activity
19992026
most citedThe synthesis of the cosmic X-ray background in the Chandra and XMM-Newton era

929 citations · 4.2k across the 88 of their papers we have counts for

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Showing 2023Show all

10 papers · 1 filter

astro-ph.IM20231 cited

AGN in overdense environments at high- with AXIS

Fabio Vito, Paolo Tozzi, Roberto Gilli +3

Overdense regions at high redshift () are perfect laboratories to study the relations between environment and SMBH growth, and the AGN feedback processes on the surrou…

astro-ph.GA2023

An extremely metal poor star complex in the reionization era: Approaching Population III stars with JWST

E. Vanzella, F. Loiacono, P. Bergamini +31

We present JWST/NIRSpec integral field spectroscopy (IFS) of a lensed Population III candidate stellar complex (dubbed Lensed And Pristine 1, LAP1), with a lensing-corrected stella…

astro-ph.HE2023

X-ray properties and obscured fraction of AGN in the J1030 Chandra field

Matilde Signorini, Stefano Marchesi, Roberto Gilli +13

The 500ks Chandra ACIS-I observation of the field around the quasar SDSS J1030+0524 is currently the 5th deepest extragalactic X-ray survey. The rich multi-band coverage o…

astro-ph.GA2023

Compton-thick AGN in the NuSTAR Era X: Analysing seven local CT-AGN candidates

Dhrubojyoti Sengupta, Stefano Marchesi, Cristian Vignali +14

We present the broad-band X-ray spectral analysis (0.6-50 keV) of seven Compton-Thick active galactic nuclei (CT-AGN; line-of-sight, l.o.s., column density cm) ca…

astro-ph.GA20233 cited

The most luminous blue quasars at 3.0<z<3.3 -- III. LBT spectra and accretion parameters

Bartolomeo Trefoloni, Elisabeta Lusso, Emanuele Nardini +13

We present the analysis of the rest frame ultraviolet and optical spectra of 30 bright blue quasars at , selected to examine the suitability of AGN as cosmological probes.…

astro-ph.GA2023

HYPerluminous quasars at the Epoch of ReionizatION (HYPERION). A new regime for the X-ray nuclear properties of the first quasars

L. Zappacosta, E. Piconcelli, F. Fiore +40

The existence of luminous quasars (QSO) at the Epoch of Reionization (EoR; i.e. z>6) powered by supermassive black holes (SMBH) with masses challenges models…