activity
19952023
most citedThe Chandra Deep Field South: the 1 Million Second

614 citations · 7.9k across the 95 of their papers we have counts for

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Showing 2020 · astro-ph.GAShow all

7 papers · 2 filters

astro-ph.GA2020★ 48 cited

The web of the Giant: spectroscopic confirmation of a Large Scale Structure around the z=6.31 quasar SDSS J1030+0524

Marco Mignoli, Roberto Gilli, Roberto Decarli +14

We report on the spectroscopic confirmation of a large scale structure around the luminous, z=6.31 QSO SDSS~J1030+0524, that is powered by a billion solar mass black hole. The stru…

astro-ph.GA2020

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…

astro-ph.GA2020★ 11 cited

Multiphase Circumnuclear Gas in a Low- Disk: Turbulence and Magnetic Field Reversals

Yuki Kudoh, Keiichi Wada, Colin Norman

We studied the magnetic field structures and dynamics of magnetized multiphase gas on parsec scales around supermassive black holes by using global 3D magnetohydrodynamics (MHD) si…

astro-ph.GA2020★ 13 cited

A systematic study of galactic outflows via fluorescence emission: implications for their size and structure

Bingjie Wang, Timothy M. Heckman, Guangtun Zhu +1

Galactic outflows play a major role in the evolution of galaxies, but the underlying physical processes are poorly understood. This is mainly because we have little information abo…

astro-ph.GA2020★ 21 cited

The deep Chandra survey in the SDSS J1030+0524 field

R. Nanni, R. Gilli, C. Vignali +18

We present the X-ray source catalog for the 479 ks Chandra exposure of the SDSS J1030+0524 field, that is centered on a region that shows the best evidence to date of an overdensit…

astro-ph.GA2020★ 49 cited

Dust and gas content of high-redshift galaxies hosting obscured AGN in the CDF-S

Q. D'Amato, R. Gilli, C. Vignali +14

Obscured AGN represent a significant fraction of the entire AGN population, especially at high redshift (~70% at z=3--5). They are often characterized by the presence of large gas…