X-ray – Infrared relation of AGNs and search for highly obscured accretion in the AKARI NEP Field. (arXiv:1812.06208v1 [astro-ph.GA])
<a href="http://arxiv.org/find/astro-ph/1/au:+Miyaji_T/0/1/0/all/0/1">Takamitsu Miyaji</a> (Instituto de Astronom&#xed;a sede Ensenada, Universidad Nacional Aut&#xf3;noma de M&#xe9;xico), <a href="http://arxiv.org/find/astro-ph/1/au:+Team_AKARI_NEP_Survey/0/1/0/all/0/1">AKARI NEP Survey Team</a>

The infrared Astronomical Satellite AKARI conducted deep ($sim$ 0.4 deg$^2$)
and wide ($sim 5.4$ deg$^2$) surveys around the North Ecliptic Pole (NEP) with
its InfraRed Camera (IRC) with nine filters continuously covering the 2-25
$mu$m range. These photometric bands include three filters that fill the
Spitzer gap between the wavelength coverage with IRAC and MIPS instruments.
This unique feature has enabled us to make sensitive mid-infrared detection of
AGN candidates at z$sim$ 1-2, based on the Spectral Energy Distribution (SED)
fittings including hot dust emission in the AGN torus. This enables us to
compare X-rays and the AGN torus component of the infrared emission to help
identify highly absorbed AGNs, including Compton-thick ones. We report our
results of the {it Chandra} observation of the AKARI NEP Deep Field and
discuss the prospects for upcoming Spectrum-RG (eROSITA+ART-XC).

The infrared Astronomical Satellite AKARI conducted deep ($sim$ 0.4 deg$^2$)
and wide ($sim 5.4$ deg$^2$) surveys around the North Ecliptic Pole (NEP) with
its InfraRed Camera (IRC) with nine filters continuously covering the 2-25
$mu$m range. These photometric bands include three filters that fill the
Spitzer gap between the wavelength coverage with IRAC and MIPS instruments.
This unique feature has enabled us to make sensitive mid-infrared detection of
AGN candidates at z$sim$ 1-2, based on the Spectral Energy Distribution (SED)
fittings including hot dust emission in the AGN torus. This enables us to
compare X-rays and the AGN torus component of the infrared emission to help
identify highly absorbed AGNs, including Compton-thick ones. We report our
results of the {it Chandra} observation of the AKARI NEP Deep Field and
discuss the prospects for upcoming Spectrum-RG (eROSITA+ART-XC).

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