most citedThe host galaxies of radio-loud quasars at z>5 with ALMA

8 citations · 8 across the 2 of their papers we have counts for

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astro-ph.GA2025

Infrared emission from quasar host galaxies: a direct estimate of dust physical properties

M. Costa, R. Decarli, F. Pozzi +6

Quasars at the dawn of Cosmic Time () are fundamental probes to investigate the early co-evolution of supermassive black holes and their host galaxy. Nevertheless, their infra…

astro-ph.GA2025

Discovery and characterization of 25 new quasars at 4.6 < z < 6.9 from wide-field multi-band surveys

Silvia Belladitta, Eduardo Bañados, Zhang-Liang Xie +18

Luminous quasars at provide key insights into the early Universe. Their rarity necessitates wide-field multi-band surveys to efficiently separate them from the main astrophys…

astro-ph.GA2025

Homogeneous measurements of proximity zone sizes for 59 quasars in the Epoch of Reionization

Silvia Onorato, Joseph F. Hennawi, Elia Pizzati +2

The overionized regions surrounding high-redshift quasars, known as proximity zones, provide a window into the interaction between supermassive black holes (SMBHs) and the intergal…

astro-ph.GA20248 cited

The host galaxies of radio-loud quasars at z>5 with ALMA

C. Mazzucchelli, R. Decarli, S. Belladitta +13

The interaction between radio-jets and quasar host galaxies plays a paramount role in quasar/galaxy co-evolution. However, very little has been known so far about this interaction…

astro-ph.GA2024

Characterizing the contribution of dust-obscured star formation at 5 using 18 serendipitously identified [CII] emitters

I. F. van Leeuwen, R. J. Bouwens, P. P. van der Werf +24

We present a new method to determine the star formation rate (SFR) density of the Universe at that includes the contribution of dust-obscured star formation. For this…