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A new high-precision strong lensing model of the galaxy cluster MACS J0416.1-2403
Pietro Bergamini, Piero Rosati, Eros Vanzella +8
We present a new high-precision parametric strong lensing model of the galaxy cluster MACS J0416.1-2403, at z=0.396, which takes advantage of the MUSE Deep Lensed Field (MDLF), wit…
The MUSE Deep Lensed Field on the Hubble Frontier Field MACS~J0416
E. Vanzella, G. B. Caminha, P. Rosati +21
Context: A census of faint and tiny star forming complexes at high redshift is key to improving our understanding of reionizing sources, galaxy growth and the formation of globular…
Galaxy-scale ionised winds driven by ultra-fast outflows in two nearby quasars
A. Marasco, G. Cresci, E. Nardini +14
We use MUSE adaptive optics (AO) data in Narrow Field Mode to study the properties of the ionised gas in MR 2251-178 and PG 1126-041, two nearby (z~0.06) bright quasars hosting sub…
Discovery of molecular gas fueling galaxy growth in a protocluster at z=1.7
Q. D'Amato, R. Gilli, I. Prandoni +16
Based on ALMA Band 3 observations of the CO(2-1) line transition, we report the discovery of three new gas-rich (M_H2 ~ 1.5-4.8 x 10^10 M_sun, SFRs in the range ~5-100 M_sun/yr) ga…
Piercing through Highly Obscured and Compton-thick AGNs in the Chandra Deep Fields. II. Are Highly Obscured AGNs the Missing Link in the Merger-Triggered AGN-Galaxy Coevolution Models?
Junyao Li, Yongquan Xue, Mouyuan Sun +12
By using a large highly obscured () AGN sample (294 sources at ) selected from detailed X-ray spectral analyses in the deepest Chandra…
The XMM deep survey in the CDFS XI. X-ray properties of 185 bright sources
K. Iwasawa, A. Comastri, C. Vignali +11
We present X-ray spectra of 185 bright sources detected in the XMM-Newton deep survey of the Chandra Deep Field South, combining the three EPIC cameras. The 2-10 keV flux limit of…