
arXiv preprint arXiv:1311.2595, 2013
The soft X-ray properties of a complete sample of optically selected quasars. II. Final results
A Laor, F Fiore, M Elvis, BJ Wilkes, JC McDowell
The Astrophysical Journal 477 (1), 93, 1997
Broadband observations of the naked-eye γ-ray burst GRB 080319B
JL Racusin, SV Karpov, M Sokolowski, J Granot, XF Wu, V Pal’Shin, ...
Nature 455 (7210), 183-188, 2008
GRB 090423 at a redshift of z ≈ 8.1
R Salvaterra, MD Valle, S Campana, G Chincarini, S Covino, P D’avanzo, ...
Nature 461 (7268), 1258-1260, 2009
Quasar feedback revealed by giant molecular outflows
C Feruglio, R Maiolino, E Piconcelli, N Menci, H Aussel, A Lamastra, ...
arXiv preprint arXiv:1006.1655, 2010
The Chandra COSMOS survey. I. Overview and point source catalog
M Elvis, F Civano, C Vignali, S Puccetti, F Fiore, N Cappelluti, TL Aldcroft, ...
The Astrophysical Journal Supplement Series 184 (1), 158, 2009
SN 2003lw and GRB 031203: A bright supernova for a faint gamma-ray burst
D Malesani, G Tagliaferri, G Chincarini, S Covino, M Della Valle, ...
The Astrophysical Journal 609 (1), L5, 2004
The HELLAS2XMM survey. VII. The hard X-ray luminosity function of AGNs up to z= 4: More absorbed AGNs at low luminosities and high redshifts
F La Franca, F Fiore, A Comastri, GC Perola, N Sacchi, M Brusa, ...
The Astrophysical Journal 635 (2), 864, 2005
Evidence of strong quasar feedback in the early Universe
R Maiolino, S Gallerani, R Neri, C Cicone, A Ferrara, R Genzel, D Lutz, ...
Monthly Notices of the Royal Astronomical Society: Letters 425 (1), L66-L70, 2012
AGN wind scaling relations and the co-evolution of black holes and galaxies
F Fiore, C Feruglio, F Shankar, M Bischetti, A Bongiorno, M Brusa, ...
arXiv preprint arXiv:1702.04507, 2017
The Chandra COSMOS Legacy survey: overview and point source catalog
F Civano, S Marchesi, A Comastri, MC Urry, M Elvis, N Cappelluti, ...
The Astrophysical Journal 819 (1), 62, 2016
The Athena x-ray integral field unit (X-IFU)
D Barret, TL Trong, JW Den Herder, L Piro, X Barcons, J Huovelin, ...
Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray 9905 …, 2016
UBVRI light curves of 44 type Ia supernovae
S Jha, RP Kirshner, P Challis, PM Garnavich, T Matheson, AM Soderberg, ...
The Astronomical Journal 131 (1), 527, 2006
Star formation and mass assembly in high redshift galaxies
P Santini, A Fontana, A Grazian, S Salimbeni, F Fiore, F Fontanot, ...
arXiv preprint arXiv:0905.0683, 2009
The XMM-Newton wide-field survey in the COSMOS field. I. Survey description
G Hasinger, N Cappelluti, H Brunner, M Brusa, A Comastri, M Elvis, ...
The Astrophysical Journal Supplement Series 172 (1), 29, 2007
The X-ray to optical-UV luminosity ratio of X-ray selected type 1 AGN in XMM-COSMOS
E Lusso, A Comastri, C Vignali, G Zamorani, M Brusa, R Gilli, K Iwasawa, ...
arXiv preprint arXiv:0912.4166, 2009
The XMM-Newton wide-field survey in the cosmos field (XMM-COSMOS): demography and multiwavelength properties of obscured and unobscured luminous active galactic nuclei
M Brusa, F Civano, A Comastri, T Miyaji, M Salvato, G Zamorani, ...
The Astrophysical Journal 716 (1), 348, 2010
On the cosmic evolution of the scaling relations between black holes and their host galaxies: broad-line active galactic nuclei in the zCOSMOS survey
A Merloni, A Bongiorno, M Bolzonella, M Brusa, F Civano, A Comastri, ...
The Astrophysical Journal 708 (1), 137, 2009
Faint AGNs at z> 4 in the CANDELS GOODS-S field: looking for contributors to the reionization of the Universe
E Giallongo, A Grazian, F Fiore, A Fontana, L Pentericci, E Vanzella, ...
arXiv preprint arXiv:1502.02562, 2015
The system can't perform the operation now. Try again later.
Articles 1–20