96 citations · 267 across the 8 of their papers we have counts for
7 papers · 1 filter
MIRACLE III. JWST/MIRI expose the hidden role of the AGN outflow in NGC 1068
C. Marconcini, A. Marconi, M. Ceci +27
We present new JWST IFS observations of the active galaxy NGC 1068, combining Mid-IR and optical IFS data from MIRI and MUSE to characterize the multi-phase circumnuclear gas prope…
Recovering the Dust Mass Budget with PRIMA
A. Traina, F. Pozzi, F. Calura +8
Achieving a complete picture of galaxy evolution is a primary goal of extragalactic astrophysics. To accomplish this ambitious task, a wealth of multi-wavelength surveys have been…
The IBISCO survey: I. Multiphase discs and winds in the Seyfert galaxy Markarian 509
M. V. Zanchettin, C. Feruglio, M. Bischetti +9
We present the analysis of the ALMA CO(2-1) emission line and the underlying 1.2 mm continuum of Mrk509 with spatial resolution of 270 pc. This local Seyfert 1.5 galaxy, optically…
Broad-band X-ray analysis of local mid-infrared selected Compton-thick AGN candidates
M. -M. La Caria, C. Vignali, G. Lanzuisi +2
The estimate of the number and space density of obscured AGN over cosmic time still represents an open issue. While the obscured AGN population is a key ingredient of the X-ray bac…
Feedback and feeding in the context of galaxy evolution with SPICA: direct characterization of molecular outflows and inflows
E. González-Alfonso, L. Armus, F. J. Carrera +28
A far-infrared observatory such as the {\it SPace Infrared telescope for Cosmology and Astrophysics} ({\it SPICA}), with its unprecedented spectroscopic sensitivity, would unveil t…
AGN vs. host galaxy properties in the COSMOS field
G. Lanzuisi, I. Delvecchio, S. Berta +13
The coeval AGN and galaxy evolution and the observed local relations between SMBHs and galaxy properties suggest some connection or feedback between SMBH growth and galaxy build-up…
Compton Thick AGN in the XMM-COSMOS survey
G. Lanzuisi, P. Ranalli, I. Georgantopoulos +27
Heavily obscured, Compton Thick (CT, NH>10^24 cm^-2) AGN may represent an important phase in AGN/galaxy co-evolution and are expected to provide a significant contribution to the c…