An extremely X--ray weak blazar at z=5
S. Belladitta, A. Moretti, A. Caccianiga, G. Ghisellini, C. Cicone, T., Sbarrato, L. Ighina, M. Pedani

TL;DR
This paper reports the discovery of DES0141-54, a high-redshift, radio-loud blazar with unusual X-ray weakness and a relatively small black hole, providing new insights into early Universe AGN properties.
Contribution
It presents the first high-redshift radio-loud AGN discovered in DES, highlighting its unique X-ray weakness and small black hole mass compared to similar objects.
Findings
First high-redshift radio-loud AGN in DES survey.
Unusually low X-ray luminosity for a blazar at z=5.
Hosts the smallest supermassive black hole at z≥5.
Abstract
We present the discovery and properties of DESJ014132.4-542749.9 (DES0141-54), a new powerful radio-loud active galactic nucleus (AGN) in the early Universe (z=5.0). It was discovered by cross-matching the first data release of the Dark Energy Survey (DES DR1) with the Sidney University Molonglo Survey (SUMSS) radio catalog at 0.843 GHz. This object is the first radio-loud AGN at high redshift discovered in the DES. The radio properties of DES0141-54, namely its very large radio-loudness (R>10), the high radio luminosity (L=1.7310 W Hz), and the flatness of the radio spectrum (=0.35) up to very high frequencies (120 GHz in the source's rest frame), classify this object as a blazar, meaning, a radio-loud AGN observed along the relativistic jet axis. However, the X--ray luminosity of DESJ0141-54 is much lower compared to those of the high…
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